Ecology of chaetognaths (semi-gelatinous zooplankton) in Arctic waters
Thèse
Jordan Grigor
Doctorat interuniversitaire en océanographie
Philosophiæ doctor (Ph. D.)
Québec, Canada
© Jordan Grigor, 2017
Ecology of chaetognaths (semi-gelatinous zooplankton) in Arctic waters
Thèse
Jordan Grigor
Sous la direction de :
Louis Fortier, directeur de recherche
iii
Résumé
Les chaetognathes sont d’importants membres des communautés mésozooplanctoniques de
l’Arctique en ce qui a trait à l'abondance et à la biomasse. Les chaetognathes de l’Arctique
se répartissent en trois espèces principales qui sont considérées comme étant strictement
carnivores : Eukrohnia hamata, Parasagitta elegans et Pseudosagitta maxima. Cette étude
utilise un ensemble de données de filet planctoniques recueillies sur une période de 5 ans
dans les régions européennes, canadiennes et de l'Alaska de l’Arctique (2007, 2008, 2012,
2013, 2014) et comprend un cycle annuel complet dans l'Arctique canadien (2007-2008), le
but étant d’améliorer notre compréhension sur les distributions, les cycles de vie et les
stratégies d'alimentation du E. hamata et du P. elegans. Dans la présente thèse, les points
suivants seront abordés : (1) la stratégie d'alimentation et la maturité du P. elegans dans
l'Arctique européen durant la nuit polaire en 2012 et 2013, (2) les cycles de croissance et de
reproduction, les stratégies d'alimentation et les distributions verticales du E. hamata et du
P. elegans dans l'Arctique canadien de 2007 à 2008, et (3) les différences spatiales dans les
stratégies d'alimentation du E. hamata et du P. elegans à l'automne 2014. Afin d’étudier leurs
stratégies d'alimentation, des analyses de contenu du tube digestif ainsi que des techniques
biochimiques ont été utilisées. Dans l'Arctique canadien, le E. hamata et le P. elegans vivent
tous deux pendant environ 2 ans. Le P. elegans colonise principalement les eaux
épipélagiques, tandis que le E. hamata colonise principalement les eaux mésopélagiques.
Dans cette région, P. elegans se reproduit en continue de l'été au début de l'hiver, dans la
période de forte biomasse de copépodes, qui constituent ses proies, dans les eaux proches de
la surface, un mode de reproduction basé sur l’apport immédiat d’énergie. Cependant, les
résultats ont révélé que E. hamata a engendré des couvées distinctes dont on peut voir
l’évolution au cours de fenêtres de reproduction séparées, à la fois durant les périodes de
printemps-été et d’automne-hiver, ce qui suggère une reproduction basée sur les réserves.
Les taux de prédation quotidiens évalués à partir des analyses du contenu du tube digestif
sont généralement restés faibles pour les deux espèces de chaetognathes. Toutefois, pour E.
hamata et P. elegans, les taux de prédation inférés en été-automne ont dépassé ceux de
l’hiver-printemps. Des études d’alimentation ont révélé que E. hamata consomme de la
matière organique particulaire (éventuellement des chutes de neige marine) tout au long de
l'année, mais surtout en été, alors que le P. elegans se nourrit différemment. Les deux espèces
iv
sont caractérisées par une forte croissance estivale. La croissance hivernale du P. elegans
était grandement restreinte, tandis que celle du E hamata l’était moindrement. En somme, les
différences dans la façon dont les lipides et la neige marine sont utilisés par les deux espèces
pourraient expliquer les différences dans leurs cycles de reproduction et leurs patrons de
croissance saisonnière.
v
Abstract
Chaetognaths are important members of Arctic mesozooplankton communities in terms of
abundance and biomass. Despite this, the bulk of seasonal studies have focused on grazing
copepods. Arctic chaetognaths comprise three major species which are thought to be strict
carnivores: Eukrohnia hamata, Parasagitta elegans and Pseudosagitta maxima. This thesis
uses datasets collected from plankton net sampling during five years in European, Canadian
and Alaskan areas of the Arctic (2007, 2008, 2012, 2013, 2014) and includes a full annual
cycle in the Canadian Arctic (2007-2008), the purpose being to improve our understanding
of the distributions, life history and feeding strategies of E. hamata and P. elegans. The
following topics are addressed: (1) the feeding strategy and maturity of P. elegans in the
European Arctic during the polar night in 2012 and 2013; (2) the growth, breeding cycles,
feeding strategies and vertical distributions of E. hamata and P. elegans, in the Canadian
Arctic from 2007 to 2008; and (3) spatial differences in the feeding strategies of E. hamata
and P. elegans in autumn 2014. To investigate feeding strategies, a combination of gut
contents and biochemical techniques was used. In the Canadian Arctic, both E. hamata and
P. elegans live for around 2 years. P. elegans mainly colonized epi-pelagic waters, whereas
E. hamata mainly colonized meso-pelagic waters. In this region, P. elegans reproduced
continuously from summer to early winter when copepod prey peak in near-surface waters.
This is characteristic of income breeders. However, results for E. hamata revealed that this
species spawned distinct and traceable broods during separate reproductive windows in both
spring-summer and autumn-winter, suggesting capital breeding. Daily predation rates
inferred from gut content analyses appeared to be generally low in the two chaetognath
species, though inferred predation rates in summer-autumn exceeded those in winter-spring.
Feeding studies revealed that E. hamata consumed particulate organic matter (possibly
falling marine snow) throughout the year but especially in the summer, whereas P. elegans
did not feed in this way. High summer growth seems to be a characteristic of both these
species. Growth during winter was highly restricted in P. elegans, to a lesser extent in E.
hamata. In summary, differences in how lipids and marine snow are utilised by the two
species could explain differences in their breeding cycles and seasonal growth patterns.
vi
Table of contents
Résumé iii
Abstract v
Acknowledgements xviii
Foreword xx
1. Chapter 1 – General Introduction 1
1.1 The Arctic Ocean 1
1.1.1 Physical environment 2
1.1.2 Arctic marine ecosystems 3
1.2 Zooplankton and their polar adaptations 5
1.3 Chaetognaths 8
1.3.1 Arctic species and distributions 9
1.3.2 Lifespans 10
1.3.3 Reproductive strategy 11
1.3.4 Oil vacuoles in Eukrohnia spp. 11
1.3.5 Feeding strategies and trophic importance 12
1.3.6 Fatty acids and stable isotopes 14
1.4 Climate change and other challenges for Arctic marine life 14
1.5 Study areas 17
1.6 Aims and objectives 18
2. Chapter 2 – Polar night ecology of a pelagic predator, the chaetognath Parasagitta elegans
20
2.1 Résumé 20
2.2 Abstract 21
2.3 Introduction 22
2.4 Method 23
2.4.1 Study area 23
2.4.2 Physical and biological environment 24
2.4.3 Zooplankton sampling 24
2.4.4 Sample processing 25
2.4.5 Gut content analyses 26
2.4.6 Food-containing ratio and feeding rate 26
2.4.7 Stable isotope analyses 27
2.4.8 Determination of trophic level 28
2.4.9 Fatty acid analyses 28
2.4.10 Mid-winter maturity status 29
2.5 Results 30
2.5.1 Chaetognath abundance and prey field 30
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2.5.2 Gut contents 32
2.5.3 Body composition 34
2.5.4 Mid-winter maturity status 36
2.6 Discussion 36
2.6.1 Studies during the polar night 36
2.6.2 Feeding activity and rates 36
2.6.3 Energetics 38
2.6.4 Lipid profile 38
2.6.5 Reproduction 40
2.7 Concluding remarks 41
3. Chapter 3 – Growth and reproduction of the chaetognaths Eukrohnia hamata and
Parasagitta elegans in the Canadian Arctic Ocean: capital breeding versus income breeding
42
3.1 Résumé 42
3.2 Abstract 43
3.3 Introduction 44
3.4 Method 46
3.4.1 Study area 46
3.4.2 Sampling 47
3.4.3 Chaetognath body size and sampler efficiency 48
3.4.4 Hatching and cohort development 49
3.4.5 Estimation of maturity and oil vacuole area 50
3.4.6 Vertical distributions 50
3.5 Results 51
3.5.1 Physical environment and primary production in the Amundsen Gulf 51
3.5.2 Physical environment and primary production in autumn (other sampling
locations) 51
3.5.3 Abundances and vertical distributions of chaetognath species 52
3.5.4 Length distributions and sampler efficiency 53
3.5.5 Timing of reproduction 54
3.5.6 Eukrohnia hamata length cohorts and life cycle 55
3.5.7 Parasagitta elegans length cohorts and life cycle 62
3.6 Discussion 67
3.6.1 Chaetognath cohort interpretation and lifespans 67
3.6.2 Resource partitioning in the sympatric Eukrohnia hamata and Parasagitta elegans
67
3.6.3 The potential role of lipid reserves: contrasting growth in the two species 69
3.6.4 Maturation 71
3.6.5 Capital versus income breeding in a warming Arctic 72
3.7 Conclusions 73
4. Chapter 4 – Feeding strategies of arctic chaetognaths: are they really “tigers of the
plankton”? 74
viii
4.1 Résumé 74
4.2 Abstract 75
4.3 Introduction 76
4.4 Method 77
4.4.1 Study areas 77
4.4.2 Sampling in the Amundsen Gulf 79
4.4.3 Sampling in the Chukchi Sea and Baffin Bay 80
4.4.4 Abundance of zooplankton 80
4.4.5 Gut contents 81
4.4.6 Fatty acids 82
4.4.7 Carbon and nitrogen 82
4.5 Results 84
4.5.1 Amundsen Gulf 84
4.5.1.1 Phenology of algae blooms 84
4.5.1.2 Zooplankton community 84
4.5.1.3 Visible prey items and predation rates 86
4.5.1.4 Lipid droplets and detritus 87
4.5.1.5 Scanning Electron Microscope observations 89
4.5.2 Chukchi Sea and Baffin Bay 90
4.5.2.1 In-vitro feeding observations 90
4.5.2.2 Lipid amounts 90
4.5.2.3 Fatty acid profiles: species differences 91
4.5.2.4 Fatty acid profiles: station and regional differences in Eukrohnia hamata and
Parasagitta elegans 91
4.5.2.5 Carbon and nitrogen isotopes 94
4.6 Discussion 96
4.6.1 Prey items 96
4.6.2 Predation rates 97
4.6.3 Omnivory in arctic chaetognaths 98
4.6.4 Fatty acids and stable isotopes confirm gut contents 99
4.6.4.1 18:1 (n-9)/(n-7) ratios and Calanus copepod FATMs 99
4.6.4.2 Algal FATMs 100
4.6.4.3 δ13C values 100
4.6.4.4 δ15N values and inferred TLs 101
4.6.4.5 C/N ratios 101
4.6.5 Morphological explanations 102
4.7 Concluding remarks and future studies 102
5. Chapter 5 – General Conclusions 103
5.1 Resource use by arctic chaetognaths 103
5.2 Winter ecology in Svalbard 103
5.3 Life histories, habitats and spawning times 104
5.4 Food resources 105
5.5 Limitations of the study 107
5.5.1 Sampling limitations 107
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5.5.2 Stable isotopes and trophic levels 107
5.5.3 Length cohorts 108
5.6 Future research avenues 108
5.7 A note on climate change 109
Bibliography 110
Appendix A. Information on the zooplankton samples included in Chapter 2 126
Appendix B. Vertical profiles of temperature and salinity in Chapter 2 128
Appendix C. Stations sampled in Chapter 3 129
Appendix D. Vertical profiles of temperature, salinity and chlorophyll a in Chapter 3 131
Appendix E-1. Amundsen Gulf stations sampled in Chapter 4 132
Appendix E-2. Chukchi Sea and Baffin Bay stations sampled in Chapter 4 136
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List of tables
Table 2.1 Total water-column abundances (ind. m-3) of a polar night zooplankton community
(Rijpfjorden 2012), ordered according to abundance per taxonomic group. Net sampling
(Multi-Plankton Sampler; 0.25-m2 opening, 0.2-mm mesh) was used. As larger
chaetognaths may have avoided the smaller MPS net (see Grigor et al. 2014),
chaetognath abundances presented here are likely to be underestimates. Mean
abundances for species and copepod stages were first calculated over two hauls (one at
midday and the other at midnight at various depth intervals, see Appendix A), and data
were summed across all sampling depths. Copepod stages are CI-CV, AM (adult male)
and AF (adult female). Functional (feeding) groups were extracted from Søreide et al.
(2003). “Small Calanoida” comprised the following taxa: Acartia longiremis, Aetideidae
CI-CIII, Bradyidius similis, Microcalanus spp. and Pseudocalanus spp. Only taxa with
abundances of ≥0.1 ind. m-3 are shown. 31
Table 2.2 Stable carbon and nitrogen isotope values for Parasagitta elegans sampled by the
MIK (3.14-m2 opening, 1.5-mm mesh) at various trawl depths (20, 30, 35, 60, 75 and
225 m) in Isfjorden and Rijpfjorden (2012). The average δ13C and δ15N composition (‰)
in replicate samples (usually three but six from 225 m in Rijpfjorden) containing 25
pooled individuals (10-50 mm), average proportions of animal dry weight (DW)
comprising carbon and nitrogen (%), and C/N weight ratios. All values are accompanied
by standard deviations. Trophic levels (TL) were calculated for P. elegans from each
fjord from mean δ15N (‰) values (see ‘Method’). 34
Table 2.3 Average fatty acid profile for Parasagitta elegans in 2012. Results are given as
average percentages of the various fatty acids identified across all samples from
Isfjorden and Rijpfjorden (see ‘Method’), alongside the standard deviations. Only fatty
acids with mean percentages of =>0.5 ± 0.1 across both fjords are shown. In Isfjorden,
the mean percentages of 15:0 FA and 18.2(n-6) FA differed between sampling depths
(indicated by a † symbol, one-way ANOVA, P ˂ 0.05). In Rijpfjorden, the proportion of
every fatty acid was similar between sampling depths (one-way ANOVA, P ˃ 0.05). 35
Table 3.1 Timing of peak development of maturity features in autumn and spring broods of
Eukrohnia hamata and summer brood of Parasagitta elegans, and of the oil vacuole in
E. hamata. Ages in months at peak development are given in parentheses. Monthly
collections consisted of up to 397 and 434 E. hamata individuals from its autumn and
spring broods respectively, and 177 P. elegans. 59
Table 4.1 Composition of the mesozooplankton (30 most abundant taxa) sampled in the
Amundsen Gulf from November 2007 to July 2008, based on data from 70 Multinet
hauls. *Taxa could not be identified to species level. 85
Table 4.2 Frequency of first- and second-year Eukrohnia hamata individuals with green lipid
droplets or macroaggregates in guts. Separate results are presented for the autumn
(October) and spring (April) broods of E. hamata (see Chapter 3), from approximate
month of hatching (no gut content data were available for October). 88
xi
Table 4.3 Mean sample lipid, fatty acid amounts and fatty acid proportions (± 1 SD) in (a)
Eukrohnia hamata and (b) Parasagitta elegans at different stations (stns) in autumn
2014. Sampling locations are abbreviated: CS, Chukchi Sea; SIF, Scott Inlet Fjord; GF,
Gibbs Fjord; SBB, southern Baffin Bay. Also: number (n) of samples analysed and
chaetognaths per sample, and chaetognath body lengths in mm. † Significant species
differences (P ≤ 0.05). 92
Table 4.4 Mean sample carbon (C) and nitrogen (N) masses, C/N ratios, δ13C and δ15N values
and derived trophic levels (TLs) (± 1 SD) in Eukrohnia hamata and Parasagitta elegans
at different stations in autumn 2014. Sampling locations are abbreviated: CS, Chukchi
Sea; SIF, Scott Inlet Fjord; GF, Gibbs Fjord; SBB, southern Baffin Bay. Also: number
(n) of samples analysed and chaetognaths per sample, as well as body lengths of
chaetognaths in mm. 95
xii
List of figures
Figure 1.1 Bathymetric map of the central Arctic Ocean and several marginal seas
(http://recherchespolaires.inist.fr/?L-ocean-Arctique-physiographie). 1
Figure 1.2 Water masses in the Arctic Ocean. Reproduced from Stein & Macdonald (2004).2
Figure 1.3 The planktonic food web showing protozoan and metazoan consumers at arrow
caps. Adapted from Hopcroft et al. (2008). 4
Figure 1.4 Photographs of living holo-zooplankton captured in-situ by a zooplankton imager
(Lightframe On-sight Key Species Investigation System; Schmid et al. 2016), during
deployments in the Canadian Arctic (summer 2014). 6
Figure 1.5 Typical physiology of a chaetognath belonging to the family Sagittidae.
Reproduced from Margulis & Chapman (2010). 8
Figure 1.6 Photographs of the heads and the bodies of the major arctic chaetognaths. (a)
Eukrohnia hamata with characteristic marsupial sac and oil vacuole, (b) and (c)
Parasagitta elegans and Pseudosagitta maxima without marsupial sacs and oil vacuoles.
All images except P. maxima head from:
http://www.arcodiv.org/watercolumn/Chaetognaths.html (courtesy of Russ Hopcroft). 9
Figure 1.7 Photograph of a chaetognath’s head taken by Scanning Electron Microscopy (left)
with parts labelled (right). Reproduced from Bieri & Thuesen (1990). 12
Figure 1.8 Diagram illustrating the wide variety of sampling activities conducted during the
Circumpolar Flaw Lead System Study (2007-2008) from the icebreaker CCGS
Amundsen and at an ice camp, in order to study Arctic systems. Reproduced from Barber
et al. (2010). 18
Figure 2.1 Map showing the locations of the stations sampled for chaetognaths in January
2012 and 2013. 24
Figure 2.2 Proportions (%) of Parasagitta elegans individuals per haul with gut contents
(FCRmax), identifiable prey (FCRmin), and empty guts in each fjord. The horizontal line
inside each boxplot shows the median of the proportions over multiple haul samples in
a fjord. The lower and upper boxes show the lower and upper quartiles, respectively, and
the vertical lines outside the boxes the differences between these quartiles and the lowest
and highest proportions observed. Each dot represents an outlying data point. nhauls =
numbers of hauls for each fjord. Hauls with ˂3 individuals analysed were not included.
As only one haul was analysed for Rijpfjorden in 2013, full boxplots could not be shown.
See Appendix A for numbers of individuals analysed per haul. 32
xiii
Figure 2.3 Proportions (%) of feeding Parasagitta elegans individuals per haul in each fjord
with different types of gut content. For details on the features of the boxplots and the
data, see Figure 2.2. 33
Figure 2.4 Gut contents in ascending head width size classes: proportions of Parasagitta
elegans (%) per haul with gut contents and of feeders with each gut content type.
Includes all dissected specimens from Isfjorden (50 individuals, 4 hauls) and Rijpfjorden
(152 individuals, 13 hauls) in 2012. For details on the features of the boxplots and the
data, see Figure 2.2. ninds. = total numbers of individuals for each size class. 33
Figure 3.1 Bathymetric maps of the Canadian Arctic Ocean indicating the regions, and
positions of stations (black circles) where chaetognaths were sampled from August 2007
to September 2008. Station IDs provided. 47
Figure 3.2 Illustrations and photographs of Eukrohnia hamata and Parasagitta elegans. (a)
Diagrams of the two species indicating maturity features and the centrally-positioned oil
vacuole in E. hamata. (b) Photographs of live E. hamata (top) and P. elegans (bottom)
taken in-situ by a zooplankton imager (Schmid et al. 2016) in the Canadian Arctic.
Specimens ~20 mm. (c) Photograph of oocytes in a stained P. elegans individual. (d)
Photograph of ovaries in an E. hamata individual (imaged in-situ). (e) Photograph of tail
sperm, seminal vesicles and seminal receptacles in a stained P. elegans individual. 49
Figure 3.3 Relative frequency of Eukrohnia hamata, Parasagitta elegans and Pseudosagitta
maxima in relation to bottom depth at Amundsen Gulf stations. Multinet and square-
conical net collections included. b) Weighted mean depths of E. hamata and P. elegans
normalized relative to the bottom depth at Amundsen Gulf stations (see ‘Method’).
Multinet collections. Standard deviation bars also given. The blue area indicates the
Pacific Halocline (60-200 m) and the red area indicates the Atlantic Layer ˃ 200 m
(Geoffroy et al. 2011). 53
Figure 3.4 Length frequency (mean % ± 1 SD) distributions of Eukrohnia hamata and
Parasagitta elegans in the square-conical (S-C) net (1 m2 aperture, 200 µm mesh) and
Multinet (0.5 m2 aperture, 200 µm mesh) in the Amundsen Gulf. Note the different scales
for the two species. k is the number of collections. 54
Figure 3.5 Abundance (mean numbers m-2 + 1 SD) of newborn Eukrohnia hamata and
Parasagitta elegans (body lengths of 2-4 mm) in monthly Multinet deployments from
October to September. August 2007 was inserted between July and September 2008 to
provide a complete composite of the annual cycle. Number of collections shown above
bars. The solid horizontal bar above month labels indicates sampling in the Amundsen
Gulf. 55
Figure 3.6 Monthly length frequency distributions of Eukrohnia hamata. Frequencies of
newborns highlighted in orange. Visually identified length cohorts shown as normal
distributions (in red) with red dots indicating the mean length. Each of the five cohorts
is labelled with a capital E and a number from oldest (1) to youngest (5). Blue line is the
xiv
total distribution obtained by summing the modelled distributions. Chi-square values for
the goodness-of-fit of the total distribution to the data are given. Sampling regions are
abbreviated in each panel: PC, Parry Channel; AG, Amundsen Gulf; BB, Baffin Bay. k
is the number of collections and n the number of length measurements included (see
‘Method’). 56
Figure 3.7 a) Monthly mean length (± 1 SD) of the five cohorts of Eukrohnia hamata starting
from a major birth month; b) Composite growth trajectories of the autumn brood (born
in October) and spring brood (born in April) assuming a 2-y lifespan; c) Growth-age
curves of the autumn and spring broods. Circles show mean values of each characteristic
(± 1 SD shown as ribbons). 58
Figure 3.8 Development of sexual features (a, oocyte number; b, ovary length; d, sperm load;
e, seminal vesicle width; f, seminal receptacle diameter) and oil vacuole area (c) with
length for the autumn and spring broods of Eukrohnia hamata. Circles show mean values
of each characteristic (± 1 SD shown as ribbons). Vertical line indicates average length
(15.4 mm) at one year of age. Maturity results for each brood were obtained from the
analyses of up to 283 individuals from each 1 mm length class. 60
Figure 3.9 Mean frequency (± 1 SD) of Eukrohnia hamata with oil in vacuole and/or
digestive tract by months. Number of water column collections shown inside bar (33 –
446 individuals per haul). 61
Figure 3.10 Abundances (ind. m-3) of Eukrohnia hamata age classes in discrete depth layers
of the Amundsen Gulf, characterized by their mid-points (black squares). Top panels:
autumn brood individuals. Bottom panels: spring brood individuals. Seabed shown in
brown, unsampled sections of the water column in gray. See ‘Method’ for further details.
62
Figure 3.11 Monthly length frequency distributions of Parasagitta elegans. Frequencies of
newborns highlighted in orange. Visually identified length cohorts shown as normal
distributions (in red) with red dots indicating the mean length. Each of the three cohorts
is labelled with a capital P and a number from oldest (1) to youngest (3). Blue line is the
total distribution obtained by summing the modelled distributions. Chi-square values for
the goodness-of-fit of the total distribution to the data are given. Sampling regions are
abbreviated in each panel: NF, Nachvak Fjord; PC, Parry Channel; AG, Amundsen Gulf;
BB, Baffin Bay. k is the number of collections and n the number of length measurements
included (see ‘Method’). 63
Figure 3.12 a) Monthly mean length (± 1 SD) of the three cohorts of Parasagitta elegans
starting from a major birth month; b) Composite growth trajectory of the single brood.64
Figure 3.13 Development of sexual features (a, oocyte number; b, ovary length; c, sperm
load; d, seminal vesicle width; e, seminal receptacle diameter) with length in Parasagitta
elegans. Circles show mean values of each characteristic (± 1 SD shown as ribbons).
xv
Vertical line indicates average length (20.7 mm) at one year of age. Maturity results were
obtained from the analyses of up to 63 individuals from each 1 mm length class. 65
Figure 3.14 Abundances (ind. m-3) of Parasagitta elegans age classes in discrete depth layers
of the Amundsen Gulf, characterized by their mid-points (black squares). Seabed shown
in brown, unsampled sections of the water column in gray. See ‘Method’ for further
details. 66
Figure 4.1 Bathymetric maps of the Arctic Ocean, showing the positions and IDs of sampling
stations (black circles) in (a) Amundsen Gulf, (b) north-eastern Chukchi Sea and (c)
Baffin Bay (SIF = Scott Inlet Fjord; GF = Gibbs Fjord; SBB = southern Baffin Bay).
Details of sampling stations are shown in Appendices E-1 and E-2. 79
Figure 4.2 Vertical distributions of chlorophyll a biomass (mg m-3) in the upper 200 m of the
water column along the ship track from November 2007 to July 2008 in the Amundsen
Gulf. Black dots indicate sampling depths. Details of sampling stations are shown in
Appendix E-1. Chl a data were provided by Michel Gosselin (Université du Québec à
Rimouski). 84
Figure 4.3 Average number of prey per chaetognath gut (npc) in square-conical (S-C) net and
Multinet collections from November 2007 to August 2008 in the Amundsen Gulf.
Numbers of individuals shown above data points. k is the number of collections. Inset
bottom: photograph of a Parasagitta elegans specimen (12 mm) with a relatively large
Pseudocalanus spp. copepod in the gut (from November 2 2007). 86
Figure 4.4 Photographs of substantial amounts of green macroaggregates (˃ 500 µm) in the
guts of Eukrohnia hamata, but not in the guts of Parasagitta elegans. Specimens from
the Amundsen Gulf on May 31 2008 (20-40 m depth), 20-30 mm. 87
Figure 4.5 Scanning Electron Microscope photographs of some items in Eukrohnia hamata
guts (left box) and Parasagitta elegans guts (right box), in different months. Examples:
hooks of a chaetognath, and mandibles of copepods (arrow caps). Specimens 20-30 mm.
89
Figure 4.6 Photographs of live Eukrohnia hamata individuals consuming green
macroaggregates in-vitro in the Chukchi Sea. Specimens 20-30 mm. Bottom right: An
inverted microscope photograph of phytoplankton such as Ceratium spp. in one gut. 90
Figure 4.7 Fatty acid biomarkers in Eukrohnia hamata and Parasagitta elegans at different
stations in autumn 2014. Sampling locations are abbreviated: CS, Chukchi Sea; SIF,
Scott Inlet Fjord; GF, Gibbs Fjord; SBB, southern Baffin Bay. From top panel to bottom
panel: mean ratios of the carnivory biomarker 18:1 (n-9)/(n-7), mean proportions of the
Calanus biomarkers ΣC20:1+C22:1 MUFA, and mean ratios of the algal biomarker
16:1/16:0 (± 1 SD). No bars – no data available. 94
xvi
Figure 4.8 Mean sample δ13C and δ15N values and corresponding trophic levels (± 1 SD) of
Eukrohnia hamata and Parasagitta elegans. Station IDs shown next to data points.
Results from Chukchi Sea stations inside red oval. Results from Baffin Bay region
stations inside blue oval (locations are abbreviated: SIF, Scott Inlet Fjord; GF, Gibbs
Fjord; SBB, southern Baffin Bay). 96
xvii
Dedicated to the memory of Helen McMahon, my granny, who made it possible for me to
first pursue my interest in the Arctic regions.
23 August 1929 – 25 March 2015
Angelina Kraft
JP Aubé
xviii
Acknowledgements
I am now nearing the end of my journey to gain a Ph. D. in Oceanography, and there are
several people who have supported me whom I would like to acknowledge in this thesis.
Firstly, I would like to thank my director of research, Dr. Louis Fortier for allowing me to
realize this project on the enigmatic chaetognaths. I would also like to thank Louis for giving
me opportunities to attend and present my research at several national and international
conferences, to voyage to the Arctic/sub-Arctic on three separate research cruises, and for
the many ways in which he helped me improve my experience in scientific writing. Thanks
to Drs. Jean-Éric Tremblay, Guillaume Massé and Stéphane Plourde for evaluating the ‘dépôt
initial’ of my thesis and thesis defense presentation, and providing useful suggestions for
improvements. Thanks also to Dr. Maurice Levasseur for participating in my Ph. D.
committee, and to Dr. Ladd Johnson for presiding over my defense presentation.
I express my gratitude to my colleagues Drs. Øystein Varpe (UNIS), Stig-Falk Petersen
(Akvaplan-niva), Dominique Robert, Eric Rehm, Guillaume Massé and Marcel Babin
(Université Laval), Roxane Barthélémy and Jean-Paul Casanova (Aix-Marseille Université),
and Mrs. Ariane Beauféray (Université Laval), all of whom helped to shape the direction of
this thesis. I would like to specifically acknowledge Dr. Øystein Varpe who has consistently
shown a keen interest in my research, and been happy to offer constructive ideas and
suggestions. Thanks to Drs. Catherine Lalande (Université Laval), and Tara Connelly
(Memorial University of Newfoundland), as well as anonymous journal referees for Polar
Biology and Journal of Plankton Research, for offering valuable comments on chapters.
I am grateful to the crew and scientific staff on expeditions with R/V Helmer Hanssen and
CCGS Amundsen for research support. Dr. Gérald Darnis’ assiduity onboard CCGS
Amundsen, and in the laboratory, was fundamental to the success of zooplankton sections of
the CFL project. Mr. Carl Ballantine collected samples from Svalbard in 2013. I greatly
appreciate the hard work of my student assistants; Mrs. Ariane Beauféray, Miss. Marianne
Caouette, Miss. Vicky St-Onge, Mr. Joël-Fortin Mongeau and Mr. Pierre-Olivier Sauvageau,
for helping me to analyse the vast number of chaetognaths included in this thesis. Sincere
thanks also to the following individuals and lab groups for analysing fatty acids and stable
xix
isotopes: Dr. Guillaume Massé, Miss Caroline Guilmette, Mr. Jonathan Gagnon, the Institute
for Energy Technology and UNILAB in Norway. Thanks to Drs. Jean-Éric Tremblay and
Michel Gosselin, and Miss Marjolaine Blais for contributing environmental datasets.
I would like to thank my close friends Moritz Schmid, Kai Shapiro and Sophie Regueiro for
their moral support during the most challenging stages of my Ph. D. Many others, including
Cyril Aubry, Kevin Gonthier, Arnaud Pourchez, Noémie Friscourt, Max Geoffroy and other
members of the Fortier lab, have given me great memories from my time in Québec and
Canada. I am grateful to my parents (Ali and Dave), sister Ara, as well as the rest of my
family, who were ready to Skype at a moment’s notice and were always ready to offer
support, advice and encouragement. Thanks to the School for Science and Math at Vanderbilt
(Nashville, USA) for more recently giving me the opportunity to share my passion for the
polar regions with the next generation of scientists.
Bursaries from Takuvik and Québec-Océan allowed me to keep the focus on all my doctoral
activities and reach these final stages of my Ph. D. course.
xx
Foreword
This doctoral thesis comprises a General Introduction (Chapter 1), three scientific articles
(Chapters 2, 3 and 4), and a number of General Conclusions relating to the objectives of the
thesis (Chapter 5). Chapter 2 is published in Polar Biology as part of a Special Issue on Polar
Night ecology. Chapters 3 and 4 are currently in preparation for publication:
Chapter 2
Grigor J.J., Marais A., Falk-Petersen S., Varpe Ø. (2015) Polar night ecology of a pelagic
predator, the chaetognath Parasagitta elegans. Polar Biology 38:87-98 (reproduced with
permission of the publisher). Minor formatting changes have been made to the material
published in Polar Biology, to ensure compatibility with the other chapters in this thesis (e.g.
species names are written out in full the first time they are used in every new paragraph, and
thereafter abbreviated to their shorter form. Citations follow the same format as in the other
chapters).
Chapter 3
Grigor J.J., Schmid M.S., Fortier L. Growth and reproduction of the chaetognaths
Eukrohnia hamata and Parasagitta elegans in the Canadian Arctic Ocean: capital breeding
versus income breeding. This has been revised and recently re-submitted to Journal of
Plankton Research.
Chapter 4
Grigor J.J., Barthélémy R.-M., Massé G., Casanova J.-P., Fortier L. Feeding strategies of
arctic chaetognaths: are they really “tigers of the plankton”? This will be submitted to Journal
of Plankton Research.
