Tidal Signatures in the upper Atmosphere from the Equator to the Pole Chao Xiong 1 , Hermann Lühr 1 , Claudia Stolle 1 , and Jorge Chau 2 1. Helmholtz Centre Potsdam, GFZ German Research Centre for Geosciences, Telegrafenberg, 14473 Potsdam, Germany. 2. Leibniz Institute of Atmospheric Physics, Kühlungsborn, Germany. DFG-SPP “1788 DynamicEarth” GFZ Potsdam, 03-04 July, 2014
Transcript
Slide 1
Tidal Signatures in the upper Atmosphere from the Equator to
the Pole Chao Xiong 1, Hermann Lhr 1, Claudia Stolle 1, and Jorge
Chau 2 1. Helmholtz Centre Potsdam, GFZ German Research Centre for
Geosciences, Telegrafenberg, 14473 Potsdam, Germany. 2. Leibniz
Institute of Atmospheric Physics, Khlungsborn, Germany. DFG-SPP
1788 DynamicEarth GFZ Potsdam, 03-04 July, 2014
Slide 2
WN4 and WN3 as well as Midlatitude Summer Night Anomaly (MSNA)
Equatorial region ? Northern hemi Southern hemi Weddell Sea Anomaly
(WSA), first observed by an ionosode in the 1950s (Bellchambers and
Piggott, 1958; Penndorf, 1965). Midlatitude Summer Night Anomaly
(MSNA) observed by satellites observations (Lin et al., 2009;
Thampi et al., 2010; Liu et al., 209). (Liu et al., 2010) (Lhr and
Manoj., 2013) Equatorial Electrojet Electron density
Slide 3
Wave-1 and Wave-2 patterns of MSNA in the two hemispheres
(Xiong and Lhr., 2014) Electron density Thermospheric mass density
CHAMP -40~-60 MLAT GRACE 40~60 MLAT
Slide 4
Swarm Observations during solstice seasons
Swarm-ASwarm-BSwarm-C Swarm-ASwarm-BSwarm-C Dec. S. 2013 Southern
hemisphere June. S. 2013 Northern hemisphere
Slide 5
The opportunity Swarm provides us Pole Equator
Ionosphere-Thermosphere (IT) Lower Atmosphere Mesopause 0 km 500 km
Tides Atmosphere-Ionosphere Coupling by Tides & Planetary Waves
plasma flow tidal penetra tion B E tidal dynam o tidal dissipation
O3H2OO3H2O Tides Atmosphere-Space Interaction Region PWs E equator
ial anomal y compositio n changes wind transpo rt The primary
mechanism through which energy and momentum are transferred from
the lower atmosphere to the upper atmosphere and ionosphere is
through the generation and propagation of waves (Forbes et al.,
2014). The Swarm constellation provides us good opportunity for
better understanding the Atmosphere- Ionosphere (AI) coupling
mechanisms at different latitude regions: 1. Analyzing the tidal
signatures of ionospheric and thermosperic quantities. 2. Compare
the tidal signatures at different altitudes. 3. Compare the Swarm
in situ observations with groundbased measuremtns, to separate the
different sources of the tides.