The aims and objectives of this thesis were designed by myself. All the analyses were
performed by myself (or by students under my supervision). To collect material for the thesis,
I participated in research cruises in winter 2012, autumn 2013 and autumn 2014. Chapters 2-
4 have benefited from the corrections and comments of my co-authors. Results of these three
xxi
chapters have been presented at the following national and international scientific
conferences:
[9] Grigor J.J., Marais A.E., Schmid M.S., Varpe Ø., Fortier L. (2015) Ecology of arrow
worms in the Arctic: are they really “tigers of the zooplankton”?? APECS Online
Conference – New Perspectives in the Polar Sciences
[8] Grigor J.J., Varpe Ø., Marais A.E., Schmid M.S., Rehm E., Fortier L. (2014) Ecology
of arrow worms in the Arctic: are they really “tigers of the zooplankton”?? Arctic Change
Conference (Ottawa, Canada)
[7] Grigor J.J., Marais A.E., Schmid M.S., Rehm E., Fortier L. (2014) Arrow worm
ecology in the Canadian Arctic. Arctic Change Conference (Ottawa, Canada)
[6] Grigor J.J., Marais A.E., Schmid M.S., Rehm E., Fortier L. (2014) Arrow worm
ecology in the Canadian Arctic. Assemblée générale annuelle de Québec-Océan (Rivière-
du-Loup, Canada)
[5] Grigor J.J., Marais A.E., Schmid M.S., Fortier L. (2013) Seasonal ecologies of
chaetognaths (gelatinous zooplankton) in the Canadian Arctic. ArcticNet Annual Science
Meeting (Halifax, Canada) *Awarded best poster in its category: Marine Natural Science
[4] Grigor J.J., Søreide J.E., Varpe Ø., Fortier L. (2013) Seasonal ecology and life history
strategies of the chaetognath Parasagitta elegans in the Canadian and European Arctic:
The story so far. Assemblée générale annuelle de Québec-Océan (Rivière-du-Loup,
Canada)
[3] Grigor J.J., Søreide J.E., Varpe Ø. (2013) The annual routine of a predatory arctic
chaetognath in a highly seasonal environment. Arctic Frontiers: Geopolitics and marine
production in a changing Arctic (Tromsø, Norway)
xxii
[2] Grigor J.J., Søreide J.E., Varpe Ø. (2012) The annual routine of a predatory
zooplankter in a highly-seasonal Arctic environment. Annual ArcticNet Science Meeting
(Vancouver, Canada)
[1] Grigor J.J., Søreide J.E., Varpe Ø. (2012) The annual routine of a predatory
zooplankter in a highly-seasonal Arctic environment. Québec Océan 10-yr conference: A
reality check on oceans’ health (Montreal, Canada)
During my Ph. D., I participated as a co-author in the writing of one scientific article that
used an underwater camera system, the Lightframe On-sight Keyspecies Investigation system
(LOKI), to capture excellent images of zooplankton and document their fine-scale vertical
distributions. The study also developed a model to automatically identify the species and
stages of imaged animals:
[1] Schmid M.S., Aubry C., Grigor J.J., Fortier L. (2016) The LOKI underwater imaging
system and an automatic identification model for the detection of zooplankton taxa in the
Arctic Ocean. Methods in Oceanography 15:129-160
1
1. Chapter 1 – General introduction
1.1 The Arctic Ocean
The Arctic area is characterized by strong seasonal cycles in solar radiation and surface sea-
ice cover. The sun remains more than 12° below the horizon at the height of winter (the ‘polar
night’) and does not set at the height of summer (the ‘midnight sun’). The Arctic Ocean
covers an area of 14 million km2 (Huntington & Weller 2005) and is divided by a submarine
ridge of continental crust (the Lomonosov Ridge) into two major basins, the Eurasian and
Amerasian Basins (Figure 1.1). Vast continental shelves comprise 50 % of the Arctic Ocean
area (Figure 1.1), and these are amongst its most biologically productive areas (Sakshaug
2003, see ‘Marine ecosystems’ section).
Figure 1.1 Bathymetric map of the central Arctic Ocean and several marginal seas
(http://recherchespolaires.inist.fr/?L-ocean-Arctique-physiographie).
2
1.1.1 Physical environment
Through dynamic and thermodynamic processes (movement, growth and melt), the extent of
surface sea-ice increases to its maximum in March and declines thereafter towards its
minimum in September (Stroeve et al. 2008). Sea-ice acts as a barrier between the underlying
ocean and the atmosphere affecting heat exchange and the transmission of light that algae in
the water require for primary production. Sea-ice is also a habitat for several specialized fish,
seabird and mammal species, and influences global climate. Ice formation in key locations is
important for the formation of cold and highly saline water. This briny water sinks, initiating
deep-water currents that move into other oceans as an integral part of the ‘thermohaline
circulation’ (Loeng et al. 2005). Surface water/ice follows two important surface currents: in
the western Arctic the clockwise-turning Beaufort Gyre; and in the eastern Arctic the
Transpolar Drift, which exports ice into the Atlantic (Stein & Macdonald 2004). Freshwater
contributions from ice melt, precipitation and large non-freezing rivers (e.g. Ob and Yenisei
in Eurasia, the McKenzie and Yukon in N. America), increase the buoyancy of surface waters
(i.e. the Polar Mixed Layer). Great volumes of warm, relatively saline Atlantic water, also
enter the Eurasian Basin through the deep (2600 m) Fram Strait (Figure 1.2) and the Barents
Sea. Lower volumes of cold, relatively fresh Pacific water, are supplied to the Amerasian
Basin through the 45 m-deep Bering Strait (Stein & Macdonald 2004, Figure 1.2).
Figure 1.2 Water masses in the Arctic Ocean. Reproduced from Stein & Macdonald (2004).
3
In the Amerasian Basin, the Atlantic Water cools and becomes denser, plunging below the
Pacific water to depths ˃200 m, where it resides for ~30 years (Stein & Macdonald 2004,
Figure 1.2). The inflows of Pacific water in the Amerasian Basin and of Atlantic water in the
Eurasian basin create salinity gradients (haloclines) that protect sea-ice from warm waters
below (Winsor & Bjork 2000). Arctic deep water (cold and relatively saline), can occur below
900 m in the deep areas of the basins, where it has a residence time of 75-300 years (Stein &
Macdonald 2004, Figure 1.2).
1.1.2 Arctic marine ecosystems
Arctic marine ecosystems are considered less complex than most temperate and tropical
systems, with lower productivity and biodiversity in general (Loeng et al. 2005). In Arctic
marine ecosystems, extreme cycles in solar illumination and sea-ice cover lead to strong
seasonal cycles in primary production by autotrophic algae, with a considerable reduction in
winter (Ji et al. 2013). However, biological hotspots occur where a good nutrient supply to
surface waters supports high primary productivity. For instance, large blooms of
phytoplankton in some parts of the Chukchi Sea near Alaska support sizable communities of
invertebrates, both in the water column and on the seabed (Hopcroft et al. 2004, Grebmeier
et al. 2006, Nishino et al. 2016). Furthermore, polynyas (permanently open water areas
otherwise surrounded by sea-ice) are viewed as biological ‘oases’, with phytoplankton
blooms occurring in polynyas earlier in the season than in any surrounding areas (Ingram et
al. 2002, Hannah et al. 2009). This provides less-seasonally restricted access to food for
grazers and in turn their predators. Polynyas can be formed by the upwelling of warm
seawater which prevents ice from forming (i.e. sensible heat polynya), and/or by the influence
of wind in driving ice away (i.e. latent heat polynya; Hannah et al. 2009). The large North
Water Polynya in northern Baffin Bay (Canadian Arctic) is mainly a latent heat polynya in
winter and spring, however, sensible heat is also important for its growth in late spring
(Ingram et al. 2002).
In ice-covered seas, a bloom of under-ice algae is initiated during spring which is then
succeeded by a bloom of pelagic phytoplankton when the ice retreats in the spring/summer.
4
Some locations can have another distinct phytoplankton bloom in autumn (Ardyna et al.
2014). Increases in the occurrence of autumn blooms across the Arctic may be a symptom of
global warming (see ‘Climate change and other challenges for Arctic marine life’ section).
On average, phytoplankton production is higher (12 to 50 g C m-2 yr-1) than ice algae
production (5 to 10 g C m-2 yr-1). However, ice algae production exceeds that of
phytoplankton in locations with thick multi-year ice cover (Legendre et al. 1992, Leu et al.
2011). Bloom phenology varies with latitude and timing of open water (Zenkevich 1963,
Falk-Petersen et al. 2009, Tremblay et al. 2012), and the magnitude of a phytoplankton bloom
during the ice-free period is determined by nitrogen availability (Tremblay & Gagnon 2009),
and also influenced by zooplankton grazing (e.g. Banse 2013).
Arctic marine ecosystems contain at least 5000 species of invertebrate animal taxa from 24
phyla (Hoberg et al. 2013 and references therein), 91 % of which are associated with the
seabed (i.e. ‘benthic’), 8 % with the water column (i.e. ‘pelagic’) and 1 % with the sea-ice
(i.e. ‘sympagic’). Copepods belonging to the genus Calanus (Figure 1.3) are known as ‘key
species’ in the Arctic seas. They convert carbohydrates and proteins taken up from the algae
into high-energy lipids (wax esters) that comprise the main energy source within the food
web (e.g. Falk-Petersen et al. 2009).
Figure 1.3 The planktonic food web showing
protozoan and metazoan consumers at arrow
caps. Adapted from Hopcroft et al. (2008).
5
Amongst the vertebrates, up to 250 fish species reside in the Arctic area defined by the
Conservation of Arctic Flora and Fauna (an Arctic Council Working Group), for part or all
of the year (Hoberg et al. 2013). The polar cod Boreogadus saida is an endemic species which
can channel up to ~75 % of energy flow from zooplankton to vertebrate predators (Welch et
al. 1992). In addition, 35 species of mammals and 60 species of seabirds are observed in
Arctic waters, with the Baffin Bay little auk population considered to be the largest seabird
population in the world (Hoberg et al. 2013). Heterotrophic microbes and protists (Figure
1.3) remineralize dissolved organic carbon (˂0.45 µm) excreted from these consumers into
inorganic forms of carbon which can then be taken up again by protozoans (Hopcroft et al.
2008).
1.2 Zooplankton and their polar adaptations
Zooplankton are aquatic animals with body sizes ˂ 0.002 mm to ˃ 200 mm which have limited
ability to control their horizontal positions against water currents. As zooplankton have little
capacity to evade warming waters and are typically not harvested by humans, variations in
their distribution or phenology may strongly herald climate change effects (Richardson
2008). Zooplankters include herbivores, omnivores and carnivores, and are food for a wide
diversity of invertebrate and vertebrate predators. Zooplankton fecal pellets can be an
important source of carbon sequestration (e.g. Wassmann et al. 1999). However, fecal pellets
excreted in epi-pelagic waters are typically removed rapidly in surface waters. This is due to
degradation by bacteria, protozooplankton and copepods (Morata & Seuthe 2004, Turner
2015). Copepods, chaetognaths and other zooplankters are classified as ‘holoplankton’ taxa
(that drift in the sea throughout their entire life cycle). In contrast, a variety of fish, decapods
and other species are plankton only when they are larvae (‘meroplankton’), before then
continuing life as nekton or benthos (Stübner et al. 2016). Some zooplankton species are
capable of migrating considerable distances through the water column over day-night,
seasonal or ontogenetic cycles. These behaviors may be associated with finding food,
avoiding predation, or gaining an energy bonus from resting in colder waters, and they alter
the spatial distributions of food, materials and energy (Longhurst et al. 1984, Haney 1988).
6
Arctic zooplankton biomass is typically dominated by Calanus copepods, followed by non-
copepod taxa such as amphipods and chaetognaths (Figure 1.4). Zooplankton abundance is
dominated by small cyclopoid and calanoid copepods including Oithona similis and
Pseudocalanus spp., amongst others (e.g. Søreide et al. 2003, Hopcroft et al. 2004, Darnis &
Fortier 2014). For stable co-existence, similar species must occupy slightly different
ecological niches, efficiently partition available food and share habitat resources (Gause
1934, Ross 1986).
Figure 1.4 Photographs of living holo-zooplankton captured in-situ by a zooplankton imager
(Lightframe On-sight Key Species Investigation System; Schmid et al. 2016), during
deployments in the Canadian Arctic (summer 2014).
Due to reduced growth rates in colder temperatures, zooplankton and other polar
invertebrates often have longer lives and they reach maturity at older ages than those at lower
latitudes (Hoberg et al. 2013). High-latitude zooplankton display a range of adaptations to a
seasonal food source associated with, for instance, the timing and extent of growth and
7
reproduction, diapause, lipid content and feeding strategy (e.g. Conover 1988, Falk-Petersen
et al. 2009, Varpe 2012, Grigor et al. 2014).
For grazers, such as Calanus glacialis, timing their growth and reproduction to coincide with
the ice algae bloom can be of the utmost importance, as it would enable offspring to hatch
~3 weeks later during the phytoplankton bloom (Søreide et al. 2010, Leu et al. 2011, Daase
et al. 2013). The high-quality food provided during this latter bloom allows for critical early
growth of copepod offspring, without risk of starvation. Such a ‘match’ between the
development of primary production and copepod offspring benefits copepod populations and
the food web in general. However, in cases where offspring hatch before or after the peak of
the phytoplankton bloom, they miss the phytoplankton food needed for healthy growth
(Søreide et al. 2010, Leu et al. 2011). Such a ‘mismatch’ scenario has been shown to
drastically reduce Calanus biomass (Leu et al. 2011).
Storage lipids are important for Arctic organisms, in which they may be used to fuel one or
more of the following processes; basal metabolism, growth, maturation and reproduction
(Kattner et al. 2007). Wax esters (comprising one fatty acid and one fatty alcohol) are the
main long-term energy deposit in zooplankton, whereas triacylglycerols (comprising three
hydrocarbon chains on a glycerol backbone) provide energy for activities in the short term
(Lee et al. 2006). In winter, Calanus copepods and other grazers survive by entering diapause
in relatively deep waters during which time accumulated wax ester stores are metabolized
for energy. Capital breeders (e.g. C. hyperboreus) use their wax esters to fuel reproduction,
and can produce offspring earlier in the season giving them a longer time to develop their
energy reserves, required for surviving the next winter. Reproductive fitness is also improved
(Varpe et al. 2007). Income breeders need recent food to reproduce, and mixed capital-
income breeders use a combination of the two strategies (e.g. Sainmont et al. 2014a).
Carnivores are assumed to have a low capacity for long-term energy storage (Hagen 1999),
however, this may not be true for some species. Carnivorous and omnivorous zooplankters,
like amphipods (Figure 1.4) are also assumed to feed opportunistically year-round (Hagen
1999).
8
1.3 Chaetognaths
Chaetognaths (Figure 1.5) are a phylum of semi-gelatinous (dry weight ˃5 % wet weight;
Larson 1986) marine mesozooplankton. They are represented worldwide by at least 127
pelagic and benthic species from 23 genera with body lengths 2-120 mm (e.g. Bone et al.
1991, Foster 2011). The name ‘chaetognath’ (Chaeto = bristle, gnath = jaw) relates to the
presence of hooks on the head (Figure 1.5). Chaetognaths are also known as ‘arrow worms’
due to their lean appearance and rapid motion. These coelomates have existed from the
Middle Cambrian and possibly before then (Walcott 1911). The global biomass of
chaetognaths has been estimated at 10-30 % of that of copepods (Bone et al. 1991). The
majority of species are residents of the upper 200 m of the water column (i.e. epi-pelagic;
Pierrot-Bults & Nair 1991).
Figure 1.5 Typical physiology of a chaetognath belonging to the family Sagittidae.
Reproduced from Margulis & Chapman (2010).
Chaetognaths occur in the diets of zooplankton such as amphipods (Gibbons et al. 1992),
jellyfish (e.g. Zavolokin et al. 2008) and other chaetognaths (e.g. Pearre 1982), and recently
have received attention as the preferred prey for the larvae of tropical fish and commercially
9
important decapods (e.g. Sampey et al. 2007, Saunders et al. 2012). In the Arctic, fish such
as the polar cod (Rand et al. 2013), seabirds such as the little auk (Mehlum & Gabrielsen
1993) and baleen whales (Pomerleau et al. 2012), feed on chaetognaths. Suthers et al. (2009)
described chaetognaths as “the tigers of the plankton”. Animals in the phylum are generally
thought to be opportunistic, but strict carnivores (Marazzo et al. 1997). For further details,
see ‘Feeding strategies and trophic importance’ section.
1.3.1 Arctic species and distributions
In contrast to the high chaetognath diversity observed in other seas (e.g. De Souza et al.
2014), only three major species (Eukrohnia hamata, Parasagitta elegans and Pseudosagitta
maxima) are frequently reported in Arctic plankton surveys (e.g. Kramp 1939, Buchanan &
Sekerak 1982, Sameoto 1987, Figure 1.6). Another two species have been detected in Arctic
bathy-pelagic surveys; Heterokrohnia involucrum (Dawson 1968) and H. mirabilis (Kapp
1991). Kosobokova & Hopcroft (2009) reported that chaetognaths represented, on average,
about 13 % of the zooplankton biomass in the Canadian Arctic in summer 2005.
Figure 1.6 Photographs of the heads and the bodies of the major arctic chaetognaths. (a)
Eukrohnia hamata with characteristic marsupial sac and oil vacuole, (b) and (c) Parasagitta
elegans and Pseudosagitta maxima without marsupial sacs and oil vacuoles.
All images except P. maxima head from:
http://www.arcodiv.org/watercolumn/Chaetognaths.html (courtesy of Russ Hopcroft).
10
Parasagitta elegans (previously Sagitta) is restricted to the North Atlantic, North Pacific and
Arctic Oceans, with its lower distribution limit at 41°N and a northern limit short of the
central Arctic basin (e.g. Bogorov 1946, Bieri 1959, Grainger 1959). It is generally an epi-
pelagic, neritic species throughout most of its range (e.g. Terazaki 2004). Terazaki (2004)
described P. elegans as the best-studied chaetognath species. In contrast to P. elegans,
Eukrohnia hamata and Pseudosagitta maxima are cosmopolitan species occurring in all
oceans, with predominantly meso- or bathy-pelagic affinities (e.g. Bigelow 1926, Bieri 1959,
Cheney 1976, Thuesen et al. 1993). All three species occasionally co-occur at epi-pelagic
depths in the Arctic (e.g. Alvarino 1964, Hopcroft et al. 2005, Bieri 1959). The life cycle and
feeding strategy of E. hamata is more thoroughly studied in the Southern Ocean (e.g.
Øresland 1990, Øresland 1995, Froneman & Pakhomov 1998, Froneman et al. 1998, Kruse
2009, Kruse et al. 2010), and few studies exist on the ecology of P. maxima in the Arctic (see
Sameoto 1987).
Some chaetognaths may migrate long distances vertically through the water column. Grigor
et al. (2014) reported seasonal vertical migrations (SVM) in a fjord population of Parasagitta
elegans in the European Arctic. In this Svalbard fjord, the youngest age class resided near
the surface during the summer phytoplankton bloom, whereas all three age classes mostly
remained below 60 m from September to April (seasonal migrations closely mirrored those
of Calanus prey). Daase et al. (2016) also reported diel (day-night cycle) vertical migrations
(DVM) in a population of Eukrohnia hamata in another Svalbard fjord, towards the end of
the midnight sun period. Migrations involved upward movements of E. hamata to surface
waters, apparently to feed at night, and downward movements to deeper waters, apparently
to avoid predators in well-lit waters during the day.
1.3.2 Lifespans
The life history characteristics of chaetognath species (e.g. life span, size at maturity, time
and number of spawning cycles per year) differ throughout their geographical ranges in
response to variations in temperature, food quantity and quality (Pearre 1991, Alvarino 1990,
Terazaki 2004). In temperate seas, both Eukrohnia hamata and Parasagitta elegans may
11
have lifespans of less than a year (e.g. Russell 1932, Terazaki & Miller 1986, Sameoto 1971,
Zo 1973, King 1979, Terazaki & Miller 1986). In the Arctic, two-year lifespans have been
suggested for E. hamata (Sands 1980, Sameoto 1987, Pearre 1991); one to three-year
lifespans have been suggested for P. elegans (e.g. Dunbar 1940, McLaren 1961, Timofeev
1995, Welch et al. 1996, Grigor et al. 2014); and the larger Pseudosagitta maxima may live
for four to five years (Sameoto 1987).
1.3.3 Reproductive strategy
Chaetognaths are hermaphrodites, able to reproduce by both cross and self-fertilization. Male
gonads in the tail region (testes and seminal vesicles, Figure 1.5) produce and transmit sperm,
whilst female gonads in the trunk region (ovaries and seminal receptacles, Figure 1.5)
produce ova and receive sperm from a neighbor (Alvarino 1992). Although cross-fertilization
is more common due to sperm maturing earlier than oocytes, this strategy makes self-
breeding possible when access to mates is limited (Alvarino 1992). The eggs of chaetognaths
hatch a few days after oocytes are fertilized (e.g. Kotori 1975). Hatching takes place inside a
marsupial sac in Eukrohniidae (Figure 1.6a) and in open water in Sagittidae (Alvarino 1968,
Kotori 1975, Hagen 1985). Kuhl (1938) suggested that chaetognaths die immediately after
spawning. However, several other authors have disputed this finding, instead showing
iteroparity and continued spawning after laying their first batch of eggs (Conway & Williams
1986, Grigor et al. 2014). Whilst Eukrohnia hamata is reported to breed year-round in the
Southern Ocean (Øresland 1995), breeding of Parasagitta elegans in the Arctic mainly
coincides with peak abundance of zooplankton food (e.g. Kramp 1939, Dunbar 1940,
Grainger 1959, McLaren 1961, Dunbar 1962, Grigor et al. 2014).
1.3.4 Oil vacuoles in Eukrohnia spp.
The middle section of the gut in Eukrohnia spp. contains an elliptical oil vacuole (Figure
1.6a), also described in earlier reports as an ‘oil droplet’ (Øresland 1990, Froneman &
Pakhomov 1998, Froneman et al. 1998, Kruse et al. 2010, Giesecke & Gonzalez 2012, Pond
2012). Such an oil vacuole is not present in Sagittidae species (e.g. Figure 1.6b and Figure
1.6c). Oil vacuoles in Eukrohnia species may store wax esters. Wax esters seem to occur in
12
much higher amounts in Eukrohnia hamata compared to Parasagitta elegans and
Pseudosagitta maxima (e.g. Lee & Hirota 1973, Falk-Petersen et al. 1987, Donnelly et al.
1994, Lee et al. 2006, Connelly et al. 2012, Connelly et al. 2016). Large wax ester supplies
in Eukrohnia chaetognaths could suggest a potential for metabolic reduction/capital breeding,
as occurs in overwintering zooplankton, though the centralized position of the oil vacuole in
the body also hints at a buoyancy control function (Pond 2012).
1.3.5 Feeding strategies and trophic importance
Zooplankton prey includes a wide range of ichthyoplankton and zooplankton, particularly
copepods (e.g. Terazaki 2004). Prey is sensed mechanically; chaetognath hairs detect
vibrations at distances of 1-3 mm (Feigenbaum & Reeve 1977, Goto & Yoshida 1981).
Specific prey types can be differentiated by their unique movements (Tonnesson & Tiselius
2005). The eyes of chaetognaths lack lenses capable of forming images but they do contain
a pigment that detects light direction (Pearre 1973). Therefore, their eyes may help them to
detect prey outside the maximum distance for hair detections (Goto & Yoshida 1981). Dorso-
ventral undulating movements are used to dart at prey, which is then seized by the hooks and
punctured by rows of small teeth (Figure 1.7). The locomotion appendages, as well as the
feeding appendages, differ between chaetognath species, for instance Eukrohnia hamata
lacks anterior teeth (Furnestin 1965), present in P. elegans (Terazaki 1993). Relatively large
items are consumed by expansions of the head (Bieri & Thuesen 1990). Chaetognaths may
paralyze prey by secreting a bacterial-produced neural poison (tetrodotoxin) from vestibular
ridges (Thuesen & Kogure 1989, Bieri & Thuesen 1990, Figure 1.7).
Figure 1.7 Photograph of a chaetognath’s head taken by Scanning Electron Microscopy
(left) with parts labelled (right). Reproduced from Bieri & Thuesen (1990).
13
In the waters of Nova Scotia (Canada), Sameoto (1971, 1972) suggested that the abundant
Parasagitta elegans could remove considerable fractions of the copepod standing stock per
day (36 % to ˃100 % depending on season). Welch et al. (1992) suggested that Eukrohnia
hamata and Pseudosagitta maxima may ingest up to 51 % of the copepod biomass in
Lancaster Sound annually, but noted that their conclusions for these chaetognaths were “little
better than guesses” (Welch et al. 1992). The above estimates of predation rates or proportion
of prey standing stock removed, were based on observations of gut contents in dead
chaetognaths, and specifically, methodology which treated visible lipid droplets in their
bodies as evidence of recent prey digestion (e.g. Sameoto 1971, Sameoto 1972, Sameoto
1987). This approach was also adopted for E. hamata in the Southern Ocean (Froneman &
Pakhomov 1998). Including lipids in predation rate calculations may be suitable for species
without considerable capacity for lipid storage. For Eukrohnia species it seems there is a risk
of confusing diagnostic lipid stores with oil droplets from copepods, which is likely to have
occurred in at least the Sameoto (1987) study (Øresland 1990). Several other polar studies
on E. hamata, as well as P. elegans and P. maxima, have reported much lower predation rates
when lipid droplets were excluded from the estimates (e.g. Sameoto 1987, Øresland 1995,
Froneman & Pakhomov 1998, Brodeur & Terazaki 1999, Bollen 2011, Giesecke & Gonzalez
2012).
Whilst chaetoganths are generally recognized as predators, several studies have also observed
algae (e.g. Alvarino 1965, Boltovskoy 1981, Alvarez-Cadena 1993, Kruse et al. 2010) or
high amounts of algae biomarkers (e.g. Philp 2007, Connelly et al. 2014) in chaetognath guts,
possibly indicating that these opportunistic feeders also ingest algae in seawater or graze
them from a substrate. Chaetognaths belonging to the genera Archeterokrohnia and
Heterokrohnia reside in the nepheloid layer, where they are reported to feed on organic
matter and bacteria from sediments (Casanova 1986). In an interesting recent study,
Casanova et al. (2012) suggested facultative osmotrophy (ingestion of dissolved organic
matter in ambient seawater) as the main mode of nutrition in chaetognaths.
14
1.3.6 Fatty acids and stable isotopes
Fatty acid profiles and stable isotope signals can also reveal information about consumer
diets, trophic positions, as well as the main primary producers in the food web. Chaetognaths
are easily stressed and damaged in plankton sampling nets. Potential food loss from damaged
guts or stress-induced regurgitation and defecation, as well as cod-end feeding, can all bias
gut content analyses and predation rate estimates (see Baier & Purcell 1997 and references
therein). In contrast to gut contents, fatty acid and stable isotope signals can persist for weeks
or months (Dalsgaard et al. 2003, Arim & Naya 2003). Fatty acid analysis is based on the
premises that (a) fatty acids are produced by specific organisms, and (b) the fatty acids
undergo limited breakdown and transformation in consumers (Dalsgaard et al. 2003, Arim &
Naya 2003). Nitrogen isotopes are used to assess trophic position, based on the premise that
the 15N/14N ratio undergoes a constant level of change between trophic levels (Minagawa &
Wada 1984, Michener & Schell 1994). Previous studies have used this technique to infer that
Eukrohnia hamata may feed more omnivorously than Parasagitta elegans in the Arctic
(Søreide et al. 2006, Hop et al. 2006). Carbon isotopes can indicate the carbon source in a
food web since the 13C/12C ratio differs little between a consumer and its food (Hobson &
Welch 1992).
1.4 Climate change and other challenges for Arctic marine life
Over millions of years, Arctic marine ecosystems have been shaped by profound
environmental changes that include transitions between glacial periods and interglacial
periods, in addition to large variations in sea level (Darby et al. 2006). However, the 2-3 ºC
rise in mean annual air temperatures since 1950 (Chapman & Walsh 2003) has had an
anthropogenic source (greenhouse gas emissions, and CO2 in particular). Sea surface
temperatures are increasing 2-3 times as fast as in the temperate oceans (known as ‘Arctic
amplification’), as elevated influx of warm Atlantic waters causes major heat advection
(Spielhagen et al. 2011). Overland et al. (2014) predicted further warming by up to 13 °C
prior to the autumn of 2100 if greenhouse gas emissions continue unabated. Consistent with
these changes, conditions in the Arctic Ocean are becoming more similar to those in
temperate oceans (referred to as ‘Atlantification’, see Wassmann et al. 2006).
15
Arctic seas are acidifying twice as fast as temperate seas due to enhanced CO2 solubility in
colder waters (Bates et al. 2011). This shift could directly affect zooplankters such as the
pteropod mollusc Limacina helicina, a prominent component of Arctic zooplankton
communities (Gannefors et al. 2005). L. helicina precipitates CaCO3 to build a shell required
for its survival. However, experiments suggest that the lower pH values expected to occur by
the end of the century will be associated with a drastic 28 % decrease in shell calcification
rate and the death of these animals (Comeau et al. 2009).
Previous studies have reported decreases in both the annual mean extent of Arctic sea-ice by
3.5-4.1 % per decade (1979-2012; IPCC 2014), and mean sea-ice thickness at the end of the
melt season by 1.6 m (1958-2000; Kwok et al. 2009) as well as a 5-day increase in the length
of the summer melt-season (1979-1996; Smith 1998). Further sea-ice loss would be
disastrous for species that depend on sea-ice to live, hunt and breed, such as some
invertebrates and vertebrates including the polar bear. Ice algae would also lose their
substrate (Loeng et al. 2005). Despite this, some phytoplankton taxa may benefit because a
major barrier to sunlight access would be removed. Whilst oceanic primary production has
recently decreased at lower latitudes, Pabi et al. (2008) reported an overall ~30 % Arctic
increase in oceanic primary production between 1998 and 2006. Ardyna et al. (2014) also
noted that phytoplankton blooms in autumn are becoming more common throughout the
Arctic, as reduced ice cover allows winds to stir the water, breaking down any existing water
column stratification, and making nutrients previously at depth available to phytoplankton
near the surface. Another consequence of the recent sea-ice melt combined with an increased
river discharge (Peterson et al. 2002) has been an increase in water column stratification
(McLaughlin & Carmack 2010). This has created a scenario in which nutrients in shallow
water can become more quickly depleted by its algal residents. Li et al. (2009) have already
reported a corresponding shift from larger cells (i.e. diatoms) to smaller algal cells (i.e. pico-
phytoplankton) which can extract available nutrients more efficiently. Such changes in the
composition or biomass of primary producers could result in unpredictable ‘bottom-up’
effects that ripple through planktonic grazers to higher trophic levels. In the future, possible
loss of ice algae blooms and changes in the timing of phytoplankton blooms could cause
16
more ‘mismatch’ scenarios in the development of primary producers and grazers, with
consequences for entire food webs (Søreide et al. 2010, Leu et al. 2011).
Changes in zooplankton abundances may also affect the survival of consumers which
selectively take larger lipid-rich taxa. Falk-Petersen et al. (2007) suggested that warming in
the Barents Sea (+2-3 ºC) could result in the replacement of two large lipid-rich species of
copepods (Calanus glacialis and C. hyperboreus) by a smaller, lipid-poor North Atlantic
congener species (C. finmarchicus). This may adversely affect specialist feeding seabirds
whilst benefiting herring and baleen whales, herring predators. Global warming is also
associated with northern movements of previously southern fish and mammals. There are
recent reports of northern movements of NE Atlantic Cod in the Barents Sea (e.g. Kjesbu et
al. 2014) and of killer whales in the Canadian Arctic (e.g. Higdon et al. 2012). As particularly
voracious predators on seals and fish, killer whales could exert top-down effects on lower
trophic levels, with unpredictable effects on zooplankton (Ferguson et al. 2010).
Arctic seas provide a wide range of ecosystem services for sustenance, recreation and the
well-being of people living within and outside the Arctic (e.g. petroleum products, fish,
animal furs, tourist destinations). Seabed beyond the Arctic Circle is thought to contain 30 %
and 13 % of the world’s undiscovered oil and gas respectively, with the majority of
undiscovered oil located in Arctic Alaska (Bird et al. 2008). With ice-free waters expected
to occur as early as September 2045 (Laliberté et al. 2016), these supplies will become
increasingly accessible and may be exploited as global population grows. Potential oil spills
are a concern because Arctic ecosystems are frail and Arctic seas present significant
containment and recovery challenges. The ecological impacts of previous large spills in sub-
Arctic waters have been considerable (e.g. Exxon Valdez 1989 in the Gulf of Alaska), with
spilt oil persisting in marine habitats for decades after spillages (e.g. Peterson 2001).
Shipping has also increased: with a change in the number of recorded vessels travelling
through the Northern Sea Route from 4 in 2010 to 71 in 2013 (Linstad et al. 2016). This also
exposes ecosystems to increased pollution, and so careful regulation placed on activities will
be critical to maintaining Arctic biodiversity. Worldwide increases in jellyfish populations
in recent years have been a concern for human health and marine operations such as fishing,
17
drilling etc. These observations may be related to increasing temperatures, low populations
of forage fish (competitors for food) and the presence of humans, amongst other factors (e.g.
Brotz et al. 2012, Purcell 2012). Brotz et al. (2012) concluded with high certainty that
jellyfish numbers will increase in the Southern Ocean but it is unclear how they will fare in
the Arctic where less restricted access offers new prospects for human activity. Similarly,
few predictions have been made into how polar chaetognaths might respond to climate
change and other environmental pressures.
1.5 Study areas
This thesis includes depth-integrated and depth-stratified sampling of zooplankton in several
different regions of the Arctic Ocean. The major sampling regions were the Svalbard
archipelago in the European Arctic (Chapter 2), and Amundsen Gulf, located in the south-
eastern Beaufort Sea of the Canadian Arctic (Chapters 3 and 4). Additional collections from
other regions of the Canadian Arctic (the Labrador Sea, Baffin Bay and the Canadian
archipelago) were included in the analyses for Chapters 3 and 4. Finally, collections from the
Alaskan part of the Chukchi Sea were included in Chapter 4.
The Svalbard archipelago: The first of our main sampling regions; the Svalbard archipelago
in Arctic Norway, is a meeting point for Arctic water and Atlantic water (Strömberg 1989).
We studied chaetognaths in several fjords on the west and north coasts of Svalbard.
Parasagitta elegans is the dominant chaetognath species in the Barents Sea (Falkenhaug
1991) and along the west coast of Svalbard (Grigor et al. 2014, Hirche et al. 2015), but
Eukrohnia hamata dominates to the north in regions with pack ice and reduced influence of
Atlantic water (Daase & Eiane 2007, Daase et al. 2016). Several Arctic fjords including those
in Svalbard and Baffin Bay are particularly useful for zooplankton studies due to having
‘sills’, seabed intrusions that reduce advection of water masses, and associated plankton
communities (e.g. Syvitski et al. 1990, Bell & Josenhans 1997, Arnkvaern et al. 2005, Grigor
et al. 2014). Svalbard fjords in recent years have been the focus of novel polar night research
cruises led by Norwegian universities to investigate pelagic biology and winter ecology
(Lønne et al. 2014).
18
The Amundsen Gulf: The second of our main sampling regions; the Amundsen Gulf in the
southeastern Beaufort Sea, was the site of a unique overwintering sampling campaign in
which an icebreaker was used to sample zooplankton and other ecosystem components year-
round (Figure 1.8). This formed a key part of the Circumpolar Flaw Lead (CFL) System
Study of 2007-2008. Several studies on copepod ecology have already been published from
this time (e.g. Forest et al. 2010, Wold et al. 2011a, Darnis & Fortier 2014).
Figure 1.8 Diagram illustrating the wide variety of sampling activities conducted during the
Circumpolar Flaw Lead System Study (2007-2008) from the icebreaker CCGS Amundsen
and at an ice camp, in order to study Arctic systems. Reproduced from Barber et al. (2010).
1.6 Aims and objectives
The central aim of this doctoral thesis is to improve our understanding of the ecology of two
major arctic chaetognath species; Eukrohnia hamata and Parasagitta elegans (Pseudosagitta
maxima was generally excluded from the thesis because of its rarity or absence at the
sampling locations). Specifically, the thesis aims at improving our understanding of these
chaetognaths’ feeding strategies and life cycles in the European Arctic, Canadian Arctic and
Alaskan Arctic. To that end, the thesis comprises three main chapters (2-4), presented as
scientific articles. The seasonal adaptations of arctic chaetognaths are interesting given the
19
high seasonality in the abundance of known prey (copepods) in epi-pelagic waters, which
could require these predators to carry out seasonal vertical migrations (SVM), or be able to
quickly switch their food sources. Chapters 2-4 each comprise winter sampling, addressing
the knowledge gap of biological processes during the polar night (Lønne et al. 2014). This
will allow us to gain a more holistic understanding of how chaetognaths in the Arctic could
react to climate change and other environmental pressures. The inclusion of locations with
different environmental conditions at the same time of the year allowed me to investigate
possible differences in life cycles and feeding strategies between populations.
The objective of Chapter 2 was to shed light on the polar night ecology of Parasagitta elegans
in fjords of the Svalbard archipelago, where P. elegans is previously reported to be an
abundant chaetognath species. Feeding ecology and reproductive dynamics were examined
in four different fjords during January 2012 and January 2013. Gut content analyses were
used to assess diets, feeding rate and potential impacts of P. elegans on copepod populations.
To gain further insights on the trophic positions of chaetognaths, stable isotope and fatty acid
trophic marker (FATM) analyses were carried out.
The objective of Chapter 3 was to describe the life histories of Eukrohnia hamata and
Parasagitta elegans in the Canadian Arctic, mainly in the Amundsen Gulf, over a full annual
cycle (August 2007 to August 2008). Growth and reproductive dynamics were inferred from
body length, and the condition of oil vacuoles and maturity features. I tested the hypothesis
that E. hamata is a capital breeder that spawns during most of the year, whilst P. elegans is
an income breeder, reproducing exclusively during periods of high prey availability.
The objective of Chapter 4 was to understand how food resources are utilized year-round by
co-existing Eukrohnia hamata and Parasagitta elegans in the Canadian and Alaskan Arctic.
In the Amundsen Gulf, gut contents were examined to reveal diets from November 2007 to
August 2008. FATM and stable isotope signatures of E. hamata and P. elegans in two distant
regions (the Alaskan portion of the Chukchi versus Sea and Baffin Bay) were compared,
based on collections made in autumn 2014.
20
2. Chapter 2 – Polar night ecology of a pelagic predator, the
chaetognath Parasagitta elegans
2.1 Résumé
Les routines annuelles et l'écologie saisonnière des espèces de zooplancton herbivores sont
relativement bien connues en raison de leur couplage étroit avec leur source de nourriture à
variation saisonnière, la production primaire. Quant aux niveaux trophiques planctoniques
supérieurs, ces interactions saisonnières sont moins bien comprises. Le présent chapitre
traitera de l’alimentation des chaetognathes dans les écosystèmes des fjords du haut-Arctique
au milieu de l’hiver. Les chaetognathes sont des prédateurs planctonophages très présents
dans les mers de haute latitude. Nous avons étudié l’espèce commune, le Parasagitta elegans,
autour de l'archipel du Svalbard (78-81ºN) au cours des hivers 2012 et 2013. Nos échantillons
étaient constitués de spécimens (longueur de corps : 9-55 mm), échantillonnés dans trois
fjords, dont le contenu du tube digestif (n = 903), la présence d’isotopes stables, la
composition en acides gras et l'état de maturité (n = 352) ont été étudiés. Environ un quart
des spécimens présentaient du contenu dans leur tube digestif, principalement des
gouttelettes de lipide et de débris chitineux, alors que seulement 4 % d’entre eux contenaient
des proies identifiables, principalement des copépodes Calanus spp. et Metridia longa. La
teneur élevée en δ15N du P. elegans et son niveau trophique moyen de 2.9 a confirmé son
profil de carnivore. Dans la même perspective, le profil d'acides gras [en particulier ses
niveaux élevés de 20:1 (n-9) et 22:1(n-11)] a confirmé la consommation de Calanus. Des
observations de gonades non-développées dans la plupart des P. elegans de grande taille,
ainsi que l'absence de petits spécimens ˂10 mm, a suggéré que la reproduction n'a pas
commencé si tôt dans l'année. Le taux d'alimentation moyenne du P. elegans selon les fjords
et les années était de 0,12 proie/ind.-1/jour-1, ce qui est faible par rapport aux mesures du taux
d'alimentation printanier et estival dans des environnements de haute latitude. Nos résultats
suggèrent une activité d'alimentation réduite pendant l'hiver. Par ailleurs, la prédation du P.
elegans semble avoir peu d'effets sur la mortalité des copépodes.
21
2.2 Abstract
The annual routines and seasonal ecology of herbivorous zooplankton species are relatively
well known due to their tight coupling with their pulsed food source, the primary production.
For higher trophic levels of plankton, these seasonal interactions are less well understood.
Here, we study the mid-winter feeding of chaetognaths in high-Arctic fjord ecosystems.
Chaetognaths are planktivorous predators which comprise high biomass in high-latitude seas.
We investigated the common species Parasagitta elegans around the Svalbard archipelago
(78-81ºN) during the winters of 2012 and 2013. Our samples consisted of individuals (body
lengths 9-55 mm) from three fjords, which were examined for gut contents (n = 903), stable
isotopes, fatty acid composition, and maturity status (n = 352). About a quarter of the
individuals contained gut contents, mainly lipid droplets and chitinous debris, whilst only 4
% contained identifiable prey, chiefly the copepods Calanus spp. and Metridia longa. The
δ15N content of P. elegans, and its average trophic level of 2.9, confirmed its carnivorous
position and its fatty acid profile [in particular its high levels of 20:1 (n-9) and 22:1 (n-11)]
confirmed predation on Calanus. Observations of undeveloped gonads in many of the larger
P. elegans, and the absence of small individuals ˂10 mm, suggested that reproduction had
not started this early in the year. Its average feeding rate across fjords and years was 0.12
prey ind.-1 day-1, which is low compared to estimates of spring and summer feeding in high-
latitude environments. Our findings suggest reduced feeding activity during winter and that
predation by P. elegans had little impact on the mortality of copepods.
22
2.3 Introduction
The Arctic is a highly seasonal environment, with conditions in the marine pelagic varying
greatly between summer and winter. The extreme cycles in solar illumination and sea-ice
cover create strong seasonality in primary production (Ji et al. 2013), which affects food
availability for organisms at higher trophic levels (Varpe 2012). Food availability for
herbivores such as Calanus copepods is severely reduced during the polar night. Many
grazers survive winter food shortages by resting at depth and sustaining themselves on
storage lipids accumulated when food was last available (e.g. Conover 1988). Although
pelagic omnivores and carnivores may experience a less-pulsed food source than for the
herbivores, they may also display adaptations to a seasonal food source (e.g. Newbury 1971,
Choe et al. 2003, Kraft et al. 2013). However, for many predators we lack knowledge of their
feeding opportunities and activities during winter.
The chaetognath Parasagitta elegans (Verrill 1873) is highly represented in Arctic
mesozooplankton communities, numerically and in biomass terms (e.g. Søreide et al. 2003,
Hopcroft et al. 2005). This typically neritic species (Bieri 1959) can exert high predation
pressure on Arctic copepods and compete with larval fish (e.g. Sameoto 1987). Some authors
have proposed that chaetognaths are not particularly sensitive to seasonality (e.g. Hagen
1999), suggesting that their varied diets (reviewed by Terazaki 2004) and non-visual food
search should allow them to find adequate nutrition throughout the year. Lipid-rich copepods,
often preferred prey, diapause in large densities and in an unalert state during winter, so they
may be easy prey for some carnivores (Darnis et al. 2012). However, some chaetognath
species at high latitudes are found to contain considerable amounts of lipids, including wax
esters, which may be used for storage (e.g. Lee 1974, Kruse et al. 2010). Furthermore, winter
growth rates of P. elegans in the Arctic is lower than those in spring and summer (Grigor et
al. 2014), and these observations could indicate reduced winter feeding and resting strategies
in this chaetognath.
We report here on the winter feeding ecology of Parasagitta elegans in the European high
Arctic. We used three different methods to assess its diet and trophic level: gut content
23
analysis, which records recent feeding, as well as stable isotope and fatty acid trophic marker
(FATM) analyses, which provide additional information on its feeding history, over time
frames of weeks to months (Graeve et al. 2005). We calculated feeding rates and possible
impact on copepod populations. Although we did not expect mid-winter reproduction (e.g.
Kramp 1939, Grigor et al. 2014), we also examined their level of maturity, allowing us to
infer how close P. elegans is to reproducing, which links to how actively individuals are
expected to feed.
2.4 Method
2.4.1 Study area
Chaetognaths were collected from waters around Svalbard (78-81ºN) during the winters of
2012 and 2013, during the ARCTOS ‘Polar Night Cruises’ (8 to 21 January 2012 and 9 to 18
January 2013).
The Svalbard archipelago is a meeting place for warm Atlantic water sourced from more
southern regions and colder Arctic water from the north. The northward moving West
Spitsbergen Current deposits Atlantic water into fjords on the west coast, with one branch
finally turning north-east at the top of Spitsbergen and affecting conditions in the Arctic
Ocean (Saloranta & Haugen 2001). We sampled three fjords in 2012: Rijpfjorden (station
R3), Isfjorden proper, and Adventfjorden, a tributary fjord of Isfjorden (station ISA, see
Figure 2.1). The latter two locations are hereafter referred to as ‘Isfjorden’. Another fjord,
Kongsfjorden, was sampled in 2013, and Rijpfjorden was re-sampled. See Appendix A for
full details on the sampling activities. Isfjorden (78ºN, 14ºE) and Kongsfjorden (79ºN,
11.5ºE) are influenced by Atlantic water masses and the outer parts are ice free for much of
the year (Svendsen et al. 2002, Nilsen et al. 2008), causing important seasonal changes in
biodiversity and animal populations in these fjords. Rijpfjorden, in contrast (80ºN, 22ºE), is
influenced by Arctic water, typically remaining ice-covered from December/February to July
(Wallace et al. 2010).
24
Figure 2.1 Map showing the locations of the stations sampled for chaetognaths in January
2012 and 2013.
2.4.2 Physical and biological environment
At all stations, vertical profiles of salinity, temperature, density, and fluorescence were
obtained using a CTD (SBE 9) and processed following standard Sea Bird Electronics (SBE)
procedures. In 2012, a steep thermocline was observed in Rijpfjorden between ~70 and 100
m, over which temperature rose to 2 ºC and then fell again to 0.5 ºC at ~200 m (Appendix
B). At the mouth of Isfjorden, the thermocline was much weaker, with temperature increasing
gradually to 2 ºC at ~200 m. At Isfjorden (station ISA), temperature varied little with depth
(Appendix B). At all stations, salinity varied with depth in similar ways to temperature. A
strong halocline occurred in Rijpfjorden only, at the same depths as the thermocline
(Appendix B). Fluorescence was very low (˂0.6 g l-1) at all stations in January 2012.
2.4.3 Zooplankton sampling
Horizontal trawls of the large Methot Isaac Kidd gear (MIK, 3.14-m2 opening, 1.5-mm mesh)
were used to obtain large numbers of Parasagitta elegans for the various dietary analyses
(Appendix A). MIK sampling depths in Rijpfjorden and Isfjorden (in 2012) captured all water
25
masses in the fjords (melt water, Arctic water/mixed Fram Strait water and Arctic deep
water). In contrast, most MIK sampling for chaetognaths in 2013 (Kongsfjorden and
Rijpfjorden) was carried out in the upper 20 m (Appendix A). This sampling decision was
taken to reduce haul time, as chaetognaths can easily become damaged and stressed during
net sampling, which poses several problems for gut content analyses (Baier & Purcell 1997).
In Rijpfjorden in 2012, vertical hauls of the smaller Multi-Plankton Sampler gear (MPS,
0.25-m2 opening, 0.2 mm mesh) were also performed to collect zooplankton community data
(see also Daase et al. 2014) and to source smaller Parasagitta elegans for gut content analyses
(sampled strata: 260-200 m, 200-100 m, 100-50 m, 50-20 m, 20-0 m; see Appendix A for
details). The MPS captured higher densities of smaller P. elegans (10-19 mm) in the upper
20 m than the MIK (0.5 ± 0.4 compared to 0.1 ± 0.1 ind. m-3), but fewer individuals ≥20 mm
(1.8 ± 1.7 compared to 5.9 ± 8.2 ind. m-3). Individuals ˂10 mm were not captured by either
gear in Rijpfjorden or Isfjorden in 2012. Grigor et al. (2014) similarly showed that the MPS
captured the smaller size fraction of P. elegans more efficiently than a larger ‘WP3’ net with
a 1-m2 opening. MPS samples collected from Isfjorden ISA on 27 January 2012 were also
analysed for abundance data.
2.4.4 Sample processing
Upon retrieval of each MIK haul, the cod end was immediately transferred to a marked bucket
and diluted up to the 10 l mark. A 0.6 l sub-sample was taken for community analysis and
fixed in 4 % buffered formalin-seawater solution. Webster et al. (2013) show presence-
absence data for zooplankton in Rijpfjorden from the community samples from 2012. From
a second 0.6 l subsample, 100 Parasagitta elegans were randomly picked out for gut content
analyses (Appendix A) and preserved in 4 % buffered formalin-seawater solution. On the
2012 cruise, 75-150 P. elegans were also picked out of this second sub-sample for stable
isotope analyses (n individuals = 675, Appendix A), and 30 individuals were randomly
picked out for fatty acid trophic marker (FATM) analyses (n individuals = 290, Appendix
A). These samples were frozen at -80 ºC until the end of the cruise and then stored at -80 ºC
for further processing.
26
2.4.5 Gut content analyses
A total of 202 individuals from 2012 (body lengths 10-55 mm) and 701 from 2013 (body
lengths 9-42 mm) were dissected and analysed for gut contents. In 2012, a minimum of 10
individuals were dissected from each MIK haul. In 2013, we examined the guts of all 100
individuals preserved from each MIK haul; 3-10 smaller individuals were sourced from each
MPS haul (Appendix A).
Parasagitta elegans individuals were measured to the nearest millimeter (excluding the
caudal fin) and stained with a solution of lignin-red, used to stain tissues of crustacean prey
in their guts (Falkenhaug 1991), and borax carmine, capable of highlighting the gonads of
prey (Pierce 1941), diluted 50 times in water. Head widths were measured to the nearest 0.01
millimeter under the binocular microscope. All visible gut contents were described. Detected
prey was identified to the lowest possible taxonomic level and photographed using a digital
camera connected to a dissecting microscope (Leica DFC 320).
2.4.6 Food-containing ratio and feeding rate
The food-containing ratio (FCR) is the proportion of individuals in a population with food in
their gut. Some only include chaetognaths containing identifiable prey in the FCR calculation
(FCRmin, e.g. Falkenhaug 1991, Kruse et al. 2010). However, this approach may not account
for loss of prey items from guts during net towing, due to damage or stress-induced
regurgitation (Baier & Purcell 1997, see ‘Discussion’). Other studies also included
individuals with other signs of recent prey digestion (gut lipids and debris, e.g. Sameoto 1987,
Froneman & Pakhomov 1998), which may give an upper estimate of the proportion feeding
(FCRmax). FCRmax measurements may not be appropriate for some chaetognath species, such
as those that contain oil vacuoles in the centre of their bodies. This includes another Arctic
species, Eukrohnia hamata (Möbius 1875), in which oil vacuoles may be for storage or
buoyancy (Øresland 1990, Pond 2012, pers. obs.). However, these oil vacuoles do not occur
in Parasagitta elegans. We calculated both FCRmax and FCRmin for P. elegans from each
haul. We also calculated feeding rates (FR: no. of prey items consumed ind.-1 day-1) according
27
to Eq. (2.1). Only individuals containing identifiable prey were included in the FR
calculation.
FR =𝑛prey x 24
tdig (2.1)
where nprey = mean no. of identifiable prey per chaetognath, and tdig = digestion time in hours.
Feigenbaum (1982) suggested a tdig of 10.2 h for Parasagitta elegans from a laboratory study
on starved specimens from Vineyard Sound, maintained at 0 ºC. As the water temperature in
all our study fjords was close to 0 ºC (Appendix B), we used Feigenbaum’s tdig estimate.
Proportions of individuals per haul containing different gut types were analysed using
Kruskal–Wallis tests.
2.4.7 Stable isotope analyses
As the ratios of 13C/12C and 15N/14N in organisms at different trophic levels tend to differ
considerably, stable isotope analyses can be used to examine marine food web structure and
the transfer of energy between trophic levels (McConnaughey & McRoy 1979). Stable
isotope analyses were performed on our 2012 samples at the Institute for Energy Technology
in Kjeller, Norway, using similar methods to Søreide et al. (2006). Three replicate samples
each containing 25 Parasagitta elegans were analysed from seven of the MIK hauls, whilst
six replicate samples of 25 inds. were analysed from an eighth MIK haul at 225 m in
Rijpfjorden (Appendix A). All P. elegans had body lengths within the range of 10-50 mm.
The whole body of each chaetognath was used, except lipids and non-dietary carbon (i.e.
carbonates), which were removed before analyses by Soxhlet extraction with CH2Cl2. Lipids
have notably lower levels of 13C than proteins and carbohydrates (van Dongen et al. 2002),
and their removal reduces a main source of measurement variability between individuals
(Hobson & Welch 1992). C/N ratios were expressed as the deviation from standards in ppt
(‰) according to Eq. (2.2) (Søreide et al. 2006).
28
δX=[(𝑅sample/𝑅standard) − 1]×1000 (2.2)
where X = 13C or 15N and R = the corresponding ratios 13C/12C or 15N/14N. International
standards, Pee Dee Belemnite for δ13C (PDB: USGS 24), and atmospheric air for δ15N
(IAEA-N-1 and 2) were used to determine R. Carbon and nitrogen composition were
expressed as percentages of animal dry weight.
2.4.8 Determination of trophic level
The trophic level (TL) of Parasagitta elegans in each fjord was calculated as the difference
between its average δ15N content and that of the winter food web baseline, assuming a
constant fractionation between trophic levels [Eq. (2.3), Søreide et al. 2006].
TL =∝ +δ15N 𝑃.𝑒𝑙𝑒𝑔𝑎𝑛𝑠− δ15N 𝐶.𝑔𝑙𝑎𝑐𝑖𝑎𝑙𝑖𝑠
∆N (2.3)
where α = trophic level of the food web baseline and DN = the trophic enrichment factor for
δ15N (average amplification) per trophic level. We took the abundant grazer Calanus
glacialis (α = 2) to represent the winter food web baseline. This decision was made because
Parasagitta elegans are thought to be carnivores that typically do not feed on primary
production but feed often on Calanus, and primary production is anyway low in winter (pers.
comm.: J Søreide).
We used a δ15N value for Calanus glacialis of 9.6 ± 0.2 ‰, estimated for individuals from
300 m in Svalbard fjords during December (Søreide et al. 2008). We used Δ = 3.4 ‰, also
determined for the European Arctic by Søreide et al. (2006).
2.4.9 Fatty acid analyses
Groups of primary producers and some herbivores produce fatty acids that are unique to
them, known as fatty acid trophic markers (FATMs, Dalsgaard et al. 2003). Higher
consumers possess a lower capacity to synthesise their own fatty acids, or to modify those
received from their prey. Therefore, when FATMs persist in a predator for some time with
little modification, they can be used to quantify its diet (Dalsgaard et al. 2003).
29
Determination of the fatty acid signatures of Parasagitta elegans from Isfjorden and
Rijpfjorden (in 2012) were performed on triplicate samples from nine MIK hauls (Appendix
A) at UNILAB, Tromsø, Norway, using similar methods to Wold et al. (2011b). Each sample
contained 10 pooled individuals with dry weights between 0.001 and 0.05 g. Total lipid was
extracted in 15 ml 2:1 chloroform–methanol with butylated hydroxytoluene (BHT) (Folch et
al. 1957). Each sample was supplemented with a known amount of the fatty acid 21:0, as an
internal standard, and trans-methylated in methanol containing 1 % sulphuric acid with
toluene for 16 h at 50 ºC. The relative compositions (%) of FA methyl esters were determined
on an Agilent 6890 N gas chromatograph, equipped with a fused silica, wall-coated capillary
column with an Agilent 7683 injector and flame ionisation detection. The fatty acid methyl
esters were identified and quantified by gas chromatography. Results are given as relative
percentages of the various fatty acids identified in specimens from the two fjords. Differences
in average fatty acids proportions between sampled depths in Isfjorden and Rijpfjorden were
analysed using one-way ANOVA. Differences in the fatty acid profile between fjords was
analysed using the Mann-Whitney U test (sum rank test).
2.4.10 Mid-winter maturity status
Chaetognaths are hermaphrodites possessing male and female gonads (Alvarino 1992). The
male gonads (testes and seminal vesicles) produce and secrete sperm, whilst the female
gonads (ovaries and seminal receptacles) produce ova and receive sperm from a sexual
partner (Alvarino 1992). Mature Parasagitta elegans are characterised by advanced ovaries
containing large oocytes, high sperm loads filling the tail section of the animal, and pairs of
pronounced seminal receptacles and vesicles (Russell 1932, Choe et al. 2003). We described
the maturity of 29 of the largest individuals (40-51 mm, 8×1 mm size classes), and in 323
smaller individuals (13-39 mm, 26×1 mm size classes) in MIK samples from all fjords (both
years, Appendix A). Measured individuals were stained with borax carmine solution to
highlight their gonads (Pierce 1941). Maturity assessments were made under the binocular
microscope following the methods of Grigor et al. (2014). Ovaries were measured to the
nearest 0.1 mm, and individuals showing advanced ovary development were taken as those
with ovaries ≥5.4 mm, whilst shorter ovaries ˂5.4 mm were considered to be poorly
developed. The volume of loose sperm in the tail was estimated to the nearest 25 %. Low
30
sperm loads could suggest that sperm is filling the tail or has already been released. However,
when sperm has already been released, remaining sperm appears more sparsely distributed.
Therefore, spent individuals can be separated from those which have not yet secreted sperm.
The size of the seminal receptacles was also described (see Grigor et al. 2014 for further
details).
2.5 Results
2.5.1 Chaetognath abundance and prey field
In Rijpfjorden in 2012, the most abundant zooplankton taxa based on the MPS sampling were
the larger calanoid copepod Calanus finmarchicus and the smaller copepods Pseudocalanus
spp. (Calanoida) and Oithona similis (Cyclopoida) (Table 2.1). Parasagitta elegans was the
most abundant chaetognath, but overall chaetognaths were also less abundant than the non-
copepod taxa Oikopleura spp. (Tunicata) and Beroe cucumis (Ctenophora) (Table 2.1).
Average Parasagitta elegans abundances in Rijpfjorden MIK trawls ranged from 2.4 ± 1.2
ind. m-3 (225 m) to 14.7 ± 7.0 ind. m-3 (75 m), comparing relatively well with the MPS results.
For further details on the polar night zooplankton community in Rijpfjorden, see Webster et
al. (2013), Kraft et al. (2013), and Daase et al. (2014).
31
Table 2.1 Total water-column abundances (ind. m-3) of a polar night zooplankton community
(Rijpfjorden 2012), ordered according to abundance per taxonomic group. Net sampling
(Multi-Plankton Sampler; 0.25-m2 opening, 0.2-mm mesh) was used. As larger chaetognaths
may have avoided the smaller MPS net (see Grigor et al. 2014), chaetognath abundances
presented here are likely to be underestimates. Mean abundances for species and copepod
stages were first calculated over two hauls (one at midday and the other at midnight at
various depth intervals, see Appendix A), and data were summed across all sampling depths.
Copepod stages are CI-CV, AM (adult male) and AF (adult female). Functional (feeding)
groups were extracted from Søreide et al. (2003). “Small Calanoida” comprised the
following taxa: Acartia longiremis, Aetideidae CI-CIII, Bradyidius similis, Microcalanus
spp. and Pseudocalanus spp. Only taxa with abundances of ≥0.1 ind. m-3 are shown.
Taxonomic group Functional (feeding) group Abundance (ind. m-3)
Cyclopoida (Copepoda) Omnivores 1467.6
Small Calanoida (Copepoda) Omnivores 1257.5
Calanus spp. (Copepoda) CI-AF Herbivores 881.5
Metridia longa Omnivore 78.6
Tunicata Variable between species 36.9
Ctenophora Carnivores 23.5
Limacina helicina (Pteropoda) Herbivore 17.3
Parasagitta elegans (Chaetognatha) Carnivore 5.5
Clione limacina (Pteropoda) Carnivore 3.9
Other Mollusca Variable between species 3.9
Isopoda Variable between species 3.4
Eukrohnia hamata (Chaetognatha) Carnivore 1.4
Travisiopsis sp. (Polychaeta) Carnivores 1.2
Harpacticoida (Copepoda) Variable between species 0.9
Echinodermata Variable between species 0.6
Hydrozoan medusae Variable between species 0.6
Euphasiacea Variable between species 0.3
Apherusa glacialis (Amphipoda) Herbivore 0.1
Carnivorous Calanoid copepods Carnivores 0.1
Pseudomma truncatum (Mysidacea) Omnivore 0.1
Ostracoda Variable between species 0.1
32
2.5.2 Gut contents
Observed gut contents were copepods, chitinous debris, lipid droplets, and other detritus that
could not be identified. The proportions of Parasagitta elegans with gut contents (FCRmax)
varied between fjords and years (Kruskal-Wallis test, P < 0.01), ranging from 9 to 53 %
(Figure 2.2). Some individuals contained two or more gut content types. Lipid droplets were
the most common gut observation overall (Figure 2.3 and Figure 2.4), observed in 106 (11.7
%) of the 903 chaetognaths. A total of 33 individuals (3.7 %) contained identifiable copepod
prey, including Calanus finmarchicus, Metridia longa, and harpacticoid copepods.
Proportions containing prey (FCRmin) also varied between fjords and years (Kruskal-Wallis
test, P ˂ 0.05), ranging from 0 to 10 % (Figure 2.2). FRs ranged from 0.00 to 0.24 prey ind.-
1 day-1 (mean = 0.12 prey ind.-1 day-1). Amongst feeding P. elegans, median per haul
proportions with prey varied with fjord (Kruskal-Wallis test, P ˂ 0.005), but proportions with
other gut contents did not (P ˃ 0.05, Figure 2.3). The relationship between chaetognath head
width and body length was linear (y = 0.031x + 0.37, R2 = 0.79), and prey was identified in
individuals with head widths ≥0.87 mm (Figure 2.4). Per haul proportions of P. elegans with
gut contents increased with head width size class (Kruskal-Wallis test, P ˂ 0.05, Figure 2.4),
but amongst feeders, proportions with each gut content type did not vary with head width (P
˃ 0.05, Figure 2.4).
Figure 2.2 Proportions (%) of Parasagitta elegans individuals per haul with gut contents
(FCRmax), identifiable prey (FCRmin), and empty guts in each fjord. The horizontal line inside
each boxplot shows the median of the proportions over multiple haul samples in a fjord. The
lower and upper boxes show the lower and upper quartiles, respectively, and the vertical
lines outside the boxes the differences between these quartiles and the lowest and highest
33
proportions observed. Each dot represents an outlying data point. nhauls = numbers of hauls
for each fjord. Hauls with ˂3 individuals analysed were not included. As only one haul was
analysed for Rijpfjorden in 2013, full boxplots could not be shown. See Appendix A for
numbers of individuals analysed per haul.
Figure 2.3 Proportions (%) of feeding Parasagitta elegans individuals per haul in each fjord
with different types of gut content. For details on the features of the boxplots and the data,
see Figure 2.2.
Figure 2.4 Gut contents in ascending head width size classes: proportions of Parasagitta
elegans (%) per haul with gut contents and of feeders with each gut content type. Includes
all dissected specimens from Isfjorden (50 individuals, 4 hauls) and Rijpfjorden (152
individuals, 13 hauls) in 2012. For details on the features of the boxplots and the data, see
Figure 2.2. ninds. = total numbers of individuals for each size class.
34
2.5.3 Body composition
Values for carbon and nitrogen isotopes varied little between fjords and sampling depths
(Table 2.2). The δ13C content of Parasagitta elegans ranged from -22.0 ± 0.3 ‰ (Rijpfjorden)
to -21.5 ± 0.2 ‰ (Isfjorden), whilst δ15N content ranged from 12.5 ± 0.3 % to 12.9 ± 0.1 ‰
(both Isfjorden). Average trophic level (TL) based on the δ15N content was 2.9, and average
C/N ratio over fjords and depths was 3.1 (Table 2.2).
Table 2.2 Stable carbon and nitrogen isotope values for Parasagitta elegans sampled by the
MIK (3.14-m2 opening, 1.5-mm mesh) at various trawl depths (20, 30, 35, 60, 75 and 225 m)
in Isfjorden and Rijpfjorden (2012). The average δ13C and δ15N composition (‰) in replicate
samples (usually three but six from 225 m in Rijpfjorden) containing 25 pooled individuals
(10-50 mm), average proportions of animal dry weight (DW) comprising carbon and
nitrogen (%), and C/N weight ratios. All values are accompanied by standard deviations.
Trophic levels (TL) were calculated for P. elegans from each fjord from mean δ15N (‰)
values (see ‘Method’).
Parasagitta elegans fatty acid signature did not differ between Isfjorden and Rijpfjorden
(Mann-Whitney U test, P ˃ 0.05). Similarly, percentage composition of almost all fatty acids
did not differ between sampling depths in the two fjords (one-way ANOVA, P ˃ 0.05). The
high levels of 18:1 (n-9) compared with those of 18:1 (n-7) strongly indicate carnivory. The
Calanus fatty acid marker 20:1 (n-9) and 22:1 (n-11) were both abundant. The dinoflagellate
marker docosahexaenoic acid (DHA) 22:6 (n-3) was recorded in interestingly high amounts,
Location Trawl depth (m) δ13C (‰) δ15N (‰) DW%C DW%N C/N TL
Mouth of Isfjorden 250 -21.7±0.0 12.5±0.3 48.4±0.5 15.6±0.4 3.1±0.0 2.9
Isfjorden (ISA) 30 -21.5±0.2 12.9±0.1 48.4±0.4 15.5±0.1 3.1±0.0 3.0
-"- 35 -21.5±0.1 12.8±0.2 47.9±1.1 15.4±0.4 3.1±0.0 2.9
-"- 60 -21.6±0.1 12.9±0.1 48.3±0.8 15.5±0.4 3.1±0.0 3.0
Rijpfjorden 20 -22.0±0.0 12.5±0.2 48.7±0.3 15.8±0.1 3.1±0.0 2.9
-"- 75 -21.8±0.2 12.5±0.2 48.0±0.2 15.4±0.0 3.1±0.0 2.9
-"- 75 -22.0±0.3 12.6±0.3 48.9±0.4 15.7±0.2 3.1±0.0 2.9
-"- 225 -21.8±0.1 12.5±0.1 48.6±0.4 15.8±0.2 3.1±0.0 2.9
35
whilst eicosapentaenoic acid (EPA) 20:5 (n-3) was recorded in moderate to high amounts
(Table 2.3).
Table 2.3 Average fatty acid profile for Parasagitta elegans in 2012. Results are given as
average percentages of the various fatty acids identified across all samples from Isfjorden
and Rijpfjorden (see ‘Method’), alongside the standard deviations. Only fatty acids with
mean percentages of =>0.5 ± 0.1 across both fjords are shown. In Isfjorden, the mean
percentages of 15:0 FA and 18.2(n-6) FA differed between sampling depths (indicated by a
† symbol, one-way ANOVA, P ˂ 0.05). In Rijpfjorden, the proportion of every fatty acid was
similar between sampling depths (one-way ANOVA, P ˃ 0.05).
Fatty acid Mean % Isfjorden
(n samples = 12)
Mean % Rijpfjorden
(n samples = 17)
14:0 FA 5.02±2.09 4.13±0.62
14:1 (n-5) FA 0.54±0.06 0.52±0.08
15:0 FA 0.72±0.07† 0.73±0.06
16:0 FA 11.91±1.16 12.65±1.47
16:1 (n-5) FA 2.97±0.41 3.30±0.39
16:1 (n-7) FA 7.13±0.27 6.05±0.33
18:0 FA 1.09±0.13 1.18±0.20
18:1 (n-7) FA 1.95±0.28 1.74±0.18
18:1 (n-9) FA 5.35±0.65 5.82±0.54
18:2 (n-6) FA 1.28±0.11† 1.35±0.09
18:3 (n-3) FA 1.11±0.11 1.37±0.07
18:4 (n-3) FA 1.76±0.63 2.35±0.35
20:1 (n-9) FA 14.80±1.02 11.46±1.71
20:4 (n-3) FA 0.82±0.10 0.99±0.07
20:5 (n-3) FA (EPA) 11.41±0.68 12.73±0.75
22:1 (n-11) FA 6.77±1.38 5.69±0.71
22:1 (n-7) FA 0.47±0.02 0.78±0.30
22:5 (n-3) FA 0.60±0.14 0.69±0.15
22:6 (n-3) FA (DHA) 18.01±2.33 18.81±1.99
24:1 (n-9) FA 2.88±0.21 3.81±0.62
36
2.5.4 Mid-winter maturity status
Amongst the largest individuals in the population (body lengths 40-51 mm), 55 % had well-
developed seminal receptacles, whereas 93 % had relatively high sperm volumes in their tails
(50-100 %) and all had advanced ovaries (≥5.4 mm). In smaller individuals (lengths 13-39
mm), 45 % had well-developed seminal receptacles and 42 % had advanced ovaries; 80 %
had synthesized relatively high sperm volumes (filling 50-100 % of the tail area).
2.6 Discussion
2.6.1 Studies during the polar night
Studies of plankton ecology in the high Arctic are typically restricted to spring and summer,
due to the logistical difficulties of sampling during winter. The polar night cruise, of which
our study formed a part, offered unique possibilities for a better understanding of polar night
marine ecology (see Berge et al. 2012, Webster et al. 2013, Daase et al. 2014).
We show that the common chaetognath Parasagitta elegans remains an active carnivore
during the polar night. This arrow worm is not in a dormant and non-feeding state although
its feeding rates may be considerably lower than in spring and summer, and reproduction is
absent (or occurring at very low rates) at this time of year. These observations add to the
increasing awareness of activity levels and ecological interactions of pelagic organisms
during the polar night.
2.6.2 Feeding activity and rates
Copepods are abundant in Svalbard fjords during winter (Table 2.1) and as a non-visual
predator Parasagitta elegans should, as opposed to fish and other visual predators, be able
to encounter and catch them also during the polar night. The behaviour of some copepods
during the polar night (i.e. diapausing in an unalert state) could make them particularly
susceptible to predators such as chaetognaths (Darnis et al. 2012). About a quarter of the P.
elegans individuals showed signs of recent feeding (mainly lipid droplets). The body of P.
elegans does not contain a centralised oil vacuole, suggesting that all lipid droplets in P.
elegans guts remained from recently digested prey, yet only 4 % contained identifiable prey.
37
Based on Feigenbaum’s (1982) digestion time estimate of 10.2 h at 0 ºC (likely longer in
colder waters), our findings would suggest that most individuals had not fed for several hours
before their capture. In contrast, Falkenhaug (1991) identified prey in 36 % of the P. elegans
population. collected from the Barents Sea in summer. Our average estimate of per capita
feeding in P. elegans was 0.12 prey ind.-1 day-1, corresponding to 0.66 prey ind.-1 m-3
consumed per day by the P. elegans population (based on the abundance data in Table 2.1).
Their predation impact on Calanus is therefore low given the high Calanus abundances
(Table 2.1, see also Daase et al. 2014). Calanus are assumed to be in a dormant, non-feeding
state during winter (Falk-Petersen et al. 2009). Daase et al. (2014) reported on Calanus from
the same cruise in 2012 and found that the Calanus finmarchicus population in Rijpfjorden
comprised mainly copepodite stage CV and some CIVs, which could indicate overwintering.
However, these authors also noted that “the bulk of the C. finmarchicus and C. glacialis
population was found close to the surface and not at greater depth where they presumably
should overwinter”, suggesting they were not in an unalert dormancy phase, at least not in
January. If not, these copepods may be more alert to the presence of predators than assumed,
allowing them to avoid or escape chaetognaths.
Our FR estimate is similar to that obtained for immature specimens in northern Sweden in
autumn-winter (0.2 prey ind.-1 day-1) and much lower than reported for spring-summer (0.7-
0.9 prey ind.-1 day-1, Øresland 1987). These findings suggest that feeding rates for
Parasagitta elegans at high-latitudes drop during winter, corresponding well with the
reduced growth rates observed during winter (Grigor et al. 2014), and the lack of reproduction
at this time of year (this study). In less seasonal environments, energetic requirements may
vary less between the seasons, accounting for relatively higher feeding rates at lower
latitudes, also during winter and early spring (e.g. up to 1.33 prey ind.-1 day-1 in Vineyard
Sound, Feigenbaum 1982).
However, care should be taken when comparing estimates of feeding rates between studies,
because each study detects prey with various levels of precision. For example, we did not
search for mandible remains in guts to detect further signs of recent copepod digestion, as in
38
other studies (e.g. Falkenhaug 1991, Giesecke and Gonzalez 2004). Feeding estimates in
chaetognaths are also highly sensitive to sampling methodology. As well as the risk of
damage to their fragile bodies, stressed chaetognaths may also regurgitate gut contents,
leading to underestimates of true feeding rates. Baier & Purcell (1997) estimated prey loss
from guts of ~50 % when tows were longer than 2 min. Such short hauls can be unfeasible,
especially when using large trawl nets such as the MIK, and when sampling populations in
deeper waters. Further studies should therefore utilize new zooplankton imaging devices for
observing chaetognaths in the water column without necessarily capturing them in nets.
Optical methods are promising avenues (e.g. Schulz et al. 2010, Sainmont et al. 2014b).
2.6.3 Energetics
Stable isotope and FATM analyses confirmed the position of Parasagitta elegans as a
predator during the polar night. From its average trophic level (TL) of 2.9, it can be classified
as a carnivore according to a trophic model devised for the European Arctic (Søreide et al.
2006, in which carnivores had TLs between 2.9 and 3.3). δ15N (an indicator of protein
content) and δ13C (an indicator of organic matter content) values varied little with station or
depth, and agree well with values from the Barents Sea in March (Søreide et al. 2006). δ15N
values were, however, lower than reported from the Bering Sea (14.7 ± 0.7 ‰, Lovvorn et
al. 2005), suggesting that P. elegans in the sub-Arctic Pacific typically feed higher up the
food chain (also see ‘Lipid profile’ section of ‘Discussion’). Many factors affect the
elemental composition of zooplankton species, including age, size maturity status,
reproductive strategies, as well as variations in the composition and growth rates of primary
producers (Ikeda 1974), yet for P. elegans in the Barents Sea, δ15N values seem to vary little
throughout the year. Søreide et al. (2006) reported δ15N values ranging from 11.9 ± 0.2 ‰ in
spring to 12.2 ± 0.1 ‰ in winter. δ13C values varied slightly more between spring (-19.3 ±
0.8 ‰) and winter (-20.8 ± 0.3 ‰).
2.6.4 Lipid profile
The high levels of the FATMs 20:1 (n-9) and 22:1 (n-11) confirm that Parasagitta elegans
is part of the Arctic Calanus-based food web (Falk-Petersen et al. 2007, Wold et al. 2011b).
39
Furthermore, the high level of 22:6 (n-3) indicates that the base of the food chain is dominated
by dinoflagellates, which can be very abundant in waters north of Svalbard in spring-summer
(Hegseth & Sundfjord 2008). This lipid signature agrees well with previous results from the
European sub-Arctic (Falk-Petersen et al. 1987). Both the presence of green detritus in P.
elegans guts, and the surprisingly high levels of the dinoflagellate fatty acid marker
docosahexaenoic acid, may suggest that some omnivory and/or detritivory occurs. Non-
carnivorous feeding in chaetognaths has been suggested by Casanova et al. (2012). In the
Canadian Arctic, Eukrohnia hamata and Pseudosagitta maxima have been observed
ingesting green detritus under the microscope (pers. obs.). Eukrohnia species in Antarctica
were found to contain higher amounts of 16:0, reflecting feeding on the Antarctic copepods
including Rhincalanus gigas (Kruse et al. 2010). We suggest that winter feeding is captured
in these results, following the suggestions of Graeve et al. (2005) that a new signal (source
of food) will be visible relatively quickly (~4-8 days after feeding). If P. elegans starves
during autumn and early winter, and if 22:6 (n-3) undergoes little transformation or
metabolism (Dalsgaard et al. 2003), it remains possible that this signal is retained from
feeding on Calanus during a previous summer or autumn bloom (Falk-Petersen et al. 1990,
Wold et al. 2011b). However, this study and others (e.g. Feigenbaum 1982, Øresland 1987,
Falkenhaug 1991) suggest a low likelihood of long-term fasting in P. elegans.
An important difference between the two main chaetognath species in Arctic waters,
Eukrohnia hamata and Parasagitta elegans, is that the former typically possess oil vacuoles
in the centre of their bodies, whilst the latter do not (Øresland 1990, Pond 2012, pers. obs.).
Previous studies that considered the presence of oil vacuoles in this species to reflect recent
feeding may therefore have overestimated feeding rates (e.g. Sameoto 1987, Froneman and
Pakhomov 1998). The role of these vacuoles in E. hamata (e.g. buoyancy, storage) is not yet
clear (Pond 2012), but unlike P. elegans, E. hamata has a cosmopolitan range. In the Arctic,
both species commonly occur at epi-pelagic depths (Bieri 1959), but in the North Pacific, E.
hamata populations are commonly found residing deeper, and throughout a wider depth
range than P. elegans (e.g. Bieri 1959, Alvarino 1964). Maintaining such wide vertical
distributions would certainly require a strong control of buoyancy, which could be offered
by having centrally positioned oil vacuoles (Pond 2012). Lipid reserves form a central
40
component of the life history of polar zooplankton species (Falk-Petersen et al. 2009, Varpe
et al. 2009). In Antarctica, 34 % of examined E. bathyantarctica individuals were found to
contain oil droplets in summer compared to 57 % of individuals in winter. This species also
contained relatively high amounts of the fatty acid 18:1 (n-9), which is found in storage lipids
(Kruse et al. 2010). If the primary role of oil vacuoles is storage, this could suggest that
survival and possibly reproduction in E. hamata is less dependent on concurrent food intake
than in P. elegans. Studies of the extent of capital breeding (Varpe et al. 2009) in E. hamata
are therefore needed.
2.6.5 Reproduction
Small Parasagitta elegans <10 mm were absent from MPS samples from January, and whilst
many individuals above 20 mm had synthesised high sperm loads, many of the largest P.
elegans specimens in the nets (40-51 mm) still lacked well developed seminal receptacles,
suggesting that they were not fully mature (Russell 1932, Choe et al. 2003). Grigor et al.
(2014) frequently observed pronounced receptacles in individuals ≥20 mm from February to
May, after which they disappeared. In the Arctic, breeding of P. elegans generally takes place
in spring and summer (Kramp 1939, Ussing 1939, Bogorov 1940, Grigor et al. 2014); this is
in contrast to Eukrohnia hamata, which may also reproduce in winter (pers. obs.). Saito &
Kiørboe (2001) showed that P. elegans <5 mm in the North Sea fed almost exclusively on
prey <350 μm in length. In Svalbard, the prey in this size range is represented by small
cyclopoids such as Oithona similis, as well as Calanus nauplii and the young Calanus stages.
In winter, individuals may be waiting for increased food input before they reproduce or for
suitable food for the young and newborns to feed on (in terms of size and availability). By
investing energy into maturation during winter, egg hatching can be scheduled to coincide
with the reproduction of a wide range of copepod prey in spring and summer, and the
buoyancy of chaetognath eggs may also allow them to hatch in shallow waters (Hagen 1999
and references therein) amongst their grazing prey. In another fjord on Svalbard, large
numbers of P. elegans eggs became visible in the water column in March 2003, suggesting
that conditions for reproduction begin to improve at this time of year (Hirche & Kosobokova
2011).
41
2.7 Concluding remarks
Knowledge of an organism’s activity level and foraging ecology outside of the windows of
the main primary production period (spring–summer) is key to establishing an understanding
of the full annual routine (Varpe 2012). Here, we have focused on the polar night feeding
ecology of a predatory zooplankter, adding to recent work on the life history and vertical
distribution (Grigor et al. 2014). We found the chaetognath Parasagitta elegans to feed
during the polar night, but with feeding rates lower in winter than have been reported from
other seasons. As growth rates (e.g. Dunbar 1962, Grigor et al. 2014) may also decrease at
this time and reproduction does not seem to occur, individuals should have lower-energy
requirements and require less food. Although several copepod taxa may rest at depth in an
unalert state during the Arctic winter, our study shows that mortality on copepods caused by
P. elegans in the water column is low at this time of year. This study did, however, not sample
the zone immediately above the seafloor, the hyperbenthic zone, where high densities of
chaetognaths are known to aggregate during winter (Choe & Deibel 2000), and where
abundances of resting copepods may also peak. The activities of P. elegans in this zone, as
well as those of the other Arctic species Eukrohnia hamata and Pseudosagitta maxima,
require more attention.
42
3. Chapter 3 – Growth and reproduction of the chaetognaths
Eukrohnia hamata and Parasagitta elegans in the Canadian Arctic
Ocean: capital breeding versus income breeding
3.1 Résumé
Dans les mers arctiques, la production primaire et l’accessibilité de la nourriture du
zooplancton varient fortement durant la courte période estivale. Nous avons testé l'hypothèse
selon laquelle Eukrohnia hamata et Parasagitta elegans, deux chaetognathes arctiques
similaires et sympatriques, partitionnent les ressources selon différentes stratégies de
reproduction. Les deux espèces avaient des longévités naturelles similaires d'environ 2 ans.
Espèce mésopélagique, E. hamata engendre deux couvées distinctes à l'automne et au
printemps. La production de jeunes coïncide avec une baisse de la fréquence d’E. hamata
présentant des réserves lipidiques visibles, ce qui est caractéristique d’une reproduction basée
sur les réserves. La croissance s’est avérée positive d'avril à janvier et négative en février-
mars. La croissance et la maturation étaient similaires pour les deux cohortes. Les réserves
lipidiques contenues dans une vacuole permettent à E. hamata de se reproduire et de croitre
en dehors de la courte saison de productivité. Espèce plus néritique, P. elegans produit une
couvée en été-automne, durant la production biologique maximale dans les eaux près de la
surface, un mode de reproduction basé sur l’apport immédiat d’énergie. Cependant, avec le
réchauffement climatique réchauffe, un bloom phytoplanctonique automnal pourrait
favoriser la couvée d'été-automne chez P. elegans.
43
3.2 Abstract
In Arctic seas, primary production and the availability of food to the zooplankton are strongly
pulsed over the short productive summer. We tested the hypothesis that Eukrohnia hamata
and Parasagitta elegans, two similar and sympatric arctic chaetognaths, partition resources
through different reproductive strategies. The two species had similar natural longevities of
around 2 years. The meso-pelagic E. hamata spawned two distinct broods in autumn and
spring. Offspring production coincided with drops in the frequency of E. hamata with visible
lipid reserves, characteristic of capital breeders. Growth was positive from April to January
and negative in February and March. Growth and maturation were similar for the two broods.
Storage reserves contained in an oil vacuole may allow E. hamata to reproduce and grow
outside the short production season. The neritic P. elegans produced one brood in summer-
autumn during peak production in near-surface waters, characteristic of income breeders.
However, as the Arctic warms, the development of an autumn phytoplankton bloom could
favour the summer-autumn brood of P. elegans.
44
3.3 Introduction
Arrow worms or chaetognaths form a phylum of gelatinous zooplankton represented by ~200
species worldwide, with biomass estimated at 10-30 % that of copepods (Bone et al. 1991).
They can represent a significant fraction of the diet of many animals such as amphipods (e.g.
Gibbons et al. 1992), other chaetognaths (e.g. Pearre 1982), seabirds (e.g. Mehlum and
Gabrielsen 1993), and are the preferred prey of the larvae of some tropical fish and
commercially important decapods (e.g. Sampey et al. 2007, Saunders et al. 2012).
Chaetognaths are hermaphrodites. Spermatogonia bud off from testes parallel to the tail walls
to produce spermatocytes, which are transmitted to a conspecific to fertilise its oocytes
(Alvarino 1992, Bergey et al. 1994). Each chaetognath possesses one pair of seminal vesicles
on the tail segment and one pair of seminal receptacles at the posterior ends of the oviducts.
Two individuals first come into contact with each other, before sperm is passed from the
seminal vesicles of one individual to the seminal receptacles of the other (Goto & Yoshida
1985). Hatching strategies vary amongst species. For instance, Parasagitta elegans releases
buoyant eggs that hatch near the surface where small prey is abundant (Kotori 1975, Hagen
1985). Eukrohnia hamata broods its eggs in an external sac from which the young later swim
out, often at depth (Alvarino 1968 and references therein).
In contrast to the high diversity of chaetognaths in other seas (e.g. De Souza et al. 2014), only
three species are frequently reported in Arctic plankton surveys. Parasagitta elegans is a
neritic species, often peaking in abundance in epi-pelagic waters; Eukrohnia hamata is
abundant in meso-pelagic and deep waters; and Pseudosagitta maxima, growing much larger
(up to 90 mm) than the other species (40-45 mm), is typically bathy-pelagic but may also
occur near the surface in the Arctic (Bieri 1959, Alvarino 1964, Terazaki & Miller 1986,
Sameoto 1987). A fourth species, Heterokrohnia involucrum has also been recorded at bathy-
pelagic depths, so far only in the Arctic Ocean (Dawson 1968). Whilst their contribution to
higher trophic levels is poorly documented, arctic chaetognaths may consume an important
fraction of copepod biomass. Although admittedly little better than a guess, Welch et al.
45
(1992) estimate that chaetognaths in Lancaster Sound ingest 51 % of the copepod biomass
annually (164 of 319 kJ m-2 yr-1).
At high arctic latitudes, resource availability is strongly pulsed seasonally, with maximum
phytoplankton and zooplankton biomass occurring during the short ice-free season in late
summer and autumn (e.g. Falk-Petersen et al. 2007, Falk-Petersen et al. 2009, Søreide et al.
2010). Here, the co-existence of similar species may depend on the seasonal partitioning of
resources, which can be achieved through differences in vertical distribution, diet and
reproductive strategies. For instance, the reproductive strategies of the two dominant arctic
herbivorous copepods differ markedly in ice-covered waters. The large capital-breeder
Calanus hyperboreus reproduces in winter, fuelling egg production with lipids accumulated
in summer (e.g. Conover 1967, Hirche & Niehoff 1996, Pasternak et al. 2001). Calanus
glacialis may combine lipid stores and high-quality food to fuel reproduction (e.g. Conover
1988, Sainmont et al. 2014a). Income breeders do not synthesise reserves as fuel for
reproduction at a later time. Peak reproduction occurs in spring-summer in the epi-pelagic
Parasagitta elegans (e.g. Kramp 1939, Sameoto 1971, Grigor et al. 2014), which suggests
income breeding with the summer maximum in prey abundance fuelling reproduction. By
contrast, year-round breeding in Gerlache Strait, Antarctica (Øresland 1995), and the
accumulation of lipids and wax esters in an oil vacuole (Pond 2012) suggest capital breeding
fuelled by lipid reserves in E. hamata.
We describe the life histories of Eukrohnia hamata and Parasagitta elegans over an annual
cycle based on weekly sampling of zooplankton in the Amundsen Gulf (Beaufort Sea) from
August 2007 to July 2008, complemented by collections from other areas of the Canadian
Arctic in autumn of the two years. In particular, growth of size cohorts, reproduction, and oil
reserves are tracked to explore the hypothesis that E. hamata is a capital breeder that spawns
during most of the year, whilst P. elegans is an income breeder, reproducing during periods
of high prey availability.
46
3.4 Method
3.4.1 Study area
Sampling was conducted on-board the CCGS Amundsen, primarily from October 2007 to
August 2008 in the Beaufort Sea (Figure 3.1). To complete the annual cycle of observations,
additional collections from the Labrador Sea, the Canadian archipelago and Baffin Bay were
included in the analyses (Figure 3.1). In addition to the 27 stations sampled at weekly or
higher resolution in the Amundsen Gulf region (69-72°N, 121-131°W) from November 2007
to August 2008, two stations were sampled in Nachvak Fjord in August 2007, two stations
in Parry Channel in October 2007, and two stations in northern Baffin Bay in September
2008 (Figure 3.1 and Appendix C). Amundsen Gulf, our main sampling region, is a 400 km
long, 170 km wide channel with a maximum bottom depth of ~630 m that connects the south-
eastern part of the Beaufort Sea to the Canadian archipelago. Amundsen Gulf is typically
covered with sea-ice from October to early June (Barber & Hanesiak 2004). Three water
masses are detected in the Amundsen Gulf (Geoffroy et al. 2011 and references therein); the
Pacific Mixed layer (PML; 0-60 m), the Pacific Halocline (PH; 60-200 m) and the Atlantic
layer (AL; ˃ 200 m). Nachvak Fjord is a pristine 45-km long sill-fjord in Nunatsiavut,
Northern Labrador, with a maximum depth of 210 m (Bell & Josenhans 1997, Simo-Matchim
et al. 2016). The deep semi-enclosed basin of Baffin Bay lies further north, and is connected
via Parry Channel to the Beaufort Sea in the west (Figure 3.1).
47
Figure 3.1 Bathymetric maps of the Canadian Arctic Ocean indicating the regions, and
positions of stations (black circles) where chaetognaths were sampled from August 2007 to
September 2008. Station IDs provided.
3.4.2 Sampling
In the Amundsen Gulf, estimates of weekly profiles of temperature and salinity between
November 2007 and July 2008 are from Geoffroy et al. (2011), and those of chlorophyll a
(chl a) biomass are from Darnis & Fortier (2014). Salinity, and temperature profiles of the
water column at single stations in Nachvak Fjord, Parry Channel and Baffin Bay, were
obtained using a conductivity-temperature-depth (CTD) system. We also collected seawater
samples from 9-10 depths in the upper 100 m, using the CTD rosette equipped with twenty-
four 12 1 Niskin-type bottles (OceanTest Equipment). Subsamples (500 ml) for the
determination of total chlorophyll a (chl a) were filtered onto 25 mm Whatman GF/F filters
48
(nominal porosity of 0.7 µm). Chl a was measured using a Turner Designs 10-AU
fluorometer, after 24 h extraction in 90 % acetone at 4 °C in the dark without grinding
(acidification method of Parsons et al. 1984).
Two similar samplers were used to collect zooplankton: a square-conical net with a 1 m2
opening area, 200 µm mesh and a rigid cod-end, and a Hydrobios® Multinet with 9 individual
opening and closing nets with 0.5 m2 openings, 200 µm mesh and rigid cod ends. At 12
stations, the 1 m2 net was deployed cod-end first (non-filtering) to 10 m above the seabed
and hauled back to the surface at a speed of 0.5 m s-1. At 22 stations, the Multinet was
deployed to 10 m above the seabed and retrieved at 0.5 m s-1, sampling sequentially over pre-
set depth intervals, the overall thickness of which varied from 100 to 520 m. Typically, 3×20-
m depth strata were sampled from 10 m above the seafloor upward, and 3×20-m depth strata
were sampled from 60 m depth to the surface. The remaining interval (from 70 m above the
bottom to 60 m below the surface) was then divided into three equal sampling layers
(Appendix C). Samples were fixed in 4 % formaldehyde-seawater solution buffered with
sodium borate.
3.4.3 Chaetognath body size and sampler efficiency
Chaetognaths were sorted from the samples, identified to species and when possible,
measured (nearest mm) from the top of the head to the tip of the tail, excluding the caudal
fin. Heavily damaged or broken individuals were excluded, but those missing heads only (~1
mm) were included in the analyses, as positive identification remained possible (Figure 3.2)
and length could be estimated. Out of 8179 chaetognaths sorted, 7245 chaetognaths (5918
Eukrohnia hamata and 1298 Parasagitta elegans were included. Twenty-nine (29)
Pseudosagitta maxima present in the samples were not analysed further. The relative
efficiency of the Multinet and square-conical net at capturing chaetognaths was assessed by
comparing the size frequency distribution of E. hamata or P. elegans in the two nets.
49
Figure 3.2 Illustrations and photographs of Eukrohnia hamata and Parasagitta elegans. (a)
Diagrams of the two species indicating maturity features and the centrally-positioned oil
vacuole in E. hamata. (b) Photographs of live E. hamata (top) and P. elegans (bottom) taken
in-situ by a zooplankton imager (Schmid et al. 2016) in the Canadian Arctic. Specimens ~20
mm. (c) Photograph of oocytes in a stained P. elegans individual. (d) Photograph of ovaries
in an E. hamata individual (imaged in-situ). (e) Photograph of tail sperm, seminal vesicles
and seminal receptacles in a stained P. elegans individual.
3.4.4 Hatching and cohort development
The occurrence of newborns (2-4 mm) in Multinet collections was used as an index of recent
hatching. The subsequent growth of the different cohorts was inferred visually from
successive monthly length frequency distributions in collections from both samplers. Lengths
from the Multinet collections were included twice in the histograms to give equal weight to
this sampler (0.5 m2 aperture) and the square-conical net (1 m2 aperture). Each cohort was
detected by visual means, and the MIXdist library in RTM (Du 2002) was used to estimate its
mean length (arithmetic mean), standard deviation and length range in each month. Monthly
50
growth rates of each cohort were calculated from changes in mean length. In most cases, a
cohort was clearly defined in the month length frequency distributions. In some cases, the
interpretation of cohorts was aided by two assumptions. First, based on published estimates
of growth (Welch et al. 1996, Choe & Deibel 2000, Grigor et al. 2014), we assumed that
monthly growth of a cohort could not exceed 7 mm mo-1. Second, the possibility that a cohort
was absent from the population in one month if clearly present during the preceding or
following month in the time series was excluded. Solutions aimed to minimise cohort length
overlaps. Goodness-of-fit was tested using the Chi-square statistic. Parasagitta elegans data
for August are from Nachvak Fjord in 2007 due to the scarcity of this species in the
Amundsen Gulf collections in that month in 2008.
3.4.5 Estimation of maturity and oil vacuole area
Eukrohnia hamata and Parasagitta elegans were stained with a Borax Carmine solution to
highlight gonads (Pierce 1941, Grigor et al. 2014). Oocytes (Figure 3.2) in single ovaries
were counted and diameters measured under the stereomicroscope. Ovary length, diameter
of the externally protruding part of the seminal receptacles and width of the seminal vesicles
(Figure 3.2) were measured to the nearest 0.01 mm. The distribution of
spermatogonia/spermatocytes in tails was characterised as absent, spermatogonia present
near walls only, or spermatocytes dispersed throughout the tail. The width of seminal vesicles
was measured to the nearest 0.01 mm. The presence or absence of an oil vacuole (Figure 3.2)
was noted in 2089 individuals of E. hamata. The width and height of the vacuole were
measured to the nearest 0.01 mm under the stereomicroscope. Area was calculated as
π×0.5width×0.5height. The presence of oil in the vacuole and/or oil droplets in the gut was
noted.
3.4.6 Vertical distributions
19 Multinet collections (typically 9 samples per haul), 1-2 per month from August 2007 to
September 2008, were analysed to estimate the abundances of Eukrohnia hamata and
Parasagitta elegans populations and age classes in discrete layers of the water column (ind.
m-3). Contour plots were produced in the R computing environment (R Development Core
51
Team 2008), using Akima bilinear interpolation performed vertically for every meter of the
water column. Assuming a lognormal distribution, species abundances A were log-
transformed as log10(A+1) prior to interpolation, also serving to preserve abundance A = 0
(Legendre & Legendre 2012). Vertical distributions of populations were also characterized
by their weighted mean depths in the water column [Zm, m, Eq. (3.1a)] with standard
deviations [Zs, m, Eq. (3.1b)] as described by Dupont & Aksnes (2012). Zm was normalized
between 0 and 1 to identify the positions of animals relative to a station’s bottom depth.
𝑍𝑚 = ∑ 𝑤𝑖𝑛𝑖=1 𝑑𝑖𝑧𝑖/ ∑ 𝑑𝑖
𝑛𝑖=1 𝑧 (3.1a)
𝑍𝑠 = √(∑ 𝑤𝑑1𝑛𝑖=1 𝑧1
2/ ∑ 𝑑1𝑧1𝑛𝑖=1 ) − 𝑊𝑀𝐷2 (3.1b)
Where wi is the abundance of animals in depth interval i, di is the thickness of interval i, and
zi is its mid-point.
3.5 Results
3.5.1 Physical environment and primary production in the Amundsen Gulf
From November 2007, onwards, the PML in the Amundsen Gulf had temperatures of -1.6 to
-0.6 ºC, but warmed to ˃ 9 ºC at some stations in June and July 2008 on top of a strong
thermocline. Throughout the study, temperatures in the PH were -1.6 to 0 ºC, and
temperatures in the AL were ~0 ºC. Salinities were 30-32 psu in the PML, 32-34.6 psu in the
PH, and ˃ 34.6 psu in the AL (Geoffroy et al. 2011). Ice algae was first detected in late March
in the PML and peaked in late April and early May (~10 mg m-3), when it was succeeded by
a surface phytoplankton bloom. In July, a subsurface chl a maximum (SCM) occurred at ~40
m (16 mg m-3), and the phytoplankton penetrated the PH (Darnis & Fortier 2014).
3.5.2 Physical environment and primary production in autumn (other sampling
locations)
In August 2007, a steep thermocline was observed in Nachvak Fjord between the surface and
60 m, with temperature decreasing from 3.4 °C to -1.6 °C (Appendix D). Chl a concentrations
peaked at 20 m (2.8 µg L-1). In October 2007, temperatures at our Parry Channel station rose
52
from ˂-1 °C at the surface to 0.4 °C at ~45 m, fell to ˂ 1 °C at 60 m, and then rose again from
-1.5 °C at 200 m to 0.7 °C at 500 m. Chl a concentrations remained below 0.5 µg L-1 at
sampled depths. In September 2008, temperatures at our Baffin Bay station rose from ˂-1 °C
at the surface to ˃ 0.3 °C at ~85 m, fell to ˂ 1.1 °C at 100 m, with smaller fluctuations in
temperature in deeper waters. Chl a concentrations peaked at 45 m (1.1 µg L-1). Strong
haloclines were observed in the upper 100 m at all three stations (Appendix D).
3.5.3 Abundances and vertical distributions of chaetognath species
Eukrohnia hamata was present at all stations in the Amundsen Gulf with abundances ranging
from 56 ind. m-2 in late July to 894 ind. m-2 in mid-April, based on Multinet collections.
Parasagitta elegans was less abundant than E. hamata at all stations in Amundsen Gulf (16
ind. m-2 in November to 244 ind. m-2 in December), and in Parry Channel (320 ind. m-2) and
Baffin Bay (64 ind. m-2) in October and September respectively. Pseudosagitta maxima
occurred in only 4 Multinet collections from the Amundsen Gulf, typically in the Atlantic
Layer, with maximum abundances of 4 ind. m-2. Relative to P. elegans, the abundance of E.
hamata increased with station depth (Figure 3.3a). E. hamata occurred primarily in the deep
AL of the Amundsen Gulf (˃ 200 m, Figure 3.3b), based on weighted mean depth, except on
two dates in late May and late July when the E. hamata population was centred in the PH
(60-200 m). In Parry Channel (October) and Baffin Bay (September), the E. hamata
population remained ˃ 200 m. In the Amundsen Gulf, seasonal vertical migration (SVM) was
most pronounced in P. elegans, which, based on weighed mean depth, resided primarily in
the PH from December to March, rose into the PML (0-60 m) in March/April during the
development of ice algae, and returned to the PH in late June (Figure 3.3b). P. elegans was
39 times more abundant than E. hamata in Nachvak Fjord in August (462 ind. m-2). At
Nachvak Fjord, Parry Channel and Baffin Bay, the P. elegans population remained ˂ 200 m
(Figure 3.3b).
53
Figure 3.3 a) Relative frequency of Eukrohnia hamata, Parasagitta elegans and Pseudosagitta
maxima in relation to bottom depth at Amundsen Gulf stations. Multinet and square-conical
net collections included. b) Weighted mean depths of E. hamata and P. elegans normalized
relative to the bottom depth at Amundsen Gulf stations (see ‘Method’). Multinet collections.
Standard deviation bars also given. The blue area indicates the Pacific Halocline (60-200
m) and the red area indicates the Atlantic Layer ˃ 200 m (Geoffroy et al. 2011).
3.5.4 Length distributions and sampler efficiency
Eukrohnia hamata in the Amundsen Gulf ranged in length from 2 to 40 mm (≤34 mm in
other sampling regions) and Parasagitta elegans from 2 to 42 mm (up to 45 mm in other
sampling regions). The length frequency distributions of each species were not significantly
different (Kolmogorov-Smirnov test, P ˃ 0.1) between the two samplers (Figure 3.4). The
few E. hamata and P. elegans ≥ 40 mm were caught solely by the larger-aperture square-
conical net.
54
Figure 3.4 Length frequency (mean % ± 1 SD) distributions of Eukrohnia hamata and
Parasagitta elegans in the square-conical (S-C) net (1 m2 aperture, 200 µm mesh) and
Multinet (0.5 m2 aperture, 200 µm mesh) in the Amundsen Gulf. Note the different scales for
the two species. k is the number of collections.
3.5.5 Timing of reproduction
The hatching seasons of the two chaetognath species were approximately complementary
over the annual cycle (Figure 3.5). Apart from the occurrence of newborns in October,
Eukrohnia hamata hatched from December to July with the production of newborns ramping
up from low values in December-January to a maximum in April, and stopping after July
(Figure 3.5). Except for their absence in our collections in November and January,
Parasagitta elegans newborns were observed continuously from July to February, with
hatching peaking in December (Figure 3.5).
55
Figure 3.5 Abundance (mean numbers m-2 + 1 SD) of newborn Eukrohnia hamata and
Parasagitta elegans (body lengths of 2-4 mm) in monthly Multinet deployments from October
to September. August 2007 was inserted between July and September 2008 to provide a
complete composite of the annual cycle. Number of collections shown above bars. The solid
horizontal bar above month labels indicates sampling in the Amundsen Gulf.
3.5.6 Eukrohnia hamata length cohorts and life cycle
Four cohorts were distinguished in all months except August and September 2008, when
there were three (Figure 3.6). The cohort of largest/oldest chaetognaths was labelled E1
(Eukrohnia 1), the intermediate-sized cohorts E2 and E3, and the cohort of autumn (October)
newborns E4. The E1 cohort of large chaetognaths increased little in length from October to
March and disappeared from the collections in April. The length-frequency distributions of
intermediate cohorts E2 and E3 shifted to larger length quasi-monotonically throughout the
annual cycle from October to September. Cohort E2 disappeared from the collections in
August. Initially, the length frequency distribution of cohort E4 progressed slowly to longer
lengths or even regressed as some limited numbers of newborns were added to the cohort
56
starting in December. A new cohort E5 hatched in April (Figure 3.6). Cohort E5 hardly
increased in average length from April to July, as newly hatched chaetognaths were
constantly added to it, but the width of the adjusted Gaussian distribution increased (declining
kurtosis).
Figure 3.6 Monthly length frequency distributions of Eukrohnia hamata. Frequencies of
newborns highlighted in orange. Visually identified length cohorts shown as normal
distributions (in red) with red dots indicating the mean length. Each of the five cohorts is
57
labelled with a capital E and a number from oldest (1) to youngest (5). Blue line is the total
distribution obtained by summing the modelled distributions. Chi-square values for the
goodness-of-fit of the total distribution to the data are given. Sampling regions are
abbreviated in each panel: PC, Parry Channel; AG, Amundsen Gulf; BB, Baffin Bay. k is the
number of collections and n the number of length measurements included (see ‘Method’).
A similar pattern of annual growth was observed for cohorts E1 to E5 of Eukrohnia hamata
(Figure 3.7). After a period of latency of 3-4 months, the mean length of cohorts E4 and E5
of newly hatched E. hamata started to increase (Figure 3.7a). Apart from this initial latency
in younger animals, cohorts E2-E4 increased more or less regularly in mean length from
March to June. The mean length of all cohorts declined from January to February and this
decline persisted until March in cohorts E3 and E4 (Figure 3.7a).
The average length of cohort E4 and E5 in September corresponded to the average length of
cohort E2 and E3 in October respectively (Figure 3.7a), strongly suggesting the co-existence
of an autumn brood (October) and a spring brood (April) of Eukrohnia hamata. Connecting
the corresponding cohorts created a composite of the growth trajectory of the assumed
autumn and spring broods (Figure 3.7b). In all months, the standard deviations around
average length of the presumed autumn and spring broods were distinct. The E1 cohort of
large chaetognaths likely represented the final months of life of the spring brood (Figure
3.7b). The growth trajectory of the autumn brood terminated after 22 months with the
disappearance of cohort E2 from the collections. The growth trajectory of the spring brood
indicated a slightly longer life cycle of two years (24 months). Mean length at a given age
did not differ significantly (t-test, t = 43 df = -0.36, P = 0.72) between the autumn and spring
broods (Figure 3.7c). For the autumn brood, growth was significantly faster in the second
year of life than in the first (ANCOVA, P ˂ 0.01). In the spring brood, growth rates were not
significantly different between years one and two (ANCOVA, P ˃ 0.05).
58
Figure 3.7 a) Monthly mean length (± 1 SD) of the five cohorts of Eukrohnia hamata starting
from a major birth month; b) Composite growth trajectories of the autumn brood (born in
October) and spring brood (born in April) assuming a 2-y lifespan; c) Growth-age curves of
the autumn and spring broods. Circles show mean values of each characteristic (± 1 SD
shown as ribbons).
The autumn and spring broods of Eukrohnia hamata matured in different seasons (Table 3.1)
but at similar body lengths (Figure 3.8). In the autumn brood, all variables peaked in the
second year of life (16 to 23 months of age) from the winter (January-March) to July (Table
59
3.1). Maturity was somewhat less protracted in the spring brood, with ovary length, width of
seminal vesicles and diameter of the protruding seminal receptacles first peaking in August
of the second year of life at 17 months of age (Table 3.1). Maturity indices and oil vacuole
area peaked at different times from November (age 20 months) to March (age 24 months). In
both broods, oocyte number, ovary length and oil vacuole area started to increase by the end
of the first year of life (Figure 3.8a, Figure 3.8b and Figure 3.8c). Some chaetognaths
presented dispersed sperm in the tail during their first year, but sperm frequency started to
increase systematically around the 21th month of life (Figure 3.8d). Seminal vesicle width,
and sperm receptacle diameter began to develop by the 21th month of life as well (Figure 3.8e
and Figure 3.8f).
Table 3.1 Timing of peak development of maturity features in autumn and spring broods of
Eukrohnia hamata and summer brood of Parasagitta elegans, and of the oil vacuole in E.
hamata. Ages in months at peak development are given in parentheses. Monthly collections
consisted of up to 397 and 434 E. hamata individuals from its autumn and spring broods
respectively, and 177 P. elegans.
Characteristic Month(s) of peak maturity (age in months)
E. hamata
autumn brood
E. hamata
spring brood
P. elegans
summer brood
Number of oocytes Jan-Jul (16-23) Mar (24) Feb (20)
Length of ovaries Mar-Jul (18-23) Aug (17), Jan (22) Jan-Aug (19-26)
Area of oil vacuole Mar-Jul (18-23) Dec-Jan (21-22) -
Fraction of inds. with dispersed sperm Mar-Jul (18-23) Nov (20) Feb-Mar (20-21), Aug (26)
Width of seminal vesicles Feb-Jul (17-23) Aug (17), Feb (23) Aug (14), Aug (26)
Diameter of protruding seminal receptacles Mar-Jul (18-23) Aug (17), Feb (23) Jan (19)
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Figure 3.8 Development of sexual features (a, oocyte number; b, ovary length; d, sperm load;
e, seminal vesicle width; f, seminal receptacle diameter) and oil vacuole area (c) with length
for the autumn and spring broods of Eukrohnia hamata. Circles show mean values of each
characteristic (± 1 SD shown as ribbons). Vertical line indicates average length (15.4 mm)
at one year of age. Maturity results for each brood were obtained from the analyses of up to
283 individuals from each 1 mm length class.
61
A vacuole was observed in 99 % of Eukrohnia hamata (n = 2089), the exception being in
newborns 2-3 mm long from the spring brood. Overall, oil was observed in the vacuole or
the digestive tract of 72 % of the E. hamata examined. The fraction of the population with
oil in the vacuole or the body cavity peaked in February (85 %), declined slowly from
February to April, then faster to a minimum in June (54 %) before peaking again in
September (Figure 3.9). Low percentages were observed in October (72 %) and December
(51 %).
Figure 3.9 Mean frequency (± 1 SD) of Eukrohnia hamata with oil in vacuole and/or digestive
tract by months. Number of water column collections shown inside bar (33 – 446 individuals
per haul).
In the Amundsen Gulf, individuals that rose into the PML during summer were mostly
second-year members of the autumn brood and first-year members of the spring-brood
(Figure 3.10).
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Figure 3.10 Abundances (ind. m-3) of Eukrohnia hamata age classes in discrete depth layers
of the Amundsen Gulf, characterized by their mid-points (black squares). Top panels: autumn
brood individuals. Bottom panels: spring brood individuals. Seabed shown in brown,
unsampled sections of the water column in gray. See ‘Method’ for further details.
3.5.7 Parasagitta elegans length cohorts and life cycle
Two cohorts were distinguished in all months except August 2007 and July 2008, when there
were three (Figure 3.11). The cohort of largest/oldest chaetognaths was labelled P1
(Parasagitta 1), the intermediate-sized cohort P2, and the cohort of summer (July) newborns
P3. Cohort P1 (monthly mean lengths >32 mm) disappeared from the collections by
September. The length-distribution of P2 (monthly mean lengths = 21-33 mm) shifted to
larger sizes from July to September and then remained constant until April. That of P3
63
(monthly mean lengths = 5-19 mm) increased from July to November, remained constant or
shifted to smaller sizes from December to April, and then increased again starting in May
(Figure 3.11). A decrease in the length of cohort P3 in December may not be realistic, because
P. elegans reproduced in December (Figure 3.5). However, any winter cohort produced was
not detected in the size-frequency distributions from subsequent months (Figure 3.11).
Figure 3.11 Monthly length frequency distributions of Parasagitta elegans. Frequencies of
newborns highlighted in orange. Visually identified length cohorts shown as normal
distributions (in red) with red dots indicating the mean length. Each of the three cohorts is
labelled with a capital P and a number from oldest (1) to youngest (3). Blue line is the total
distribution obtained by summing the modelled distributions. Chi-square values for the
64
goodness-of-fit of the total distribution to the data are given. Sampling regions are
abbreviated in each panel: NF, Nachvak Fjord; PC, Parry Channel; AG, Amundsen Gulf;
BB, Baffin Bay. k is the number of collections and n the number of length measurements
included (see ‘Method’).
The growth trajectories of the three cohorts over the annual cycle indicated relatively fast
growth from April to September/October followed by stagnation over the winter months and
even a slight regression in length from January to April (Figure 3.12a). Assembling the
growth trajectories of the individual cohorts of Parasagitta elegans (Figure 3.12a) revealed
a single summer brood, which terminated at 2.2 years with the disappearance of cohort P1
from the collections (Figure 3.12b).
Figure 3.12 a) Monthly mean length (± 1 SD) of the three cohorts of Parasagitta elegans
starting from a major birth month; b) Composite growth trajectory of the single brood.
65
Figure 3.13 Development of sexual features (a, oocyte number; b, ovary length; c, sperm
load; d, seminal vesicle width; e, seminal receptacle diameter) with length in Parasagitta
elegans. Circles show mean values of each characteristic (± 1 SD shown as ribbons). Vertical
line indicates average length (20.7 mm) at one year of age. Maturity results were obtained
from the analyses of up to 63 individuals from each 1 mm length class.
In Parasagitta elegans, oocyte number, ovary length, the occurrence of dispersed sperm, and
seminal receptacle diameter first peaked in January or February at ages 19 or 20 months
(Table 3.1). Occurrence of sperm peaked again in August (26 months). The width of seminal
66
vesicles reached a maximum in August early in the second year of life (14 months) and again
in August at 26 months of age (Table 3.1). As P. elegans increased in length, the presence of
oocytes and perceptible ovaries were the first sign of maturation, both indices starting to
increase at 7 mm (Figure 3.13a and Figure 3.13b). Dispersed sperm was first detected around
8 mm and was present in nearly 100 % of individuals >35 mm (Figure 3.13c). Seminal
vesicles and receptacles started to develop around 17 mm in length (Figure 3.13d and Figure
3.13e).
In the Amundsen Gulf, similar SVM behaviour was detected in first- and second-year
individuals. Based on weighted mean depths, the typically resided in the PH from December
to March, ascended in February, were distributed between the PML and the PH from March
to November, and descended in December (Figure 3.14).
Figure 3.14 Abundances (ind. m-3) of Parasagitta elegans age classes in discrete depth layers
of the Amundsen Gulf, characterized by their mid-points (black squares). Seabed shown in
brown, unsampled sections of the water column in gray. See ‘Method’ for further details.
67
3.6 Discussion
3.6.1 Chaetognath cohort interpretation and lifespans
Terazaki & Miller (1986) reported three separate broods of Eukrohnia hamata (spring,
summer and autumn) in the north Pacific with lifespans of 8-10 months. Two-year lifespans
were suggested from the existence of two distinct size cohorts in summer in northern Norway
(Sands 1980), and Baffin Bay (Sameoto 1987). In the present study, E. hamata autumn and
spring broods (staggered by 6 months) also had lifespans of 2 years.
Parasagitta elegans lifespans in Arctic waters ranged from one year in a land-locked fjord
(McLaren 1961), to three years in the Barents Sea (Falkenhaug 1993) and Svalbard (Grigor
et al. 2014). Two-year lifespans were suggested in Disko Bay (Dunbar 1940) and Lancaster
Sound (Welch et al. 1996). In this study, a single annual summer-autumn brood had two-year
life cycles in the Amundsen Gulf, Parry Channel and Baffin Bay. In the Amundsen Gulf, a
possible fourth cohort that contained offspring in late December may have quickly perished
in the lower part of the Pacific Halocline. McLaren (1969) found that first-feeding P. elegans
preyed upon Pseudocalanus nauplii. Darnis & Fortier (2014) reported that Pseudocalanus
spp. CI resided relatively deeper in the PH/AL in December compared to January.
Admittedly, cohort interpretation for P. elegans could also have been hampered by relatively
low sample sizes. In Nachvak Fjord (August 2007), the capture of several individuals up to
45 mm long could indicate a slightly longer lifespan there, which could complicate using
these data to fill in missing data from the Amundsen Gulf time series. Differences could be
due to lower growth rates, genetic differences or different feeding strategies between
populations (Pearre 1991, Øresland 1995). The relatively shallow waters of Nachvak Fjord
also contained low numbers of Eukrohnia hamata, which could reduce competition for
resources.
3.6.2 Resource partitioning in the sympatric Eukrohnia hamata and Parasagitta elegans
In arctic seas where many planktonic species depend on a single brief annual bout of primary
production in summer, morphologically similar species can co-occur thanks to subtle
differences in the ecological niches occupied. For instance, in the Beaufort Sea the
morphologically identical larvae and juveniles of polar cod (Boreogadus saida) and ice cod
68
(Arctogadus glacialis) share the same spatio-temporal distribution, hatching season and
growth rate, but a slightly larger size at hatch results in A. glacialis being longer and feeding
on different prey at a given date than B. saida (Bouchard et al. 2016). As well, the herbivorous
calanoid copepod Calanus glacialis is morphologically almost identical to its sympatric
congener C. hyperboreus except for a smaller size starting at the copepodite IV
developmental stage. Within their sympatric distribution, C. glacialis is preferentially
distributed over the shelf while C. hyperboreus concentrates over the slope and deeper basin
(Darnis et al. 2008 and references therein). The two species also differ in their vertical
distribution and ontogenetic migration (Darnis & Fortier 2014).
Our results support the notion that the morphologically similar and sympatric chaetognaths
Eukrohnia hamata and Parasagitta elegans also partition resources in arctic seas. First,
although the two species generally overlapped in time and space, observations confirm the
more pelagic distribution of E. hamata relative to the neritic P. elegans (Figure 3.3) as
reported in previous studies (Hopcroft et al. 2005, Kosobokova & Hopcroft 2009). Darnis et
al. (2008) identified three zooplankton assemblages in southeastern Beaufort Sea: the Shelf
(43-182 m depth range), Polynya (250-537 m) and Slope (435-1080 m) assemblages. The
pelagic E. hamata thus associated with the Polynya assemblage dominated by Calanus
hyperboreus and the Slope assemblage where omnivores and carnivores are abundant (Darnis
et al. 2008). The neritic P. elegans preferentially associated with the Shelf assemblage, which
is strongly dominated by the neritic copepods Pseudocalanus spp. (Darnis et al. 2008).
Interestingly, McLaren (1969) found that first-feeding P. elegans preyed upon
Pseudocalanus nauplii.
Second, the two species produced offspring in mostly opposite seasons, Eukrohnia hamata
mainly from February to July with a second brood in the autumn (October, December); and
Parasagitta elegans from July to February (Figure 3.5). Consistent with our observations, E.
hamata breeds mostly in spring and summer in the waters off west Greenland and northern
Norway, with reports of continuous low reproduction rates during autumn and winter in west
Greenland and Gerlache Strait, Antarctica (Kramp 1939, Sands 1980, Øresland 1995).
Eukrohnia young are retained in the folded lateral fins of the adults and released at meso-
69
bathy-pelagic depths (Alvarino 1968, Kruse 2009, Terazaki et al. 2013). Emergence at meso-
pelagic levels in the Amundsen Gulf suggests that they may feed on sinking particles,
protozoans, and copepod nauplii present at depth (Makabe et al. 2016), and gut content
observations in 2007 and 2008 in the same region suggest that E. hamata ingested substantial
amounts of large, amorphous macroaggregates (marine snow) throughout the year, while P.
elegans did not feed in this way (unpublished results).
Summer-autumn reproduction in Parasagitta elegans also agrees with previous observations
in Arctic waters (e.g. Kramp 1939, Dunbar 1940, Grainger 1959, McLaren 1961, Sameoto
1971, Grigor et al. 2014). A similar breeding season from July to February in the Canadian
sub-Arctic led Dunbar (1962) to propose that the breeding season of P. elegans is determined
by temperature rather than food availability. However, the epi-pelagic hatching of the
buoyant eggs of P. elegans (Hagen 1985) matches the emergence of the nauplii and CI of the
copepods Pseudocalanus spp. and Oithona similis in the surface layer from July to January
(Darnis & Fortier 2014), potentially ensuring suitably-sized prey (Saito & Kiørboe 2001) to
newborns for the length of the hatching period. At body lengths ˂ 15 mm, first-year P.
elegans participated in the autumn/winter migrations from the PML to the PH (Figure 3.14),
possibly in pursuit of several species of seasonally migrating copepods (Darnis & Fortier
2014).
We suggest that the generally asynchronous reproduction and depth distributions of
Eukrohnia hamata and Parasagitta elegans may reduce potential competition for food during
the early life of arctic chaetognaths.
3.6.3 The potential role of lipid reserves: contrasting growth in the two species
In Eukrohnia hamata, a large fraction (72 %) of total lipids are in the form of the long-term
energy stores steryl esters and wax (Connelly et al. 2012). The lipids contained in the oil
vacuole could have roles in growth, reproduction and/or buoyancy (e.g. Kruse et al. 2010,
Pond 2012, Grigor et al. 2015), although Øresland (1990) doubted a storage role from their
small size. By comparison, lipids in Parasagitta elegans contain low amounts of wax and
70
steryl esters (˂1-8 % of total lipids), and short-term lipid stores such as triacylglycerol are
present only in low to moderate amounts (Falk-Petersen et al. 1987, Lee et al. 2006, Connelly
et al. 2012, Connelly et al. 2016). Lipids gained from copepod prey by P. elegans during
spring-summer feeding may be rapidly utilized for reproduction (Choe et al. 2003).
Some studies have reported reduced growth in winter in arctic and subarctic chaetognaths
(Dunbar 1962, Grigor et al. 2014), and others have not (Welch et al. 1996). Slow winter
growth has been attributed to poor feeding as indicated by gut content analyses (e.g. Øresland
1987, Falkenhaug 1991, Grigor et al. 2015). In the present study, both Eukrohnia hamata and
Parasagitta elegans exhibited slower growth in winter, but the annual growth pattern differed
between the two species. In E. hamata growth was variable but positive over ten months from
March to January (1.55 and 1.82 mm mo-1 on average for the autumn and spring broods
respectively), followed by a 1 to 2-month period of negative growth in late winter (January
to February-March, Figure 3.8b). In P. elegans, fast growth from April to September or
November (2.1 mm mo-1 in year 1 and 3.7 mm mo-1 in year 2 of life), was followed by a long
period of winter stagnation from September-November to April (Figure 3.12b).
The migration of some copepod prey to meso-pelagic depths in the autumn could decrease
prey availability for epi-pelagic chaetognaths in winter (Hagen 1999). The seasonal vertical
migrations in Parasagitta elegans suggest that conscious efforts were made to reduce
starvation (Figure 3.3 and Figure 3.14), but if winter food access was a problem, arrested
growth from late autumn to April in this species may reflect the absence of lipid stores and
oil vacuole. On the other hand, the return of migrating copepods to epi-pelagic depths as
early as February (Darnis & Fortier 2014) could decrease prey availability for Eukrohnia
hamata in spring, and this species carried out relatively limited seasonal migrations (Figure
3.3 and Figure 3.10). Sullivan (1980) suggested that E. hamata requires less prey than P.
elegans. The morphology, growth and vertical distribution of E. hamata suggests that long-
term energy stores enable this species to limit starvation at depths ˃ 200 m to a brief interlude
in late winter and spring. However, contradicting this interpretation, the frequency of E.
hamata presenting oil reserves peaked from January to March during the months of negative
growth in length, and started to decline in April-May (Figure 3.9) coinciding with peak
71
reproduction in April (Figure 3.5). The rebuilding of lipid reserve frequency from June to
September was followed by drops in October and then December (Figure 3.9), which both
coincided with short bouts of reproduction (Figure 3.5). The observed negative correlation
between lipid frequency in the population and offspring production is consistent with the
suggestion by Båmstedt (1978) that part of the lipid content of large specimens of E. hamata
is drawn upon during reproduction, thus lowering the average individual lipid proportion in
the population. We conclude that E. hamata invests its lipid reserves primarily into
reproduction rather than growth, which may contribute to a loss of length in February and
March when prey is likely scarce in deep waters.
3.6.4 Maturation
Dispersed sperm in the tail early in the first year of life was the first sign of maturation in
Eukrohnia hamata, confirming the protandric nature of the species (Terazaki & Miller 1982).
All other maturation traits and the oil vacuole developed in the second year of life. In the
North Pacific, only 3 days separated egg release from the appearance of juveniles (Kotori
1975). Accordingly, the successive maturation episodes in spring and autumn (Table 3.1)
coincided with the occurrence of juvenile E. hamata in net collections. These two maturation
cycles at 6-mo intervals could be interpreted as a sign of iteroparity but actually reflect the
asynchronous maturation of the two broods, which supports the suggestion that E. hamata is
semelparous and dies after a single reproduction effort in the second year of life (Kuhl 1938).
Dunbar (1940) and Grigor et al. (2014) suggested an age-at-maturity of one year for
Parasagitta elegans in the Canadian and European Arctic respectively. Consistent with this,
first-year P. elegans (3-20 mm) could not reproduce as they lacked seminal receptacles and
vesicles. However, oocyte numbers and the frequency of dispersed sperm started to increase
at 9-12 mm corresponding to an age of ca. 6 months. Contrary to Eukrohnia hamata, sexual
maturation occurred from January to August in P. elegans, several months prior to the
emergence of the annual brood from July to December.
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3.6.5 Capital versus income breeding in a warming Arctic
Capital breeding based on wax esters accumulated in summer to fuel reproduction in winter
so as to match the emergence of offspring with the spring-summer maximum in biological
production has been documented in several arctic zooplankton taxa (e.g. Kattner et al. 2007
for a review). Arctic cod (Boreogadus saida), a pivotal forage fish in the arctic pelagic food
web, also spawn in winter with the buoyant eggs hatching in the surface layer before the
onset of the spring-summer primary production (e.g. Bouchard & Fortier 2011). In the
present study, Eukrohnia hamata relied on wax ester reserves to fuel reproduction. But
contrary to other arctic capital breeders such as Calanus hyperboreus and B. saida that
produce a single spring brood, E. hamata produced distinct broods in the autumn and the
spring. Much of the reproduction occurred in deep waters (Figure 3.10). The comparison of
growth trajectories and maturity at length shows a similar developmental rate in the two
broods, which suggests that E. hamata is impervious to differences in temperature regime or
food availability between the two seasons. The distribution of E. hamata in the meso-pelagic
(Atlantic) layer where temperature is constant and where copepod prey resides for most of
the year (Darnis & Fortier 2014) may explain the parallel existence of two sub-populations
that hatch, develop, and reproduce separated by a 6-month time-lag.
The alternative strategy to capital breeding is income breeding in which reproduction is
fueled by immediate food availability in spring-summer with the production of offspring
coinciding with peak production in summer. By contrast to Eukrohnia hamata, the epi-
pelagic Parasagitta elegans, which accumulates few lipid reserves, produced a single brood
in summer, typical of an income breeder. This strategy, which increases in frequency towards
lower latitudes (e.g. Kattner et al. 2007), is also used for instance by the Pacific sand lance
(Ammodytes hexapterus) a recent subarctic invader of the Beaufort Sea (Falardeau et al.
2014). The end result of the remarkably different reproduction strategies of the two species
is the staggering of three distinct broods of morphologically and ecologically similar
chaetognaths: the E. hamata spring cohort in April, the P. elegans summer cohort in July,
and the E. hamata autumn cohort in October. The sequestration of lipids thanks to the early
development of an oil vacuole may enable young E. hamata at meso-pelagic depths to
overcome potential food shortages in spring and autumn, while the only survival window for
73
the lipid-poor P. elegans would be during peak availability of prey in the surface layer in
summer.
3.7 Conclusions
Based on our observations from August 2007 to September 2008 in the Canadian Arctic, the
processes of growth and reproduction are more seasonally-restricted in Parasagitta elegans
compared to Eukrohnia hamata. Length and maturity data for the two species from other
years would help to confirm if this is a general trend. As the Arctic warms and the ice-free
season lengthens, wind mixing increasingly triggers a second phytoplankton bloom in the
autumn, with potentially major impacts on arctic marine ecosystems (Ardyna et al. 2014). If
the availability of suitable prey at the first-feeding stage is critical to the survival of young
chaetognaths, we hypothesize that this autumn bloom would more directly and quickly
benefit the income-breeding P. elegans as copepod prey in epi-pelagic waters would increase.
74
4. Chapter 4 – Feeding strategies of arctic chaetognaths: are they
really “tigers of the plankton”?
4.1 Résumé
Les chaetognathes, aussi connus sous le nom de « tigres du plancton » jouent un rôle
important dans les communautés mésozooplanctoniques, en termes d'abondance et de
biomasse. Bien que traditionnellement considérés comme étant strictement carnivores, des
études récentes suggèrent l’usage de stratégies non -carnivores au sein du phylum. Les
stratégies d'alimentation des chaetognathes de l’Arctique sont particulièrement intéressants
comptes tenus de la forte saisonnalité dans les abondances et les distributions de proies
connues (copépodes). Le présent chapitre traiter des stratégies d'alimentation saisonnières de
deux principales espèces de l’Arctique : Eukrohnia hamata de la zone mésopélagique, ainsi
que Parasagitta elegans de la zone épipélagique. Le contenu du tube digestif de spécimens
récoltés au printemps, en été et en hiver au sud-est de la mer de Beaufort suggère de faibles
taux de prédation chez toutes les espèces (0-0,27 proie ind. d-1). Toutefois, les taux de
prédation de E. hamata et de P. elegans étaient plus élevés au printemps-été par rapport à
l'automne-hiver. E. hamata mange des macroagrégats ne contenant pas de proies (˃500 µm),
probablement de la neige marine, tout au long de l'année. Ce mode d'alimentation
précédemment non répertorié a été confirmé pour E. hamata par des observations
d'alimentation in-vitro dans la mer de Chukchi à l'automne, mais n’a pas été observé chez P.
elegans. Des quantités étonnamment élevées d’acides gras marqueurs de diatomées en
automne dans les spécimens de E. hamata suggèrent fortement que les diatomées ont été
consommées directement, tandis que des ratios inférieurs à 18:1 (n-9)/(n-7), et valeurs
inférieures de δ15N et δ13C comparativement au P. elegans ont tous suggéré son régime
alimentaire plus omnivore. Nous suggérons que par la consommation de neige marine, les
pelotes fécales du E. hamata pourraient contribuer davantage à la séquestration du carbone
qu'on ne le pensait auparavant.
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4.2 Abstract
Chaetognaths, also known as the “tigers of the plankton” are important components of
mesozooplankton communities, in terms of abundance and biomass. Although traditionally
considered to be strict carnivores, recent studies suggest non-carnivorous strategies occur
within the phylum. The feeding strategies of arctic chaetognaths are particularly interesting
given the strong seasonality in the abundance of known food items, chiefly copepods. This
chapter addresses the seasonal feeding strategies of two major Arctic species; the meso-
pelagic Eukrohnia hamata and the epi-pelagic Parasagitta elegans. Gut contents of
specimens collected in spring, summer and winter in the south-eastern Beaufort Sea
suggested low predation rates in the two species (0 – 0.27 prey ind. d-1), but predation rates
in E. hamata and P. elegans were higher in spring-summer compared to autumn-winter. E.
hamata ate non-prey macroaggregates (˃ 500 µm, probably marine snow) throughout the
year. This previously unreported feeding mode was confirmed for E. hamata by in-vitro
feeding observations in the Chukchi Sea in the autumn. High levels of diatom fatty acid
markers in E. hamata sampled in autumn, strongly suggested that diatoms were consumed
directly, whilst lower 18:1 (n-9)/(n-7) ratios, δ15N and δ13C, compared to P. elegans
confirmed its more omnivorous diet. We suggest that by containing algal-rich contents, the
fecal pellets of E. hamata could contribute more to carbon sequestration than those of strict
carnivores.
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4.3 Introduction
Chaetognaths, the so-called “tigers of the plankton” (Suthers et al. 2009), are semi-gelatinous
zooplankters considered to be primary carnivores in the marine food web (Reeve 1970).
Reported prey includes fish larvae, copepods and other chaetognaths (e.g. Alvarino 1965,
Sullivan 1980, Brodeur & Terazaki 1999). In some locations, chaetognath populations could
control copepod standing stocks (e.g. Sameoto 1972, Williams & Collins 1985). The fecal
pellets of chaetognaths are said to be large and carbon-rich, and, considering the high
abundances of chaetognaths in the ocean, these pellets could be important food for
zooplankton in the water column or in the flux of carbon to the benthos (Dilling & Alldredge
1993, Giesecke et al. 2010).
The presence of algal cells (Alvarino 1965, Alvarez-Cadena 1993, Marazzo et al. 1997, Kruse
et al. 2010), green detritus and phaeophytin (Philp 2007, Grigor et al. 2015) in chaetognath
guts hints at non-carnivorous feeding. However, such vegetal remains are generally
interpreted as originating in the guts of digested animal prey. Based on various aspects of
chaetognath nutrition, notably in-vitro ingestion of seawater and active digestive processes
in gut cells in the absence of visible gut content, Casanova et al. (2012) suggested that
dissolved and fine particulate organic matter were major food sources for chaetognaths.
Several studies on the polar chaetognaths Eukrohnia hamata, Parasagitta elegans and
Pseudosagitta maxima have reported on ˃90 % of individuals lacking visible gut prey (e.g.
Sameoto 1987, Øresland 1995, Froneman & Pakhomov 1998, Brodeur & Terazaki 1999,
Bollen 2011, Giesecke & Gonzalez 2012, Grigor et al. 2015). For many polar zooplankters,
the ability to switch between carnivorous and non-carnivorous feeding (e.g. detritivory or
filtering) is an important adaptation to seasonal cycles in food availability (e.g. Auel et al.
2002, Hirche et al. 2003, Norkko et al. 2007, Søreide et al. 2008). Could the polar
chaetognaths utilize similar seasonal adaptations, even though they do not obviously exhibit
adaptations to filter phytoplankton?
Gut content analysis provides information on recent feeding but the resulting interpretation
of trophic relationships can be flawed if sampling or handling protocols damage the gut,
77
induce regurgitation or defecation, or if feeding is biased by the concentration of predator
and prey in the sampling gear (Baier & Purcell 1997 and references therein). Additional and
likely less-biased longer-term information on trophic dynamics can be gained from the
analysis of fatty acids and stable isotopes. Some fatty acids specific to a given prey typically
persist in predators for weeks to months with little or no breakdown or transformation, and
can be useful trophic markers (Dalsgaard et al. 2003, Arim & Naya 2003, Grigor et al. 2015).
Nitrogen isotopes are routinely used to infer trophic levels due to a step-wise increase in
15N/14N ratio (δ15N) with every ascending trophic level (Minagawa & Wada 1984, Michener
& Schell 1994). Carbon isotopes can be used to infer the source of primary productivity,
given close similarities in the 13C/12C ratios (δ13C) of an animal and its food (Hobson &
Welch 1992).
This study aims at understanding how food resources are utilized year-round by co-existing
Eukrohnia hamata and Parasagitta elegans in the Canadian and Alaskan Arctic. In the south-
eastern Beaufort Sea, gut contents are examined to reveal diets from November 2007 to
August 2008. In addition, we compare the fatty acid and stable isotope signatures of E.
hamata and P. elegans in the north-eastern Chukchi Sea (Alaskan Arctic) and Baffin Bay
(Canadian Arctic), based on collections made in autumn 2014.
4.4 Method
4.4.1 Study areas
Sampling surveys were carried out on-board CCGS Amundsen between from 2007 to autumn
2008 in the Beaufort Sea, and in autumn 2014 in the Chukchi Sea and Baffin Bay (Figure
4.1). 127 stations were sampled at weekly (or higher) resolution, in the Amundsen Gulf (69-
72°N, 120-131°W) between November 2007 and August 2008 (Figure 4.1a and Appendix E-
1). 6 stations were sampled in the north-eastern Chukchi Sea (71-76°N, 144-168°W) in
September 2014 (Figure 4.1b and Appendix E-2). 3 stations were sampled in the Baffin Bay
region (67-72°N, 61-73°W) in early October 2014; single stations in Scott Inlet Fjord, in
Gibbs Fjord and southern Baffin Bay (Figure 4.1c and Appendix E-2).
78
The Amundsen Gulf is a bridge between the south-eastern part of the Beaufort Sea to the
Canadian archipelago. This 400-km long gulf has a width of 170 km and a maximum depth
~630 m, and sea-ice cover between October and early June (Barber & Hanesiak 2004,
Geoffroy et al. 2011). Three water masses prevail in the region; the nutrient-poor Pacific
Mixed Layer (PML, 0-50 m depth; salinity ˂ 31.6 psu), the Pacific Halocline (PH, 50–200 m
depth; 32.4-33.1 psu), and lastly the Atlantic Layer (AL, ˃200 m depth; ˃34 psu) (Carmack
& Macdonald 2002). The Chukchi Sea (Alaska’s northernmost shelf sea) is a relatively
shallow environment characterised by hotspots of high primary productivity stimulated by
the northward invasion of nutrient-rich Pacific water (Hopcroft et al. 2004, Weingartner et
al. 2005). Sinking phytoplankton may only be partly exploited by zooplankton, supporting
benthic animals (Hopcroft et al. 2004 and references therein). On the eastern side of the
Canadian archipelago lies the semi-enclosed basin of Baffin Bay, with numerous fjords along
the east coast of Baffin Island. A unique hydrocarbon seep and chemolithic community
occurs in Scott Inlet Fjord (DFO 2015), but the plankton communities in these fjords are
poorly studied.
79
Figure 4.1 Bathymetric maps of the Arctic Ocean, showing the positions of sampling stations
(black circles) in (a) Amundsen Gulf, (b) north-eastern Chukchi Sea and (c) Baffin Bay (SIF
= Scott Inlet Fjord; GF = Gibbs Fjord; SBB = southern Baffin Bay). Details of sampling
stations are shown in Appendices E-1 and E-2.
4.4.2 Sampling in the Amundsen Gulf
The biomass of chlorophyll a (˃0.7 µm) was used as an indicator of algae blooming. At 54
stations (Appendix E-1), seawater samples were collected from 7-12 depths at using the CTD
rosette equipped with twenty-four 12 1 Niskin-type bottles (OceanTest Equipment). Methods
for the determination of chlorophyll a (chl a) from seawater subsamples are outlined in
Chapter 3 of this thesis.
80
At 10 stations, zooplankton were sampled using a large square-conical net with a 1 m2
opening area, 200 µm mesh and a 2-L rigid cod-end. At 72 stations, zooplankton were
sampled using a Hydrobios® Multinet, comprising 9 nets with 0.25 m2 apertures, 200 µm
meshes and 2-L rigid cod-ends. Individual nets open and close sequentially to sample
zooplankton from pre-selected depth intervals (Appendix E-1). Samplers were deployed to a
depth of 10 m above the seabed, cod-end(s) first (non-filtering), and then hauled back to the
surface at a constant velocity of 0.5 m s-1. For Multinet sampling, the upper 60 m and lower
60 m of the sampled water column were divided into three 20-m depth layers, and the
remainder was divided into three equal layers. Samples were fixed in 4 % buffered
formaldehyde-seawater solution.
4.4.3 Sampling in the Chukchi Sea and Baffin Bay
Square-conical nets (1 m2 opening areas, 2-L rigid cod-ends) were deployed to collect
chaetognaths for fatty acid and stable isotope analyses (Appendix E-2). At 7 stations, epi-
pelagic chaetognaths were sampled by oblique trawls of 500/750 µm-mesh nets at 90 m. The
ship speed was approximately 1 m s-1, and the cable angle was ~60º. At 6 stations, meso-
pelagic chaetognaths were sampled in vertical tows of 200/500 µm-mesh nets (see Amundsen
Gulf sampling protocol). A maximum of 30 Eukrohnia hamata or Parasagitta elegans
individuals were randomly removed from each sample, and kept frozen at -80 ºC for further
processing.
4.4.4 Abundance of zooplankton
A total of 70 Multinet collections in the Amundsen Gulf (typically 9 samples per haul), 3 to
11 per month from November 2007 to July 2008, were analysed to estimate the abundance
of main zooplankton species. Formalin-preserved samples were sieved into two size
fractions; 0.2-1 mm and >1 mm. From each fraction, known subsamples were taken until 300
copepods were removed, and all animals in the subsamples were counted and identified to
the lowest possible taxonomic level, typically species or stage. Abundances of species
present in the water column were calculated (where possible), summing abundances of
appropriate taxa in the two size fractions.
81
4.4.5 Gut contents
A total of 21 net collections in the Amundsen Gulf were used to analyze chaetognath gut
contents. 4742 chaetognaths were included in gut content analyses (4078 Eukrohnia hamata
with body lengths between 2 and 39 mm and 654 Parasagitta elegans with body lengths
between 2 and 42 mm). 10 Pseudosagitta maxima also present in the samples (15-65 mm)
were not analysed further. Each individual chaetognath was stained with a solution of Borax
Carmine to highlight potential prey tissues (Sameoto 1987). Gut contents were observed
under the stereomicroscope (maximum magnification = 11.5×). Prey items were identified to
the lowest taxonomic level possible, although accurate identifications of prey species were
often difficult due to their augmented state of digestion. Prey items in the mouths of
chaetognaths were ignored, as they are a likely reflection of the concentration of predator and
prey in the sampling gear, and therefore biased. The average number of prey per chaetognath
gut (npc) was estimated for each collection for the two species. Daily predation rates (DPR;
number of prey items consumed ind.-1 d-1) were calculated after Bajkov (1935) [Eq. (4.1)].
DPR =npc x 24
tdig (4.1)
Where tdig = digestion time in hours at a suitable temperature (here ~0 ºC). For Eukrohnia
hamata, we used 11 h, determined for this species in the Southern Ocean (Giesecke &
Gonzalez 2012). For Parasagitta elegans, we used 10.2 h, determined for this species in
Massachusetts (Feigenbaum 1982).
To detect the presence of different food items, such as algae, the color of lipid droplets and
detritus in the guts of 2118 Eukrohnia hamata and 201 Parasagitta elegans was also
described. A limited subset of individuals (3 E. hamata and 3 P. elegans from single
collections in November, February, May and July) were re-analysed using Scanning Electron
Microscopy (SEM), to detect other evidence of recent feeding only visible at these high
magnifications.
82
4.4.6 Fatty acids
To determine the fatty acid profiles of Eukrohnia hamata in autumn (2014), we analysed
samples of 5 pooled individuals from 1 station in the Chukchi Sea and 3 in the Baffin Bay
region. We also analysed samples of 5 pooled Parasagitta elegans individuals from 3 stations
in the Chukchi Sea and 2 in the Baffin Bay region (Appendix E-2). For E. hamata, three
samples were analysed per station. For P. elegans, 1-3 samples were analysed per station.
Samples were freeze-dried and an internal standard (5β cholanic acid, 1 µg) was added. Total
lipids were extracted using a mixture of dichloromethane and methanol (2/1; 5 ml; 3×15
minute ultrasonications). The total lipid fraction was dried with N2 and MeOH-H2O KOH
(80/20; 5 %; 3 ml) and was then added to the extract before heating at 90 ºC for 2 hours. The
fraction containing the non-saponifiable lipids was obtained by liquid-liquid extraction, dried
over Na2SO4, and derivatised using BSTFA (70 ºC, 30 minutes) prior to gas
chromatography–mass spectrometry (GC-MS) analysis. The saponification mixture was
acidified with HCl (10N; 2 ml) and the fatty acids extracted with hexane. Fatty acids were
methylated (BF3MeOH; 20/80; 80 ºC; 30 minutes) prior to identification and quantification
of 20 fatty acid methyl esters previously reported in Grigor et al. (2015), plus 20:1 (n-7) by
GC-MS. Results are given as relative percentages of the various fatty acids identified in
specimens at each station. A higher 18:1 (n-9)/(n-7) ratio was used to indicate a greater
tendency towards carnivory (Falk-Petersen et al. 1990, Wang et al. 2015). Higher proportions
of the monounsaturated FAs Σ20:1+22:1 MUFA were taken to indicate a greater contribution
of Calanus copepods in the diet (Falk-Petersen et al. 1987, Wang et al. 2015). A higher ratio
of 16:1/16:0 was used to indicate a greater contribution of diatoms compared to flagellates
(Nelson et al. 2001, Wang et al. 2015).
4.4.7 Carbon and nitrogen
To determine the stable isotope signatures of Eukrohnia hamata in autumn (2014), we
analysed individuals from 3 stations each in the Chukchi Sea and Baffin Bay region. We also
analysed Parasagitta elegans samples from 4 stations in the Chukchi Sea and 2 in the Baffin
Bay region (Appendix E-2). These samples each contained up to 5 individuals. For E.
hamata, 3-6 samples were analysed per station. For P. elegans, 1-5 samples were analysed
per station. Tin-wrapped samples were combusted at a localized temperature up to 1800 °C
83
using an ECS 4010 Elemental Analyser/ZeroBlank Autosampler (Costech Analytical
Technologies). Carbon and nitrogen masses were determined to the nearest microgram.
Gases produced (N2 and CO2) after oxidation/reduction and water removal were separated
using an internal GC column. Isotope ratios were measured by on-line continuous-flow
isotope ratio mass spectrometry (IRMS) with a Thermo Electron Delta Advantage
spectrometer operating the continuous-flow mode (Thermo Electron ConFlo III). Five of
each of the standards (USGS40 and USGS41, Qi et al. 2003) were analysed at the beginning
and end of each run. One standard was run for every 12 samples to check for combustion and
correct any instrumental drift; isotope ratio errors were ±0.006 or better.
δ13C values were calculated for samples as changes in sample ratios of 13C/12C from those in
the international standard Vienna Pee Dee Belemnite (13C/12C). δ15N values were calculated
as changes in sample ratios of 15N/14N from those in the standard AIR (15N/14N), as in [Eq.
(4.2)].
δ13C or δ15N = [(𝑅sample/𝑅standard) − 1]×1000 (4.2)
Where R = ratio of 13C/12C or 15N/14N
Trophic levels (TLs) of samples were calculated as changes in δ15N values from that of a
typical food-web baseline (TL = 1 in Eq. 4.3). We used particulate organic matter (POM) as
the baseline, in line with other arctic studies (e.g. Iken et al. 2005, Bergmann et al. 2009, Roy
et al. 2015).
TL = 1 +(δ15Nsample−δ15Nbaseline)
δ15Nenrichment per TL (4.3)
Where 1 = TL of POM. We used a δ15Nbaseline value of 6.8 ‰, previously reported for shallow
water POM (˂50 m) in the North Water Polynya in late spring/summer of 1998 (Hobson et
al. 2002). It was assumed that δ15N values increased by 3.8 ‰ with every ascending trophic
level (Hobson & Welch 1992, Hobson et al. 2002, Connelly et al. 2014).
84
4.5 Results
4.5.1 Amundsen Gulf
4.5.1.1 Phenology of algae blooms
Based on chlorophyll a biomass, a bloom of ice algae was first detected in late March in the
PML (0-60 m), peaked at these depths in late April and early May (chl a biomass ˃ 5 mg m-
3), and succeeded by a surface bloom of phytoplankton (10 mg chl a m-3). In July,
phytoplankton penetrated the PH (60-200 m), and phytoplankton biomass peaked in mid-July
in the PML (˃ 16 mg chl a m-3; Figure 4.2).
Figure 4.2 Vertical distributions of chlorophyll a biomass (mg m-3) in the upper 200 m of the
water column along the ship track from November 2007 to July 2008 in the Amundsen Gulf.
Black dots indicate sampling depths. Details of sampling stations are shown in Appendix E-
1. Chl a data were provided by Michel Gosselin (Université du Québec à Rimouski).
4.5.1.2 Zooplankton community
A total of 119 zoo- and icthyoplankton species and 57 other taxa not identifiable to the species
level were detected in the Amundsen Gulf collections from November 2007 to July 2008.
Numerically, the mesozooplankton was dominated by the usual guild of copepods (Oithona
similis, Triconia borealis, Metridia longa, Calanus glacialis, Microcalanus pygmaeus,
Microcalanus pusillus, Pseudocalanus elongatus, Pseudocalanus minutus and Calanus
hyperboreus), which were present at all stations (Table 4.1). Eukrohnia hamata was also
85
present at all stations in the Amundsen Gulf with abundances ranging from 4 m-2 in late
March to 3318 m-2 in late July. Parasagitta elegans was less abundant than E. hamata at all
stations in Amundsen Gulf (0 m-2 in December to 1927 m-2 in June).
Table 4.1 Composition of the
mesozooplankton (30 most
abundant taxa) sampled in the
Amundsen Gulf from November
2007 to July 2008, based on data
from 70 Multinet hauls. *Taxa
could not be identified to species
level.
Species / taxon n hauls
present
Mean number m-2
(± 1 SD)
Date of peak
abundance
Oithona similis 70 30475±14290 27/01/08
Triconia borealis 70 17583±12191 17/04/08
Metridia longa 70 15402±10758 05/03/08
Calanus glacialis 70 10255±6702 27/01/08
Microcalanus pygmaeus 70 4818±3750 27/01/08
Microcalanus pusillus 67 4603±3260 19/04/08
Pseudocalanus elongatus 70 4085±3241 27/01/08
Pseudocalanus minutus 70 3431±2874 05/12/07
Cyclopina sp.* 51 1968±2308 10/06/08
Calanus hyperboreus 70 1962±1565 19/04/08
Radiolarians* 66 1053±2262 27/05/08
Scolecithricella minor 70 798±752 18/04/08
Triconia parila/notopus 18 787±1745 01/05/08
Frittilaria sp.* 18 648±3756 06/05/08
Limacina helicina 66 608±964 01/07/08
Clione limacina 68 606±563 03/03/08
Spinocalanus longicornis 66 540±758 27/01/08
Pseudocalanus acuspes 59 467±1305 27/01/08
Eukrohnia hamata 70 456±565 23/07/08
Microcalanus sp.* 18 381±2957 25/07/08
Pseudocalanus sp.* 27 307±830 01/07/08
Boroecia maxima 69 295±274 19/04/08
Bivalves* 27 282±938 23/11/07
Aetideopsis rostrata 55 277±443 19/04/08
Oikopleura sp. 43 273±660 01/07/08
Dimophyes arctica 50 273±386 05/03/08
Paraeuchaeta glacialis 70 253±519 28/06/08
Aglantha digitale 68 252±308 27/07/08
Gaetanus tenuispinus 57 212±260 18/04/08
Parasagitta elegans 68 173±339 10/06/08
86
4.5.1.3 Visible prey items and predation rates
Prey organisms were detected in 0.9 % of Eukrohnia hamata and 0.8 % of Parasagitta
elegans in the Amundsen Gulf. Copepods comprised 97 % of total prey items in E. hamata
and all detected prey items in P. elegans. Identifiable prey taxa were Oithona similis, Calanus
spp., a female Pseudocalanus spp. (Figure 4.3), and a chaetognath in one E. hamata
individual. Multiple copepods (2 or 3) were detected in five chaetognaths. Daily predation
rates (DPRs) were in the range 0-0.27 prey ind. d-1 for E. hamata, and 0-0.09 prey ind. d-1 for
P. elegans. In general, predation rates were higher on dates in November and December
compared to dates in spring and summer. Average npc values were generally higher in
chaetognaths from Multinet collections compared to square-conical net collections, but note
that collections from the latter gear were often considerably larger (Figure 4.3).
Figure 4.3 Average number of prey per chaetognath gut (npc) in square-conical (S-C) net
and Multinet collections from November 2007 to August 2008 in the Amundsen Gulf.
Numbers of individuals shown above data points. k is the number of collections. Inset bottom:
photograph of a Parasagitta elegans specimen (12 mm) with a relatively large Pseudocalanus
spp. copepod in the gut (from November 2 2007).
87
4.5.1.4 Lipid droplets and detritus
Lipid droplets occurred in the body cavities of 72 % of 3408 analysed Eukrohnia hamata.
Amounts were substantial though not quantified. The fraction of the E. hamata population
with oil in the body cavity peaked between mid-January and early-May (74-87 %), thereafter
declining quickly to below 50 % in late-May and early-June. Low percentages were observed
in December (51 %). Droplets were typically yellow in color between late November and
early March (72-90 % of droplets), but from then until late July were typically green in color
(58-92 % of droplets). In addition to occurring in the guts of only 4 % of 497 Parasagitta
elegans, lipid droplets were smaller and less abundant in this species. Whilst detritus (mainly
crustaceous debris) was observed in the guts of 12 % of Parasagitta elegans, 38 % of
Eukrohnia hamata contained detritus in their guts, with 79 % of these containing thick green
macroaggregates ˃ 500 µm (see Figure 4.4). The fraction of the E. hamata population
containing detritus in the gut peaked in late May (71 %). Detritus in E. hamata were typically
green in color on all 11 sampling dates (56-100 %). The fractions of the population containing
detritus and green macroaggregates were lower in early May (25 % and 14 % respectively)
and in early June (28 % and 25 %).
Figure 4.4 Photographs of substantial
amounts of green macroaggregates (˃
500 µm) in the guts of Eukrohnia
hamata, but not in the guts of
Parasagitta elegans. Specimens from
the Amundsen Gulf on May 31 2008
(20-40 m depth), 20-30 mm.
88
Green-colored lipid droplets and macroaggregates were observed in both first-year and
second-year Eukrohnia hamata individuals. The fraction of the second-year individuals
containing such material was ≥ 50 % on all 11 sampling dates from November to July. The
occurrence of such gut contents in the first-year animals increased steadily throughout winter
as the animals grew. (Table 4.2).
Table 4.2 Frequency of first- and second-year Eukrohnia hamata individuals with green lipid
droplets or macroaggregates in guts. Separate results are presented for the autumn
(October) and spring (April) broods of E. hamata (see Chapter 3), from approximate month
of hatching (no gut content data were available for October).
Month Autumn brood Month Spring brood
n % with
green guts
n % with
green guts
Age 0-1
Apr 15 73 Nov 82 17
Early May 14 100 Dec 49 35
Late May 12 58 Jan 1 100
Jun 33 61 Feb 33 21
Jul 6 67 Mar 106 13
Nov 135 67 Apr 12 8
Dec 97 65 Early May 46 48
Jan 83 88 Late May 14 50
Feb 20 90 Jun 75 45
Mar 100 79 Jul 78 72
Age 1-2
Apr 3 67 Nov 159 49
Early May 14 71 Dec 86 57
Late May 7 71 Jan 51 80
Jun 29 52 Feb 67 73
Jul 16 94 Mar 74 82
Nov 50 56 Apr 4 0
Dec 33 79 Early May 35 31
Jan 4 75 Late May 27 22
Feb 19 100 Jun 104 31
Mar 26 100 Jul 47 40
89
4.5.1.5 Scanning Electron Microscope observations
Spherical structures resembling bacteria were observed in Eukrohnia hamata guts in samples
from November and May (Figure 4.5). The apparent hooks of a chaetognath, and copepod
mandibles and filaments, were observed in Parasagitta elegans guts in samples from
November and May. Individuals of both species also contained unidentified amalgamated
structures in November, February, May and July.
Figure 4.5 Scanning Electron Microscope photographs of some items in Eukrohnia hamata
guts (left box) and Parasagitta elegans guts (right box), in different months. Examples: hooks
of a chaetognath, and mandibles of copepods (arrow caps). Specimens 20-30 mm.
90
4.5.2 Chukchi Sea and Baffin Bay
4.5.2.1 In-vitro feeding observations
At station CS1 in the Chukchi Sea (Figure 4.1b), in-vitro ingestion of green macroaggregates
was observed for two living Eukrohnia hamata individuals enclosed in a petri dish (Figure
4.6). One Pseudosagitta maxima individual also observed to consumed marine snow in a
petri dish (not shown). Guts of E. hamata in Chukchi Sea samples contained algal cells
including those of the Ceratium spp. (dinoflagellate) and diatoms (inverted microscopy,
Figure 4.6).
Figure 4.6 Photographs of
live Eukrohnia hamata
individuals consuming
green macroaggregates
in-vitro in the Chukchi
Sea. Specimens 20-30 mm.
Bottom right: An inverted
microscope photograph of
phytoplankton such as
Ceratium spp. in one gut.
4.5.2.2 Lipid amounts
Lipid amounts (expressed as a fraction of sample dry weights) did not vary between
Eukrohnia hamata and Parasagitta elegans (Kruskal-Wallis ANOVA, P = 1.00). In each
species, lipid amounts were also similar between stations (E. hamata: One-way ANOVA, P
= 0.12, P. elegans: Kruskal-Wallis ANOVA, P = 0.35).
91
4.5.2.3 Fatty acid profiles: species differences
Of the 21 fatty acid methyl esters quantified, proportions of 13 varied between Eukrohnia
hamata and Parasagitta elegans (Kruskal-Wallis ANOVA, P ˂ 0.05, Table 4.3). Not
accounting for station differences, amounts of Calanus markers (ΣC20:1+C22:1) were
statistically higher in E. hamata samples (≤30.29 %) than P. elegans samples (≤13.40 %)
(Kruskal-Wallis ANOVA, P = 0.00, Table 4.3 and Figure 4.7). Diatom markers 16:1 (n-7)
and 20:5 (n-3) were dominant fatty acids in both species (Table 4.3). Amounts of 20:5 (n-3)
were similar in samples of the two species (11.12 % - 25.82 % in E. hamata, 8.40 - 22.76 %
in P. elegans), but 16:1 (n-7) amounts were higher in E. hamata (23.42 - 48.93 %) compared
to P. elegans (12.88 - 20.44 %). Some P. elegans samples contained high amounts of the
flagellate marker 16:0 (≤25.69 %), and in general, amounts of 16:0 were lower in E. hamata
samples (3.38 - 15.06 %). Corresponding 16:1/16:0 ratios were higher in E. hamata (˃3
versus ˂2 in P. elegans) (Kruskal-Wallis ANOVA, P = 0.00, Figure 4.7). The bacterial
marker 18:1 (n-7) occurred in moderate amounts in both species, but the animal marker 18:1
(n-9) occurred in lower amounts in E. hamata (2.48-5.33 %) compared to P. elegans (7.15 -
11.55 %. Corresponding 18:1 (n-9)/(n-7) ratios were higher in P. elegans (˃1 versus ˂1 in E.
hamata) (Kruskal-Wallis ANOVA, P = 0.00, Figure 4.7).
4.5.2.4 Fatty acid profiles: station and regional differences in Eukrohnia hamata and
Parasagitta elegans
For Eukrohnia hamata, proportions of only four fatty acids; 14:0, 18:2(n-6), 18:4(n-3) and
20:1 (n-9) differed between stations (One-way ANOVA, P ≤ 0.05). 18:1 (n-9)/(n-7) ratios
did not differ between regions (P = 0.43) or stations (P = 0.38). Similarly, 16:1/16:0 ratios
did not differ between regions (P = 0.65) or stations (P = 0.29). For Parasagitta elegans,
proportions of all fatty acids were similar between sampling stations (Kruskal-Wallis
ANOVA, P ˃ 0.05). Kruskal-Wallis ANOVAs also showed that P. elegans in the two regions
had different 18:1 (n-9)/(n-7) ratios (P = 0.02), and different 16:1/16:0 ratios (P = 0.07).
These differences, however, were not detected at the station level (P = 0.15 and P = 0.33),
which may be an artefact of low sample sizes (n = 1) at two stations (Table 4.3b).
92
Table 4.3 Mean sample lipid, fatty acid amounts and fatty acid proportions (± 1 SD) in (a)
Eukrohnia hamata and (b) Parasagitta elegans at different stations (stns) in autumn 2014.
Sampling locations are abbreviated: CS, Chukchi Sea; SIF, Scott Inlet Fjord; GF, Gibbs
Fjord; SBB, southern Baffin Bay. Also: number (n) of samples analysed and chaetognaths
per sample, and chaetognath body lengths in mm. † Significant species differences (P ≤ 0.05).
Fatty acid CS4 SIF GF SBB Overall average
(a) E. hamata
n samples 3 3 3 3 12
n individuals per sample 4-5 5 5 4-5
Body lengths (mm) 10-32 9-32 20-32 10-29
Lipids % DW 41.99±6.57 40.31±6.52 48.68±1.41 37.28±4.08 42.06±6.16
FA mg g-1 ind.-1 24.34±10.39 37.73±18.49 47.60±10.92 20.47±7.30 32.54±15.51
14:0† 1.32±0.63 0.86±0.42 1.19±0.34 2.81±0.66 1.55±0.90
14:1 (n-5)† 0.20±0.06 0.14±0.05 0.22±0.05 0.13±0.06 0.17±0.06
15:0† 0.10±0.02 0.07±0.04 0.09±0.03 0.16±0.06 0.11±0.05
16:0† 5.78±0.95 6.62±4.80 4.96±1.19 11.25±3.30 7.15±3.62
16:1 (n-5)† 0.48±0.07 0.42±0.28 0.70±0.17 0.89±0.37 0.62±0.29
16:1 (n-7)† 26.03±3.40 32.05±6.88 29.53±5.42 36.12±12.66 30.93±7.74
18:0† 0.76±0.22 0.82±0.51 0.50±0.14 1.04±0.22 0.78±0.33
18:1 (n-7) 10.21±5.46 7.22±2.58 10.43±2.93 6.22±0.18 8.52±3.44
18:1 (n-9)† 3.03±0.50 3.62±1.48 3.20±0.57 3.44±0.52 3.32±0.78
18:2 (n-6)† 0.84±0.12 0.54±0.10 0.33±0.28 0.86±0.26 0.64±0.29
18:3 (n-3) 0.33±0.06 0.28±0.16 0.08±0.07 0.22±0.09 0.23±0.13
18:4 (n-3) 1.88±0.33 0.61±0.35 1.01±0.67 1.58±0.39 1.27±0.64
20:1 (n-7) 0.47±0.10 0.72±0.29 0.52±0.17 0.54±0.11 0.56±0.19
20:1 (n-9)† 10.41±2.01 13.51±3.44 14.05±0.59 7.23±0.69 11.30±3.34
20:4 (n-3) 0.10±0.02 0.16±0.12 0.14±0.08 0.10±0.08 0.12±0.08
20:5 (n-3) 18.13±6.80 15.04±3.67 16.41±0.36 15.39±6.79 16.24±4.56
22:1 (n-7) 0.22±0.12 0.21±0.22 0.17±0.13 0.34±0.08 0.24±0.14
22:1 (n-11)† 6.66±2.91 10.35±4.46 9.58±0.60 4.70±1.66 7.82±3.36
22:5 (n-3) 0.53±0.34 0.60±0.54 0.53±0.20 0.35±0.15 0.50±0.31
22:6 (n-3)† 12.20±3.70 5.99±0.64 6.22±2.74 6.32±4.29 7.68±3.83
24:1 (n-9)† 0.31±0.07 0.17±0.06 0.15±0.12 0.30±0.13 0.23±0.11
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Table 4.3 (cont.)
Fatty acid CS1 (CS) CS3 (CS) CS4 (CS) SIF SBB Overall average
(b) P. elegans
n samples 2 3 1 1 2 9
n individuals per sample 5 3-5 5 4 5
Body lengths (mm) 20-28 18-34 20-27 16-24 14-27
Lipids (% DW) 29.22±20.91 40.49±2.94 41.33 38.00 58.29±11.39 41.66±13.54
FA mg g-1 ind.-1 25.95±10.80 41.85±2.67 9.78 32.35 50.71±5.49 20.88±10.03
14:0† 2.80±0.03 2.49±0.29 2.32 3.66 3.65±0.40 2.93±0.60
14:1 (n-5)† 0.02±0.00 0.01±0.00 0.01 0.01 0.01±0.00 0.01±0.00
15:0† 0.40±0.01 0.43±0.08 0.54 0.26 0.24±0.03 0.38±0.11
16:0† 13.88±0.53 17.57±7.04 20.89 23.03 16.62±2.67 17.51±4.69
16:1 (n-5)† 3.18±0.39 2.90±0.51 3.55 2.83 2.41±0.42 2.92±0.49
16:1 (n-7)† 14.69±0.49 16.63±2.90 20.44 14.67 14.19±1.84 15.86±2.57
18:0† 1.01±0.06 1.19±0.44 1.66 1.23 1.17±0.02 1.20±0.29
18:1 (n-7) 5.83±0.82 6.45±2.50 9.22 13.67 9.46±1.48 8.09±2.95
18:1 (n-9)† 8.08±0.06 8.67±2.50 11.29 9.42 8.53±0.45 8.88±1.60
18:2 (n-6)† 1.03±0.18 1.55±0.06 1.88 0.78 0.86±0.02 1.23±0.41
18:3 (n-3) 0.33±0.11 0.31±0.14 0.29 0.15 0.14±0.17 0.26±0.13
18:4 (n-3) 1.01±0.16 1.25±0.49 0.78 0.51 0.79±0.23 0.96±0.37
20:1 (n-7) 0.56±0.04 0.59±0.08 0.77 0.45 0.61±0.07 0.59±0.10
20:1 (n-9)† 6.63±0.51 7.19±1.04 6.75 7.73 6.50±1.86 6.92±0.95
20:4 (n-3) 0.10±0.04 0.10±0.05 0.06 0.03 0.10±0.03 0.09±0.04
20:5 (n-3) 17.72±0.16 13.98±5.72 8.40 12.33 19.37±4.80 15.20±4.93
22:1 (n-7) 0.35±0.04 0.21±0.08 0.26 0.13 0.27±0.02 0.25±0.08
22:1 (n-11)† 3.11±0.59 2.70±0.69 1.67 3.22 3.84±1.31 2.99±0.91
22:5 (n-3) 0.51±0.23 0.32±0.20 0.15 0.25 0.64±0.24 0.41±0.23
22:6 (n-3)† 18.18±0.63 15.00±7.97 8.52 5.35 10.16±4.85 12.84±6.24
24:1 (n-9)† 0.59±0.17 0.47±0.13 0.55 0.30 0.46±0.05 0.49±0.13
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Figure 4.7 Fatty acid biomarkers in Eukrohnia hamata and Parasagitta elegans at different
stations in autumn 2014. Sampling locations are abbreviated: CS, Chukchi Sea; SIF, Scott
Inlet Fjord; GF, Gibbs Fjord; SBB, southern Baffin Bay. From top panel to bottom panel:
mean ratios of the carnivory biomarker 18:1 (n-9)/(n-7), mean proportions of the Calanus
biomarkers ΣC20:1+C22:1 MUFA, and mean ratios of the algal biomarker 16:1/16:0 (± 1
SD). No bars – no data available.
4.5.2.5 Carbon and nitrogen isotopes
In the Baffin Bay region, δ13C values were similar in the two species (Kruskal-Wallis
ANOVA, P = 0.34). In the Chukchi Sea region, δ13C values in Parasagitta elegans remained
similar as in Baffin Bay, but δ13C values in Eukrohnia hamata dropped significantly below
those of P. elegans (Kruskal-Wallis ANOVA, P = 0.00). Interestingly, the lowest mean δ13C
values in the study (-23.1 ± 0.3 ‰), and the highest mean values in the study (-19.2 ± 0.3
‰), respectively occurred in E. hamata and P. elegans sampled at the same Chukchi Sea
station (Table 4.4 and Figure 4.8). In the Baffin Bay region, mean TLs were 2.5-2.7 for E.
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hamata and 2.9-3.1 for P. elegans. In the Chukchi Sea, mean TLs were 3.0-3.3 for E. hamata
and 3.5-3.7 for P. elegans (Table 4.4 and Figure 4.8).
Table 4.4 Mean sample carbon (C) and nitrogen (N) masses, C/N ratios, δ13C and δ15N
values and derived trophic levels (TLs) (± 1 SD) in Eukrohnia hamata and Parasagitta elegans
at different stations in autumn 2014. Sampling locations are abbreviated: CS, Chukchi Sea;
SIF, Scott Inlet Fjord; GF, Gibbs Fjord; SBB, southern Baffin Bay. Also: number (n) of
samples analysed and chaetognaths per sample, as well as body lengths of chaetognaths in
mm.
Station
n samples
(n inds. per
sample)
Body lengths
(mm)
C
(% DW)
N
(% DW) C/N
δ13C
(‰)
δ15N
(‰) TL
Eukrohnia hamata
CS2 6 (4-5) 5-32 46.0±5.8 14.3±1.8 3.2±0.0 -23.1±0.3 14.4±0.5 3.0±0.1
CS4 4 (4-5) 4-32 40.3±5.3 13.0±1.5 3.1±0.1 -22.7±0.4 15.5±0.2 3.3±0.1
CS5 4 (5) 10-32 47.8±0.6 14.9±0.2 3.2±0.0 -22.6±0.3 14.4±0.2 3.0±0.1
SIF 3 (2-5) 9-32 42.0±4.9 13.4±1.3 3.1±0.1 -19.8±0.3 13.4±0.2 2.7±0.1
GF 4 (4-5) 5-31 46.9±1.2 14.8±0.4 3.2±0.0 -20.1±0.3 12.9±0.6 2.6±0.1
SBB 5 (3-5) 4-29 39.6±5.4 12.5±1.6 3.2±0.0 -20.0±0.2 12.6±0.4 2.5±0.1
Parasagitta elegans
CS1 5 (5) 19-35 42.8±1.9 13.7±0.6 3.1±0.1 -19.2±0.3 16.8±0.9 3.6±0.2
CS2 5 (5) 17-32 36.2±10.8 11.5±3.4 3.2±0.0 -19.3±0.2 16.3±0.3 3.5±0.1
CS3 5 (1-5) 6-34 43.9±2.1 14.1±0.6 3.1±0.1 -19.9±0.7 17.1±0.4 3.7±0.1
CS4 4 (1-5) 6-27 45.2±2.1 14.3±0.5 3.2±0.1 -20.0±0.4 16.7±0.7 3.6±0.2
SIF 1 (4) 16-24 30.4 9.7 3.1 -19.8 14.9 3.1
SBB 4 (1-5) 7-27 44.2±3.4 14.1±0.8 3.1±0.1 -19.3±0.8 14.2±0.3 2.9±0.1
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Figure 4.8 Mean sample δ13C and δ15N values and corresponding trophic levels (± 1 SD) of
Eukrohnia hamata and Parasagitta elegans. Station IDs shown next to data points. Results
from Chukchi Sea stations inside red oval. Results from Baffin Bay region stations inside
blue oval (locations are abbreviated: SIF, Scott Inlet Fjord; GF, Gibbs Fjord; SBB, southern
Baffin Bay).
4.6 Discussion
4.6.1 Prey items
Kruse et al. (2010) reported a high degree of diet flexibility in Eukrohnia hamata from the
Southern Ocean, detecting copepods, jellyfish, radiolarians, tintinnids, and diatoms in their
guts. However, copepods comprised almost all prey for Parasagitta elegans in the Barents
Sea (Falkenhaug 1991). In this study, except for the meagre evidence of cannibalism in two
chaetognaths (see Figure 4.5), copepods were the only prey for P. elegans and E. hamata in
the Amundsen Gulf. Copepods taken were the same as in earlier studies; Pseudocalanus spp.,
Oithona spp. and Calanus spp. (e.g. McLaren 1969, Øresland 1990, Falkenhaug 1991). Small
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chaetognaths could ingest relatively large copepods compared to their head width (Figure
4.3).
4.6.2 Predation rates
Our detections of visible prey in only 0.9 % of 4078 Eukrohnia hamata and 0.8 % of 654
Parasagitta elegans (and the corresponding daily predation rates ˂ 0.3 prey ind.-1 d-1), provide
little evidence that either chaetognath species is an important predator on copepods in the
Amundsen Gulf. For P. elegans daily predation rates in Arctic Ocean populations may be
lower than those at lower latitudes (e.g. 5.50 ind.-1 d-1 in the North Sea; Saito & Kiørboe
2001); this is likely an effect of temperature on digestion rates/gut transit times. However,
little information exists on gut transit times in arctic chaetognaths. Lipids inside or outside
the oil vacuole of 63 % of E. hamata may not necessarily reflect recent prey consumption
(Øresland 1990, Kruse et al. 2010), so excluding these from predation rate estimates is wise.
Sameoto (1987) recorded visible prey in just 0.3 % of 2000 E. hamata during autumn 1983
in Baffin Bay, but also reported that lipid “globules” in 63 % of E. hamata resembled copepod
oil sacs. Interpreting these as evidence of recent prey consumption led Sameoto (1987) to
suggest predation rates of 1.8 prey ind. d-1. Based on this earlier estimate, Welch et al. (1992)
suggested that chaetognaths annually ingest 51 % of the copepod biomass in the Lancaster
Sound Region of the Canadian Arctic (164 of 319 kJ m-2 yr-1). However, we suspect that oil
vacuoles in E. hamata individuals were wrongly identified as copepod oil sacs in the Sameoto
(1987) study, and suggest that the estimates of Sameoto (1987) and Welch et al. (1992) are
erroneous.
Øresland (1995) reported little seasonal change in the low predation rates of Eukrohnia
hamata (0.3-0.7 prey ind.-1 d.-1) between austral summer and winter in the Gerlache Strait,
Antarctica. Differences in the seasonal behaviour of Arctic and Antarctic copepods may
affect the seasonal feeding opportunities for meso-pelagic chaetognaths such as E. hamata
(Chapter 3). Our observation of an apparent decline in winter predation in Parasagitta
elegans is consistent with earlier studies in the European Arctic (Øresland 1987, Falkenhaug
1991, Bollen 2011, Grigor et al. 2015). Several studies on this species also reported reduced
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winter growth in arctic and sub-arctic seas (Dunbar 1962, Grigor et al. 2015, Chapter 3 of
this thesis). These observations could suggest a winter decline in predation opportunities,
though individuals >12.5 mm can consume a wide variety of prey size classes > 250 μm
(Saito & Kiørboe 2001), and by migrating from the PML to the PH in winter, it seems that
P. elegans pursued several copepods which showed similar SVM behaviour (see Darnis &
Fortier 2014). Therefore, rather than prey access, changes in energy requirements may be the
main reason for the winter reductions in predation and growth rates. Some studies have
detected diurnal differences in predation rates (e.g. Sullivan 1980, Feigenbaum 1982,
Sameoto 1987, Brodeur & Terazaki 1999), a factor not accounted for in the present study.
For the fragile chaetognaths, an apparent scarcity of prey in guts could also be an artefact of
sampling and observation protocols. Baier & Purcell (1997) suggested prey was lost in 50%
of chaetognaths owing to regurgitation and defecation during net sampling, so a subsequent
study on gut contents of Mediterranean chaetognaths doubled npc estimates to account for
this potential loss (Duro & Saiz 2000). Inference of recent copepod prey from their
undigested mandible remains could also be useful. In a study from the Barents Sea
(Falkenhaug 1991), detections of such mandibles at magnifications of up to 50× suggested
that 35.7 % of Parasagitta elegans individuals had recently consumed small copepod prey.
In this study, Scanning Electron Microscope (SEM) detections of chaetognath hooks, and
copepod mandibles and filaments in the chaetognath guts, confirmed the value of high power
microscopy for chaetognath feeding studies (Figure 4.5).
4.6.3 Omnivory in arctic chaetognaths
Although vegetal remains in guts are generally interpreted as originating in the guts of
digested animal prey, gut contents suggested Eukrohnia hamata is more omnivorous than
Parasagitta elegans. Specifically, the presence of vast amounts of green macroaggregates
and green lipid droplets in E. hamata guts (Figure 4.4), and also the ingestion of green
macroaggregates by living E. hamata individuals (Figure 4.6), are two observations offering
strong evidence for omnivory. The absence of these observations in P. elegans from the same
sampling locations, times and depths, suggest reduced overlap in their feeding strategies.
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Particulate organic matter sourced in the photic zone during spring and summer sinks in the
water column as marine snow, collecting mucus, detritus, protists, bacteria, algae, other
organisms and inorganic material (Alldredge & Silver 1988). Marine snow is identified as a
food source for meso-pelagic copepods (e.g. Dagg 1993, Dilling et al. 1998, Sano et al. 2013),
euphausiids (Dilling & Brzezinski 2004), polychaete larvae (Bochdansky & Herndl 1992),
and fish (Larson & Shanks 1996). Small meso-pelagic copepods and protists which colonize
marine snow may be an important food source for feeding zooplankton.
For polar zooplankton, omnivorous and detritivorous feeding strategies may be useful to
buffer against seasonal prey shortages (Norkko et al. 2007). For instance, the arctic krill
species Thysanoessa inermis may similarly be omni-carnivorous to support growth and
reproduction (Søreide et al. 2006). Eukrohnia hamata mostly resided at meso-pelagic depths
in the Amundsen Gulf, except for some individuals which entered epi-pelagic depths, the
Pacific Halocline, in summer (Chapter 3 of this thesis). As well as adults, juveniles ate marine
snow (Table 4.2), suggesting a role of omnivory in stimulating early growth. ROV dives have
documented aggregations of arctic chaetognaths near the seabed (L Fortier, unpublished
results), where dissolved and fine particulate organic matter occurs in high concentrations
(Iken et al. 2005). In this area, E. hamata may sit-and-wait for marine snow to sink down,
occasionally also capturing the passing copepod. Other chaetognaths in the genera
Archeterokrohnia and Heterokrohnia, known to feed on organic matter and bacteria from
sediments (Casanova 1986), are also closely associated with the nepheloid layer.
4.6.4 Fatty acids and stable isotopes confirm gut contents
4.6.4.1 18:1 (n-9)/(n-7) ratios and Calanus copepod FATMs
18:1 (n-9)/(n-7) ratios ˃ 1 indicate that Parasagitta elegans are typically carnivores.
However, the lower 18:1 (n-9)/(n-7) ratios seen in P. elegans in Baffin Bay (Figure 4.7)
compared the Chukchi Sea are a sign that detritus does contribute more to its diet in the
former region. Moreover, other studies on P. elegans (e.g. Øresland 1987, Falkenhaug 1991)
do not plead in favor of evident carnivory. Unlike in P. elegans, 18:1 (n-9)/(n-7) ratios in E.
hamata populations from different regions were consistently low (~0.2), characteristic of
detritivores such as mud-ingesting seastars (e.g. Howell et al. 2003). Admittedly, care should
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be taken when interpreting 18:1 (n-9)/(n-7) ratios in animals, since 18:1 (n-9) FA could be
synthesized by some primary producers, not only zooplankton. In addition, 18:1 (n-9)/(n-7)
ratios may fluctuate with lipid content (Dalsgaard et al. 2003). Higher amounts of Σ20:1+22:1
MUFA in E. hamata than P. elegans in Scott Inlet Fjord, could indicate that in certain
environments, like fjords, E. hamata takes Calanus copepods more frequently than P.
elegans, which may focus on smaller taxa (e.g. Falkenhaug 1991). Partitioning of food
resources, including zooplankton prey, could allow for the co-existence of the two
chaetognath species in shallow environments.
4.6.4.2 Algal FATMs
Differences in the amounts of 16:0 and Σ16:1 in Eukrohnia hamata and Parasagitta elegans
represent interesting observations of the study. An earlier study conducted in the
hyperbenthic zone of the Beaufort Sea during autumn 2003 and summer 2004 (Connelly et
al. 2014) reported that E. hamata contained the diatom 16:1 (n-7) in similar proportions (21.4
± 4.9 %) to an omnivorous mysid (33.0 ± 5.3 %); (30.93 ± 7.74 in our study), whilst lower
proportions of 16:1 (n-7) occurred in hyperbenthic P. elegans (15.9 ± 2.6 %); (14.5 ± 2.6 in
our study). 16:1/16:0 ratios in hyperbenthic E. hamata were amongst the highest of all the
zooplankters analysed by Connelly et al. (2014), whilst proportions of 16:1 (n-7) in E. hamata
exceeded those in all analysed copepods. Arguably, the high amounts of the diatom markers
16:1 (n-7) and 20:5 (n-3) in E. hamata in both our study (Table 4.3a), and that of Connelly
et al. (2014), reflect direct consumption of diatoms in seawater, consistent with our in-vitro
ingestion observations (Figure 4.6).
4.6.4.3 δ13C values
Several studies have reported a general enrichment in the δ13C values of zooplankton taxa,
including copepods and chaetognaths, as longitude decreased in the Canadian Arctic (e.g.
Dunton et al. 1989, Saupe et al. 1989, Schell et al. 1989, Hobson & Welch 1992, Hobson et
al. 2002). We detected such δ13C enrichment for Eukrohnia hamata but not for Parasagitta
elegans (Figure 4.8). The reason for this difference is unclear, but according to Σ20:1+22:1
MUFA results, the contribution of Calanus copepods to the diet of E. hamata was greater in
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the west than in the east (not the case for P. elegans). This, or other regional differences in
diets may contribute to the observed change in δ13C values in E. hamata.
4.6.4.4 δ15N values and inferred TLs
Consistent with other arctic studies presenting stable isotope data for chaetognaths, our δ15N
observations (Figure 4.8) suggest that Eukrohnia hamata generally feeds at a lower trophic
level (TL) than Parasagitta elegans (Søreide et al. 2006, Pomerleau et al. 2011, Connelly et
al. 2014). Mean trophic level estimates were lowest for E. hamata in the Baffin Bay region
(2.5-2.7), and a full trophic level higher for P. elegans in the Chukchi Sea (3.5-3.7). Pelagic
animals with TLs of 2.4-2.8 are omnivores, and those with TLs of 2.9-3.3 carnivores,
according to one food web model (Søreide et al. 2006). However, in our method to estimate
TLs of chaetognaths, a potential weakness was assigning a constant δ15N value (6.8) to the
POM baseline, at all sampling stations. δ15N estimates for POM (or any baseline) could
change considerably with sampling location and time, as well as differences in the
constituents of the POM, amongst other factors. For comparison, δ15N values for POM in the
Amundsen Gulf between September and October 2011 (˂ 100 m) ranged between 2.2 and
7.2 ‰ (J-É Tremblay, unpublished results).
4.6.4.5 C/N ratios
Interestingly, the presumably lower capacity of Parasagitta elegans to maintain a wax ester
supply (Connelly et al. 2012), did not cause its C/N ratios to differ from those of Eukrohnia
hamata (Table 4.4). Mean C/N ratios for hyperbenthic chaetognaths in the Beaufort Sea
during summer and autumn were 6.6 ± 0.8 for E. hamata and 5.2 ± 0.7 for P. elegans
(Connelly et al. 2012), whereas those of the pelagic chaetognaths in this study were 3.1-3.2.
This is similar to those of pelagic P. elegans in the Barents Sea in early summer (3.2; Ikeda
& Skjoldal 1989). A C/N ratio decrease in the pelagic populations could reflect enhanced
availability of nitrogen above the nepheloid layer (Connelly et al. 2012).
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4.6.5 Morphological explanations
Consistent with the above evidence that Eukrohnia hamata feeds at a lower trophic level than
Parasagitta elegans, this species has fewer posterior teeth and fewer hooks than P. elegans,
and lacks anterior teeth which exist in their counterpart (Furnestin 1965, Terazaki 1993).
Whilst P. elegans hooks are unserrated, the hooks in young E. hamata are serrated (serrations
disappear with age). We suspect that these serrated hooks may be particularly useful for
grabbing falling particles, early in the life cycle.
4.7 Concluding remarks and future studies
Owing to the large size and presumably high abundance of chaetognath fecal pellets,
chaetognath pellets could be important in the flux of carbon to the benthos (Dilling &
Alldredge 1993). However, Giesecke et al. (2010) suggested that a zooplankton-based diet
in taxa such as Parasagitta spp., Solidosagitta spp. and Pseudosagitta spp. cause their pellets
to sink at a slower velocity (5-10 ×), compared to those of other zooplankters known to
mainly consume algae. This could certainly limit the export of fecal-pellet carbon to depth,
as the likelihood of full pellet breakdown in the water column would rise. It is possible that
the pellets of omnivorous Eukrohnia hamata would sink faster, and make more of a
contribution to carbon sequestration. As carbon sequestration by zooplankton may be
important in regulating global climate (Turner 2015), this is an interesting avenue for future
studies. Instead of using intrusive nets, underwater traps that rapidly kill invertebrates with
toxic chemicals may help to reduce prey loss, allowing us to obtain a better impression of
recent feeding. Food choice experiments would help to evaluate preferred food items for E.
hamata and other species.
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5. Chapter 5 – General Conclusions
5.1 Resource use by arctic chaetognaths
The main purpose of this Ph. D. thesis was to shed light on the ecology of two major
chaetognath species that reside in Arctic waters (Eukrohnia hamata and Parasagitta
elegans), with a particular focus on how the species use and share habitat and food resources,
allowing them to co-exist. The bulk of studies on zooplankton ecology in Arctic waters have
focused on grazing copepods such as Calanus spp., whereas many aspects of chaetognath
ecology have received relatively less attention. The data used in Chapters 2-4 were based on
chaetognath samples collected during five years (2007, 2008, 2012, 2013, 2014) in European,
Canadian and Alaskan portions of the Arctic, including a full annual cycle in the Canadian
Arctic (2007-2008). This enabled the acquisition of detailed information on feeding habits
(Chapters 2 and 4), and growth and reproductive dynamics (Chapter 3), over broad spatial
and temporal scales. Relative to many other mesozooplankton, chaetognaths were abundant
components at all locations and times sampled. The following sections re-cap upon how P.
elegans had the most specialized requirements (its distribution and life cycle appeared to be
closely associated with copepod prey), whereas E. hamata showed greater flexibility for food
options and spawning times. Co-existence of the similar chaetognaths E. hamata and P.
elegans in the Arctic is possibly due to reduced temporal and spatial overlaps in their habitats
and feeding strategies; differences that reduce competition between species (Ross 1986).
5.2 Winter ecology in Svalbard
Insights into the activities of chaetognaths during the polar night are presented in all three
manuscripts. Winter ecology is considered a “new field of science” (Lønne et al. 2014), and
the polar night sampling dimension of all three articles represents a particularly important
step forward in our understanding of zooplankton communities. The first of the three articles
(Chapter 2) added to our understanding of Parasagitta elegans ecology during the Svalbard
polar night. We showed reduced winter activity through a low predation rate and the absence
of reproduction (both contrasting spring-summer reports in the European Arctic). Reduced
predation in winter offers one explanation for the low winter growth rates reported in the
same area (Grigor et al. 2014). This could possibly be due to reduced access to prey (although
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P. elegans individuals >12.5 mm can consume many prey size classes > 250 μm, Saito &
Kiørboe 2001), or reduced energy requirements for winter activities, which may be more
likely.
5.3 Life histories, habitats and spawning times
Based on our annual time series in the Canadian Arctic, mostly the Amundsen Gulf, we
predicted similar maximum body sizes (40-45 mm), lifespans (~2 years), and ages at maturity
(1 year+) for Eukrohnia hamata and Parasagitta elegans in this region of the Arctic (Chapter
3). These results suggested that egg laying in these species did not kill chaetognaths, at least
not immediately (contradictory to Kuhl 1938).
Our observations in the Amundsen Gulf showed that the bulk of Eukrohnia hamata
individuals remained in the Atlantic layer (below ~200 m) in all seasons (Chapter 3). E.
hamata bred during all seasons including winter at these meso-pelagic depths, though most
of its spawning occurred in spring. Hatching earlier in the season would give E. hamata a
longer time to feed and develop energy reserves required for the next winter, and this would
lead to higher fitness and a competitive advantage over chaetognaths born later in the season
with little time to store lipids (Varpe et al. 2007). In stark contrast, the bulk of Parasagitta
elegans individuals was restricted to shallower, epi-pelagic depths. P. elegans bred in the
shallower water masses (mostly the Pacific Mixed Layer) later in the season, during summer
and autumn, showing an overlap in both distribution and breeding phenology with specific
copepods (e.g. Calanus glacialis, Darnis & Fortier 2014). Offspring gain because they hatch
near high numbers of suitable copepod prey, ensuring healthy early growth.
I linked the less seasonally restricted spawning cycle of Eukrohnia hamata (compared to
Parasagitta elegans), to it being a capital breeder that can draw upon its considerable supply
of pre-accumulated wax esters (e.g. Lee & Hirota 1973, Falk-Petersen et al. 1987, Donnelly
et al. 1994, Lee et al. 2006, Connelly et al. 2012, Connelly et al. 2016), as its main
reproductive fuel. Capital breeding in E. hamata could also be supported by apparent declines
in lipid amounts in the oil vacuoles when winter breeding occurred (Chapter 3). Based on our
105
interpretations, concurrent food could be more useful for sustenance or to allow E. hamata
to grow a little in winter (Varpe et al. 2007, Varpe 2012, Sainmont et al. 2014a). Peaks in the
frequency of E. hamata presenting oil reserves during the months of negative growth in
length (from January to March), suggest that reserves were not used to fuel growth.
Parasagitta elegans appears to be an income breeder dependent on high prey availability to
reproduce, perhaps because it lacks the storage mechanisms seen in its counterpart (e.g. Lee
& Hirota 1973, Falk-Petersen et al. 1987, Donnelly et al. 1994, Lee et al. 2006, Connelly et
al. 2012, Connelly et al. 2016). Income breeding in P. elegans could also be supported by the
elevated rates of growth and apparent predation in summer-autumn compared to winter-
spring (Chapters 3 and 4) and by seasonal overlaps in the habitats of P. elegans and small
copepods such as Calanus glacialis and Pseudocalanus spp. (Darnis & Fortier 2014, Chapter
3). Although some seasonal vertical migration was apparent in populations of both
chaetognath species in the Amundsen Gulf, the clearest ascent and descent signals were seen
in P. elegans. Ascensions by many P. elegans in the spring-time may have covered distances
close to 200 m. The downward migration of P. elegans in the water column during autumn,
to depths not much deeper than 200 m, also appeared to follow Calanus copepods which
overwintered here (Darnis & Fortier 2014). These copepods are likely to have fueled P.
elegans maturation in winter-spring.
5.4 Food resources
The two species ate copepods and chaetognaths, however predation rate estimates in both
Chapters 2 (Parasagitta elegans) and 4 (Eukrohnia hamata and Parasagitta elegans)
provided little evidence that either species controlled populations of copepods. Although
proportions of analysed P. elegans individuals with visible prey in guts remained below 5 %
in both feeding chapters, the higher proportions in Svalbard (4 %) compared to the Amundsen
Gulf (˂ 1 %) could be due to differences in digestion times, prey abundances, or body
conditions of the analysed chaetognaths.
106
In some ways, the feeding strategies of Eukrohnia hamata and Parasagitta elegans differed
markedly. Our observations also documented thick particulate organic matter (POM) as a
food source for E. hamata across much of the year in the Amundsen Gulf (and during our
limited samplings in the Chukchi Sea). The same gut contents were not apparent in P. elegans
over the entire annual cycle in the Amundsen Gulf (2007-2008). Our observations follow
previous assertions that fine POM and dissolved organic matter (DOM) are important food
sources for chaetognaths (Casanova et al. 2012), as well as stable nitrogen results suggesting
E. hamata to be more omnivorous than P. elegans (Søreide et al. 2006, Pomerleau et al. 2011,
Connelly et al. 2014). The most likely source of these macroaggregates (˃500 µm) is falling
marine snow (grabbed or gulped in seawater), or consumption of material on the seabed.
There were high abundances of E. hamata near the seabed in the Amundsen Gulf, possibly
in the nepheloid layer, where some chaetognath species are known to ingest organic matter
from sediments (Casanova 1986). Grazing of algal cells from ice is unlikely given the meso-
pelagic distribution of E. hamata. Copepods attached to particles may be consumed with
marine snow, and both components provide nutritional benefits for a chaetognath.
Morphological characters in E. hamata, such as the absence of anterior teeth (Furnestin
1965), provide additional and indirect evidence for such omnivory. The head and mouthpart
enhancements of P. elegans (more teeth and hooks) are evidence of a more predatory life
cycle. In-vitro observations also showed this feeding mode in Pseudosagitta maxima, and to
investigate this further, the gut contents of more individuals would need to be analysed.
In the Chukchi Sea (autumn sampling), our observations of macroaggregate consumption by
Eukrohnia hamata in-vitro are useful, but limited by sample size. However, these
observations are reflected by E. hamata fatty acid and stable isotope signatures. In particular,
the high amounts of diatom fatty acid markers in this species offers strong evidence that
diatoms were consumed directly. In Parasagitta elegans, flagellate / dinoflagellate markers
were mixed in with relatively lower amounts of diatom markers (also in Svalbard, see
Chapter 2), and could reflect a direct or an indirect source of algae. However, 18:1 (n-9)/(n-
7) ratios, δ15N values, and δ13C values were all higher in P. elegans than in E. hamata
(especially in the Chukchi Sea), again reinforcing our conclusions that P. elegans tends more
towards carnivory.
107
Marine snow could be a convenient food source for chaetognaths located below the sub-
surface chlorophyll maximum, avoiding the need for considerable migrations in the water
column to obtain high-quality food. Such food could be critical for the early survival of the
≥90 % of Eukrohnia hamata newborns that hatched at meso-pelagic depths in the months of
December, April, June and July. The specialized serrated hooks in young E. hamata could
help them to grab particles (Furnestin 1965). Interestingly, this feature does not remain in the
adults.
5.5 Limitations of the study
5.5.1 Sampling limitations
Chapters 3 and 4 were based mainly on sampling in the Amundsen Gulf, a restricted region
of the Canadian Arctic. However, since the Amundsen Gulf was not sampled during the
autumn, in Chapter 3 we included length data for Eukrohnia hamata and Parasagitta elegans
from other parts of the Canadian Arctic (the Baffin Bay area and Canadian archipelago) to
infer their growth dynamics in autumn. We have concluded that life histories of chaetognaths
may have slightly different in these regions. Ideally, future seasonal studies should aim to
remain in single sampling regions with restricted water mass advection to ensure single
populations are persistently sampled (e.g. Grigor et al. 2014).
5.5.2 Stable isotopes and trophic levels
In Chapters 2 and 4, we extracted lipids to stabilize carbon isotope values. For a given
species, comparisons between the carbon isotope signatures values reported in different
studies can be difficult, as other methods do not always take this additional step (see El-
Sabaawi et al. 2009). Trophic levels were inferred by comparing δ15N values of our samples
with those previously estimated for a food web baseline (we chose POM). We discussed how
differences in the choice of the baseline, and its assigned δ15N value, could alter trophic level
estimates in this and other studies. As for the chaetognaths, δ15N values of any baseline vary
with e.g. location and season. POM is also a mixture of various materials, with a mixture of
δ15N values.
108
5.5.3 Length cohorts
Seasonal growth dynamics and lifespans of Eukrohnia hamata and Parasagitta elegans were
predicted from body length cohorts, identified by visual means in monthly length frequency
distributions (Chapter 3). We noted that cohorts were visually clearer (and therefore growth
and lifespan interpretations were likely to be better), when species produced a single annual
brood or had restricted breeding seasons. Methods that depend less on visual identifications
of cohorts could help to reduce subjectivity, for verifications of growth rates and lifespan.
5.6 Future research avenues
This study identified important differences in how two different chaetognath species utilize
available resources for co-existence in Arctic waters. Another interesting avenue for further
study could be the investigation of the feeding ecology of the two Heterokrohnia species that
reside at bathy-pelagic depths in the Arctic (Dawson 1968, Kapp 1991). In the future,
analyses of the amounts and composition of lipids in chaetognaths throughout a full annual
cycle (as done here for gut contents) would help to clarify how reserves are utilized.
For gut content analyses of chaetognaths sampled in nature, the use of sampling techniques
that are less obtrusive than nets (sediment traps, light traps and others) can be expected to
reduce the sampling biases that corrupt predation rate estimates (Baier & Purcell 1997). Since
small, rapidly digested copepods (e.g. Oithona spp.) may be key chaetognath prey, guts must
be scanned for small body parts such as copepod mandibles (Falkenhaug 1991). This will
certainly require high power microscopy such as Scanning Electron Microscopy (SEM),
which showed promising results in Chapter 4. Information on gut passage time and real
predation rates may also be obtained by incubating chaetognaths in large containers alongside
different prey, providing they can be kept alive, which can be a challenge. Such experiments
could check if Eukrohnia hamata show selectivity for different sizes and types of marine
snow particles, or if this mode of feeding is mostly opportunistic. E. hamata remain part-time
carnivores, so what is the energetic benefit of a diet based mainly on marine snow versus one
based mainly on zooplankton prey? Is marine snow frequently consumed in other E. hamata
109
populations? Analyses of fatty acids and stable isotopes throughout a full annual cycle could
also provide insights into diet switching.
The role of arctic chaetognaths in mediating biogeochemical fluxes (their role in the
biological pump) should be re-considered. The fecal pellets of chaetognaths are large,
carbon-rich and produced year-round due to continued feeding. Large fecal pellets tend to
sink faster when loaded with algal contents and marine snow, and may be more likely to
reach seafloor depths than those of strict carnivores. This is especially the case when excreted
at meso-pelagic depths (Dilling & Alldredge 1993, Giesecke et al. 2010), so the fecal pellets
of Eukrohnia hamata could contribute more to carbon sequestration than previously thought.
A similar conclusion was reached by Casanova et al. (2012), based on their suggestions that
chaetognaths make use of the DOM products of viruses and bacteria.
5.7 A note on climate change
Climate change can affect the populations of grazers by influencing the phenology of primary
production and taxonomic composition of primary producers (Søreide et al. 2010, Leu et al.
2011). Our observations suggest that any future changes in copepod abundances, in response
to climate change, would have more severe effects on Parasagitta elegans than Eukrohnia
hamata, this being due to its greater reliance on copepods. Increased primary production in
ice-free waters (Pabi et al. 2008) could benefit E. hamata due to increased availability of
copepods, protozoans or freshly produced marine snow. Specifically, as the ice-free season
lengthens, the autumn brood of E. hamata (which currently comprises smaller numbers than
its main spring brood) may benefit from the increased food availability provided by new
phytoplankton blooms in autumn. On the other hand, P. elegans may also benefit, now
encountering more herbivorous copepod prey at epi-pelagic depths. Changes in chaetognath
abundances or distributions are expected to affect ecosystems through ‘bottom-up’ and/or
‘top-down’ effects.
110
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126
Appendix A.
Information on the zooplankton samples included in Chapter 2. Sampling date (UTC), station name, latitude, longitude and bottom depth,
sampling gear (MIK or MPS), sampling time (UTC), sampling depths (m). Sampling was horizontal (MIK) in cases where the sampling
depth is given by one number, and vertical (MPS) when given by a lower and an upper depth. The ‘Analyses performed’ column indicates if
haul individuals were analysed for gut contents (GC), data on abundance, maturity, as well as for stable isotope and fatty acid composition.
Each X indicates that 75 Parasagitta elegans from the haul were analysed for stable isotopes (3 x 25 individuals; see Table 2.2), while each
O indicates that 30 individuals were analysed for fatty acid trophic markers (3 x 10 individuals; see Table 2.3). The last column gives numbers
and body lengths (mm) of individuals dissected for gut content analyses, where relevant.
Date
(UTC) Station
Latitude
(°N)
Longitude
(°E)
Bottom depth
(m) Gear
Time
(UTC)
Sampling depth(s)
(m) Analyses performed
n P. elegans dissected :
length range (mm)
12/01/2012 Rijpfjorden (R3) 80.19 22.16 282 MIK 2353 20 GC, XO, abundance 10 : 18-38.5
-"- -"- 80.19 22.11 211 MIK 1146 75 GC, XO, abundance, maturity 40 : 17-55
-"- -"- 80.19 22.15 280 MIK 1220 225 GC, XXO, abundance, maturity 30 : 21-44.5
-"- -"- 80.19 22.16 284 MPS 1310 260-200 Abundance
-"- -"- 80.19 22.16 284 MPS 1310 200-100 Abundance
-"- -"- 80.19 22.16 284 MPS 1310 100-50 Abundance
-"- -"- 80.19 22.16 284 MPS 1310 50-20 Abundance
-"- -"- 80.19 22.16 284 MPS 1310 20-0 Abundance
-"- -"- 80.19 22.16 284 MPS 1350 256-224 GC 10 : 22.5-33
-"- -"- 80.19 22.16 284 MPS 1350 192-160 GC 6 : 24-31.5
-"- -"- 80.19 22.16 284 MPS 1350 160-128 GC 3 : 21.5-29.5
-"- -"- 80.19 22.16 284 MPS 1350 128-0 GC 10 : 15-41
13/01/2012 Rijpfjorden (R3) 80.19 22.16 278 MIK 1104 20 Abundance
-"- -"- 80.19 22.16 275 MIK 0029 75 GC, XO, abundance 11 : 22-44
-"- -"- 80.19 22.16 278 MIK 1136 75 Abundance only
-"- -"- 80.19 22.16 278 MIK 1218 225 O, abundance
-"- -"- 80.19 22.16 281 MPS 0105 260-200 Abundance
-"- -"- 80.19 22.16 281 MPS 0105 200-100 Abundance
-"- -"- 80.19 22.16 281 MPS 0105 100-50 Abundance
-"- -"- 80.19 22.16 281 MPS 0105 50-20 Abundance
-"- -"- 80.19 22.16 281 MPS 0105 20-0 Abundance
-"- -"- 80.19 22.16 281 MPS 0157 256-224 GC 8 : 18-32
-"- -"- 80.19 22.16 281 MPS 0157 224-192 GC 4 : 23-28
127
-"- -"- 80.19 22.16 281 MPS 0157 192-128 GC 10 : 20-31.5
-"- -"- 80.19 22.16 281 MPS 0157 128-20 GC 10 : 17-34.5
-"- -"- 80.19 22.16 284 MPS 0157 20-0 GC 1 : 10
17/01/2012 Mouth of Isfjorden 78.20 15.50 268 MIK 1957 250 GC, XO, maturity 20 : 20.5-42
17/01/2012 Isfjorden ISA 78.16 15.32 98 MIK 2208 35 GC, XO, maturity 10 : 18-46
-"- -"- 78.16 15.33 98 MIK 2238 60 GC, XO, maturity 10 : 20-46.5
18/01/2012 Isfjorden ISA 78.16 15.33 80 MIK 1142 30 GC, XO, maturity
-"- -"- 78.16 15.33 80 MIK 1207 60 GC, maturity 10 : 25-47
27/01/2012 Isfjorden ISA 78.16 15.33 80 MPS 1717 25-0 Abundance only
-"- -"- 78.16 15.33 80 MPS 1727 65-25 Abundance only
12/01/2013 Rijpfjorden (R3) 80.18 22.17 267 MIK 1249 20 GC, maturity 100 : 14-40
16/01/2013 Kongsfjorden 78.58 11.53 327 MIK 0952 30 GC 100 : 8-30
-"- -"- 78.58 11.52 309 MIK 1145 20 GC 100 : 16-41
-"- -"- 78.58 11.53 303 MIK 1255 20 GC, maturity 100 : 17-36
-"- -"- 78.58 11.50 298 MIK 1322 100 GC, maturity 100 : 12-42
-"- -"- 78.58 11.54 308 MIK 1634 20 GC 100 : 15-40
17/01/2013 Kongsfjorden 79.03 11.27 280 MIK 0549 20 GC 100 : 16-41
128
Appendix B.
Vertical profiles of temperature and salinity in Chapter 2. a) Rijpfjorden on 13th January 2012; b) the mouth of Isfjorden on 17th January
2012; and c) Isfjorden station ISA on 18th January 2012. Profiles were obtained by CTD downcast.
129
Appendix C.
Stations sampled in Chapter 3 for information on chaetognath body size and life history characteristics; dates, regions (NF = Nachvak Fjord, PC
= Parry Channel, BB = Baffin Bay, AG = Amundsen Gulf), positions, bottom depths, sampler used (Mn = Multinet, SCn = square-conical net),
sampling strata and sample splits analysed.
Station
ID
Date
(dd.mm.yy) Region Position
Bottom
depth (m)
Sampler
used Sampling strata (m)
Sample
split
600/602 02.08.07 NF 59° 5.25' N, 63° 26.20' W 215 Mn 0-50, 50-100, 100-150, 150-195 1
302 07.10.07 PC 74° 9.30' N, 86° 17.64' W 529 Mn 0-20, 20-40, 40-60, 61-160, 160-300, 300-460, 460-480, 480-500 0.5
308 09.10.07 PC 74° 8.19' N, 103° 7.30' W 346 SCn 0-335 1
1600 02.11.07 AG 71° 40.77'N, 130° 44.21' W 452 SCn 0-358 1
437 23.11.07 AG 71° 43.81' N, 126° 41.37' W 440 Mn 3-21, 21-40, 41-60, 61-161, 161-261, 261-360, 361-380, 381-396, 397-412 1
D3 30.11.07 AG 71° 2.39' N, 123° 58.46' W 320 SCn 0-310 1
D7 14.12.07 AG 71° 26.15' N, 125° 53.12' W 455 Mn 0-21, 21-40, 41-60, 61-150, 151-250, 251-350, 351-370, 372-390, 391-411 0.5
D12-A 26.12.07 AG 71° 14.96' N, 124° 27.10' W 289 Mn 10-30, 30-50, 50-70, 70-120, 120-170, 170-220, 220-240, 240-260, 260-280 1
D17-9 18.01.08 AG 71° 32.50' N, 125° 0.20' W 216 SCn 0-206 1
D17-I 21.01.08 AG 71° 36.20' N, 125° 9.40' W 242 Mn 10-20, 21-40, 40-60, 60-97, 97-133, 134-171, 172-191, 191-210, 211-233 1
D19-B 04.02.08 AG 71° 4.61' N, 124° 49.02' W 354 Mn 2-21, 22-41, 41-60, 61-125, 126-195, 196-264, 265-286, 286-306, 307-325 0.5
D19-E 10.02.08 AG 71° 3.93' N, 124° 46.15' W 365 Mn 0-20, 20-40, 40-60, 60-130, 130-200, 200-280, 300-320, 320-340 1
D26-12 28.02.08 AG 70° 55.79' N, 123° 51.10' W 359 SCn 0-345 1
D26-E 01.03.08 AG 70° 50.40' N, 123° 36.00' W 443 Mn 60-160 1
D27-B 03.03.08 AG 70° 48.87' N, 123° 53.50' W 352 Mn 4-22, 22-41, 41-62, 62-131, 132-206, 207-280, 280-300, 301-340 0.5
D29-27 19.03.08 AG 70° 54.50' N, 123° 28.60' W 401 SCn 0-385 1
D36-8 08.04.08 AG 71° 17.60' N, 124° 30.60' W 260 SCn 0-250 1
D41-D 18.04.08 AG 70° 37.90' N, 123° 57.90' W 499 Mn 0-20, 20-40, 40-60, 60-185, 185-309, 309-340, 376-404, 404-493 1
D41-E 18.04.08 AG 70° 37.30' N, 121° 55.40' W 500 Mn 0-20, 20-40, 40-60, 60-181, 181-303, 303-425, 424-445, 445-465, 465-485 1
D43-F 01.05.08 AG 70° 48.93 'N, 124° 13.33' W 447 Mn 11-20, 21-40, 40-60, 61-161, 161-263, 263-365, 365-385, 385-405, 405-428 1
405b 20.05.08 AG 70° 39.54' N, 122° 52.74' W 521 Mn 11-19, 20-40, 40-60, 60-179, 179-306, 307-430, 431-449, 450-470, 470-497 0.5
6010 26.05.08 AG 71° 31.86' N, 129° 34.20' W 696 SCn 0-684 1
D45-A 31.05.08 AG 71° 13.07' N, 124° 40.94' W 275 Mn 10-20, 20-40, 40-60, 60-105, 105-150, 150-195, 195-215, 215-235, 235-255 1
405c 02.06.08 AG 70° 37.22 'N, 123° 11.01' W 549 Mn 10-20, 20-40, 40-60, 60-197, 197-333, 433-470, 472-490, 490-510, 510-530 0.5
F7-5 08.06.08 AG 69° 49.45' N, 123° 37.97' W 78 SCn 0-70 1
1208-A 28.06.08 AG 71° 3.84' N, 126° 2.66' W 407 Mn 1-24, 24-40, 40-60, 60-156, 157-245, 246-336, 337-356, 357-372, 372-395 0.5
405 21.07.08 AG 70° 41.70' N, 122° 55.47' W 599 SCn 0-580 1
130
405 21.07.08 AG 70° 41.92' N, 122° 55.91' W 592 Mn 20-40, 40-60 0.5
CA16-07 23.07.08 AG 71° 47.62' N, 126° 29.13' W 439 Mn 1-21, 21-40, 41-60, 61-161, 162-261, 261-371, 371-391, 392-411, 411-433 1
CA05-07 25.07.08 AG 71° 18.19' N, 127° 34.80' W 231 Mn 1-20, 40-61, 61-82, 82-121, 122-160, 181-202, 202-220 1
CA18-07 03.08.08 AG 70° 41.74' N, 122° 54.94' W 591 SCn 0-580 1
108 14.09.08 BB 76° 15.98' N, 74° 34.85' W 436 SCn 0-436 1
118 17.09.08 BB 77° 18.62' N, 76° 38.66' W 480 Mn 0-20, 40-60, 60-177, 177-294, 294-410, 410-430, 430-450, 450-470 1
131
Appendix D.
Vertical profiles of temperature, salinity and chlorophyll a (chl a) in Chapter 3: Nachvak Fjord on 2 August 2007; Parry Channel on 7 October
2007; and Baffin Bay on 17 September 2008. Chl a data were provided by Michel Gosselin (Université du Québec à Rimouski).
132
Appendix E-1. Amundsen Gulf stations sampled in Chapter 4: abbreviated station IDs, full station IDs, dates, positions, bottom depths, sampler used and sample
depths. Properties measured are abbreviated: chl a = chlorophyll a biomass; zoop = zooplankton abundance; gc = chaetognath gut contents; vd =
chaetognath vertical distributions. SCn = square-conical net, Mn = Multinet, CTD = conductivity-temperate-depth device. See Appendix C for the
complete list of Multinet sampling intervals.
Station ID
(our study)
Full
station ID
Date
(dd.mm.yy) Position
Bottom
depth (m) Sampler Sample depths (m) Properties measured
1 1600 02.11.07 71° 40.77' N, 130° 44.21' W 452 SCn 0-358 gc
2 1606 03.11.07 71° 33.47' N, 125° 41.51' W 345 CTD 0, 3, 5, 7, 11, 18, 24 chl a
3 1908 05.11.07 71° 8.64' N, 124° 21.17' W 259 CTD 0, 10, 20, 26, 30, 50, 50, 60, 75, 100 chl a
4 405 19.11.07 70° 37.30' N, 123° 0.09' W 640 CTD 10, 40, 80, 80, 120, 240, 500 chl a
5 1100 19.11.07 71° 2.23' N, 123° 15.11' W 281 CTD 10, 30, 60, 80, 100, 267 chl a, zoop
6 437 22.11.07 71° 44.37' N, 126° 38.85' W 420 CTD 10, 30, 50, 100, 200, 414 chl a
6 437 23.11.07 71° 43.81' N, 126° 41.37' W 440 Mn 3-412 zoop, vd, gc
7 D1 28.11.07 70° 25.85' N, 126° 27.44' W 285 CTD 10, 20, 40, 100, 160, 275 chl a
8 D3 30.11.07 71° 2.39' N, 123° 58.46' W 320 SCn 0-310 zoop, gc
9 D4 02.12.07 71° 43.93' N, 125° 33.80' W 247 CTD 10, 40, 60, 90, 160, 232 chl a
10 D5 05.12.07 71° 24.50' N, 124° 50.09' W 217 Mn 2-205 zoop
11 D5 07.12.07 71° 18.30' N, 124° 47.26' W 239 CTD 10, 50, 70, 110, 170, 232 chl a
12 D7 10.12.07 71° 16.22' N, 125° 13.76' W 323 CTD 10, 40, 80, 120, 190, 315 chl a
13 D7 13.12.07 71° 16.22' N, 125° 13.76' W 323 CTD 10 chl a
14 D7 14.12.07 71° 26.15' N, 125° 53.12' W 455 Mn 0-411 zoop, vd, gc
15 D8 16.12.07 71° 24.84' N, 126° 4.69' W 440 CTD 10, 30, 100, 150, 200, 441 chl a
16 D9 18.12.07 71° 46.22' N, 125° 57.94' W 247 Mn 2-230 zoop
17 D12-A 26.12.07 71° 14.96' N, 124° 27.10' W 289 Mn 10-280 vd, gc
18 D12 27.12.07 71° 12.91' N, 124° 28.63' W 280 CTD 10, 40 chl a
19 D12-B 28.12.07 71° 19.68' N, 124° 49.80' W 222 Mn 40-211 zoop
20 D14 03.01.08 71° 14.93' N, 124° 32.20' W 290 CTD 10, 40 chl a, zoop
21 D14-D 06.01.08 71° 32.60' N, 125° 32.10' W 343 Mn 1-333 zoop
22 D14-F 09.01.08 71° 31.60' N, 125° 42.90' W 360 Mn 10-347 zoop
23 D17 17.01.08 71° 31.53' N, 124° 57.97' W 215 CTD 10, 40 chl a
24 D17-E 18.01.08 71° 32.20' N, 124° 59.70' W 217 Mn 10-208 zoop
25 D17-9 18.01.08 71° 32.50' N, 125° 0.20' W 216 SCn 0-206 gc
26 D17-H 21.01.08 71° 36.20' N, 125° 9.40' W 242 Mn 10-232 zoop
133
27 D17-I 21.01.08 71° 36.20' N, 125° 9.40' W 242 Mn 10-233 zoop, vd, gc
28 D17-J 21.01.08 71° 36.20' N, 125° 9.40' W 241 Mn 9-231 zoop
29 D17-K 21.01.08 71° 36.20' N, 125° 9.40' W 241 Mn 9-232 zoop
30 D17-L 21.01.08 71° 36.20' N, 125° 9.40' W 241 Mn 10-232 zoop
31 D19 24.01.08 71° 11.12' N, 125° 8.87' W 319 CTD 10, 40 chl a
32 D19 26.01.08 71° 6.65' N, 124° 56.70' W 312 CTD 10, 40 chl a
33 D19-D 27.01.08 71° 5.50' N, 124° 54.00' W 317 Mn 8-309 zoop
34 D19 03.02.08 71° 4.63' N, 124° 49.00' W 354 CTD 12, 30, 40, 160, 250, 300 chl a
35 D19-B 04.02.08 71° 4.61' N, 124° 49.02' W 354 Mn 2-325 zoop, vd
36 D19-D 08.02.08 71° 4.62' N, 124° 49.01' W 357 Mn 2-331 zoop
37 D19-E 10.02.08 71° 3.93' N, 124° 46.15' W 365 Mn 0-340 vd, gc
38 D19 11.02.08 71° 4.24' N, 124° 47.14' W 371 CTD 5, 12, 50, 60, 160, 250, 350 chl a
39 D19-G 12.02.08 71° 8.91' N, 125° 7.53' W 347 Mn 1-316 zoop
40 D19 14.02.08 71° 27.13' N, 126° 26.94' W 456 CTD 12 chl a
41 D22 18.02.08 71° 18.65' N, 124° 29.80' W 261 CTD 12, 20, 50, 63, 121, 201, 246 chl a, zoop
42 D24-A 23.02.08 71° 26.47' N, 125° 39.80' W 418 Mn 0-400 zoop
43 D26 25.02.08 70° 56.04' N, 123° 55.36' W 357 CTD 12, 20, 60, 80, 150, 200, 342 chl a, zoop
44 D26-12 28.02.08 70° 55.79' N, 123° 51.10' W 359 SCn 0-345 gc
45 D26-D 29.02.08 70° 50.97' N, 123° 39.92' W 425 Mn 2-405 zoop
46 D27 01.03.08 70° 47.43' N, 123° 4.16' W 370 CTD 1, 12, 40, 70, 150, 200, 363 chl a
47 D33-4 03.03.08 70° 48.66' N, 123° 54.90' W 390 CTD 0, 2, 5, 10, 25 chl a
48 D27-B 03.03.08 70° 48.87' N, 123° 53.50' W 352 Mn 4-340 zoop, vd, gc
49 D29-A 05.03.08 71° 0.80' N, 123° 23.30' W 236 Mn 1-230 zoop
50 D29-B 05.03.08 71° 2.52' N, 123° 26.34' W 249 Mn 3-230 zoop
51 D29-C 05.03.08 71° 3.61' N, 123° 27.11' W 252 Mn 2-240 zoop
52 D29-D 05.03.08 71° 4.02' N, 123° 27.13' W 242 Mn 2-230 zoop
53 D29-E 06.03.08 71° 3.94' N, 123° 27.00' W 270 Mn 2-230 zoop
54 D29-F 06.03.08 71° 4.30' N, 123° 27.01' W 236 Mn 3-255 zoop
55 D36 06.03.08 71° 3.97' N, 123° 27.05' W 250 CTD 0, 2, 5, 10, 25 chl a
56 D36 09.03.08 71° 1.09' N, 123° 50.69' W 323 CTD 0, 2, 5, 10, 25 chl a
57 D29 10.03.08 71° 2.32' N, 123° 54.65' W 320 CTD 12, 20, 40, 65, 150, 200, 310 chl a, zoop
58 D29 17.03.08 70° 54.48' N, 123° 28.62' W 401 CTD 2, 5, 10, 50 chl a
59 D31 19.03.08 70° 54.73' N, 123° 1.19' W 444 CTD 0, 10, 25 chl a
60 D29-27 19.03.08 70° 54.50' N, 123° 28.60' W 401 SCn 0-385 gc
61 D29M 19.03.08 70° 54.50' N, 123° 28.60' W 401 Mn 1-386 zoop
62 D33C 28.03.08 71° 3.90' N, 121° 47.20' W 187 Mn 5-181 zoop
134
63 D35A 02.04.08 71° 4.00' N, 121° 56.30' W 213 Mn 0-203 zoop
64 D36C 08.04.08 71° 17.60' N, 124° 30.70' W 259 Mn 0-251 zoop
65 D36-8 08.04.08 71° 17.60' N, 124° 30.60' W 260 SCn 0-250 gc
66 D38 11.04.08 71° 15.52' N, 124° 37.23' W 259 CTD 0, 2, 5, 10, 25 chl a
67 D40 15.04.08 70° 47.89' N, 122° 27.95' W 471 CTD 0, 9, 15, 25, 37, 60, 78, 100 chl a
68 D41 16.04.08 70° 46.65' N, 122° 10.66' W 528 CTD 0, 2, 5, 10, 25 chl a
69 D41C 17.04.08 70° 44.20' N, 122° 8.10' W 541 Mn 2-527 zoop
70 D41-D 18.04.08 70° 37.90' N, 123° 57.90' W 499 Mn 0-493 vd, gc
71 D41-E 18.04.08 70° 37.30' N, 121° 55.40' W 500 Mn 0-485 zoop, vd
72 D41-F 18.04.08 70° 36.50' N, 121° 53.30' W 500 Mn 0-465 zoop
73 D41-G 18.04.08 70° 37.30' N, 121° 51.60' W 514 Mn 0-500 zoop
74 D41 19.04.08 70° 36.52' N, 121° 52.32' W 508 CTD 0, 2, 5, 10, 25 chl a
75 D41-H 19.04.08 70° 35.90' N, 121° 51.00' W 515 Mn 0-500 zoop
76 D41-I 19.04.08 70° 35.90' N, 121° 51.00' W 519 Mn 0-504 zoop
77 D41-J 19.04.08 70° 35.90' N, 121° 51.00' W 519 Mn 0-505 zoop
78 D43-A 23.04.08 70° 36.20' N, 122° 13.00' W 490 Mn 0-475 zoop
79 D43 26.04.08 70° 35.25' N, 122° 26.13' W 550 CTD 0, 2, 5, 10, 25 chl a
80 D43-C 28.04.08 70° 41.33' N, 123° 1.15' W 570 Mn 11-552 zoop
81 D43-1 29.04.08 70° 43.06' N, 123° 17.10' W 459 CTD 0, 2, 5, 10, 25 chl a
82 D43-F 01.05.08 70° 48.93' N, 124° 13.33' W 447 Mn 11-428 zoop, vd, gc
83 D43-2 02.05.08 70° 50.49' N, 124° 26.53' W 475 CTD 0, 2, 5, 10, 25 chl a
84 D43-H 04.05.08 70° 59.99' N, 125° 52.06' W 407 Mn 10-380 zoop
85 D43-3 05.05.08 71° 10.56' N, 126° 18.12' W 420 CTD 0, 2, 5, 10, 25 chl a
86 1020a 06.05.08 71° 1.24' N, 127° 3.10' W 254 CTD 0, 5, 11, 17, 26, 40, 45, 54, 100 chl a
87 6010 06.05.08 72° 31.58' N, 129° 34.50' W 699 Mn 11-680 zoop
88 O2 12.05.08 69° 59.03' N, 126° 2.91' W 205 CTD 11, 18, 26, 40, 54, 75, 100 chl a, zoop
89 405b 19.05.08 70° 39.55' N, 122° 50.74' W 537 CTD 0, 5, 11, 16, 18, 27, 37, 75, 100 chl a
90 405b 20.05.08 70° 39.54' N, 122° 52.74' W 521 Mn 11-497 zoop, vd
91 1011 22.05.08 70° 42.35' N, 124° 0.02' W 455 CTD 0, 6, 13, 21, 30, 32, 51, 69, 75, 100 chl a, zoop
92 6010 26.05.08 71° 31.86' N, 129° 34.20' W 696 SCn 0-684 gc
93 9008 27.05.08 74° 19.91' N, 126° 59.48' W 347 Mn 10-331 zoop
94 D46 30.05.08 71° 13.17' N, 124° 41.11' W 273 CTD 0, 5, 10, 25 chl a
95 D45-A 31.05.08 71° 13.07' N, 124° 40.94' W 275 Mn 10-255 vd, gc
96 405 02.06.08 70° 37.37' N, 123° 11.21' W 546 CTD 0, 10, 14, 22, 35, 53, 73, 100 chl a
97 405c 02.06.08 70° 37.22' N, 123° 11.01' W 549 Mn 10-530 zoop, vd, gc
98 F7-A 07.06.08 69° 49.45' N, 123° 37.97' W 78 Mn 1-78 zoop
135
99 F7-5 08.06.08 69° 49.45' N, 123° 37.97' W 78 SCn 0-70 gc
100 405B 10.06.08 70° 39.85' N, 123° 0.04' W 562 CTD 0, 7, 12, 19, 30, 36, 46, 60, 75, 100 chl a, zoop
101 FB6 15.06.08 69° 58.95' N, 126° 5.18' W 205 CTD 0, 10, 25 chl a
102 FB6-A 16.06.08 69° 58.84' N, 126° 5.30' W 204 Mn 3-190 zoop
103 1216-A 23.06.08 70° 36.69' N, 127° 25.13' W 236 Mn 1-226 zoop
104 1200-A 28.06.08 71° 32.72' N, 124° 20.30' W 207 Mn 1-197 zoop
105 1208 28.06.08 71° 3.87' N, 126° 4.34' W 400 CTD 0, 7, 12, 18, 22, 34, 45, 60, 75, 100 chl a
106 1208-A 28.06.08 71° 3.84' N, 126° 2.66' W 407 Mn 1-395 zoop, vd
107 421-A 01.07.08 71° 27.95' N, 133° 53.78' W 1104 Mn 1-1080 zoop
108 435-A 02.07.08 71° 4.48' N, 133° 47.54' W 300 Mn 2-290 zoop
109 6006-A 04.07.08 72° 39.47' N, 128° 21.56' W 224 Mn 1-211 zoop
110 2010-A 06.07.08 75° 7.28' N, 120° 22.89' W 405 Mn 1-405 zoop
111 410 08.07.08 71° 42.34' N, 126° 29.26' W 395 CTD 0, 12, 29, 33, 54, 75, 80, 100, 108, 200, 388 chl a
112 410-A 08.07.08 71° 41.96' N, 126° 29.18' W 404 Mn 1-392 zoop
113 416 10.07.08 71° 42.16' N, 126° 7.42' W 236 CTD 0, 12, 21, 33, 52, 75, 78, 80, 100, 108 chl a
114 1100 11.07.08 71° 2.66' N, 123° 16.36' W 265 CTD 0, 7, 12, 18, 29, 46, 60, 75, 100, 200 chl a
115 1100-A 11.07.08 71° 2.58' N, 123° 15.58' W 270 Mn 2-261 zoop
116 403-10A 20.07.08 70° 5.46' N, 120° 8.90' W 410 CTD 5, 8, 14, 28, 35, 54, 73, 100, 200, 400 chl a
117 405-10A 21.07.08 70° 41.15' N, 122° 54.08' W 584 CTD 4, 9, 16, 26, 37, 41, 62, 75, 84, 100, 200, 400 chl a
118 405 21.07.08 70° 41.70' N, 122° 55.47' W 599 SCn 0-580 zoop, gc
119 437 23.07.08 71° 41.64' N, 126° 36.01' W 441 CTD 3, 11, 18, 29, 46, 55, 70, 75, 95 chl a
120 CA16-07 23.07.08 71° 47.62' N, 126° 29.13' W 439 Mn 1-433 zoop, vd, gc
121 408 25.07.08 71° 18.83' N, 127° 36.15' W 200 CTD 0, 9, 15, 25, 39, 55, 59, 75, 80, 100, 192 chl a
122 CA05-07 25.07.08 71° 18.19' N, 127° 34.80' W 231 Mn 1-220 zoop, vd
123 CA08-07 27.07.08 71° 8.73' N, 126° 8.12' W 402 Mn 1-393 zoop
124 CA04-07 30.07.08 71° 5.57' N, 133° 45.24' W 335 Mn 1-327 zoop
125 2008-10A 02.08.08 71° 19.95' N, 126° 13.09' W 442 CTD 5, 8, 13, 21, 51, 70, 75, 100, 200 chl a
126 405-10A 03.08.08 70° 40.03' N, 122° 59.01' W 536 CTD 0, 5, 8, 13, 21, 32, 43, 75, 100, 200 chl a
127 CA18-07 03.08.08 70° 41.74' N, 122° 54.94' W 591 SCn 0-580 gc
136
Appendix E-2.
Chukchi Sea and Baffin Bay stations sampled in Chapter 4: abbreviated station IDs (see
Figure 4.1b and Figure 4.1c), full station IDs, dates, positions, bottom depths, sampler
used and sampling depths. For square-conical net sampling, selected mesh size and tow
type are also shown (O = oblique tow, V = vertical tow). FA = fatty acids, SI = stable
isotopes. *Analysis performed on Eukrohnia hamata, +analysis performed on Parasagitta
elegans (see ‘Method’).
Station ID
(our study)
Full
station ID Date Position
Bottom
depth (m)
Sampler
(SCn mesh, tow type)
Sampling
depths (m)
Parameters
measured
Chukchi Sea
CS1 1034 13.09.14 71° 54' N, 154° 58' W 379 SCn (750 µm, O) 0-90 FA+, SI+
CS2 1030 14.09.14 72° 13' N, 153° 58' W 2081 SCn (750 µm, O) 0-90 SI+
CS3 1085 16.09.14 75° 3' N, 167° 8' W 254 SCn (750 µm, O) 0-90 FA+, SI+
CS4 1100 18.09.14 75° 4' N, 161° 16' W 1985 SCn (750 µm, O) 0-90 FA+, SI+
CS4 1100 18.09.14 75° 4' N, 161° 16' W 1985 SCn (200 µm, V) 0-1972 FA*, SI*
CS6 1115 20.09.14 73° 54' N, 147° 11' W 3773 SCn (200 µm, V) 0-999 SI*
CS7 1130 22.09.14 72° 36'’ N, 144° 44' W 3234 SCn (200 µm, V) 0-1000 SI*
Scott Inlet Fjord
SIF PCBC-2 01.10.14 71° 5' N, 71° 50' W 693 SCn (500 µm, O) 0-90 FA+, SI+
SIF PCBC-2 01.10.14 71° 5' N, 71° 50' W 693 SCn (500 µm, V) 0-685 FA*, SI*
Gibbs Fjord
GF Gibbs-B 01.10.14 70° 46' N, 72° 14' W 440 SCn (500 µm, V) 0-430 FA*, SI*
Southern Baffin Bay
BB 180 03.10.14 67° 28' N, 61° 42' W 214 SCn (500 µm, O) 0-90 FA*+, SI*+