o
AE-109
The Properties of CaSO4: Mn
Thermoluminescence
Dosimeters
Bengt Bjärngard
AKTIEBOLAGET ATOMENERGISTOCKHOLM, SWEDEN 1963
AE-109
THE PROPERTIES OF CaSO^Mn THERMOLUMINESCENCE DOSIMETERS
Bengt Bjärngard
Summary;
The properties of the radio the rmolumine s cence of CaSO,:Mn,
used for dosimetry of gamma and roentgen radiation, have been in-
vestigated. The light yield of the luminophor has been determined
to 1. 5 percent for 1 MeV gamma radiation. The dependance of the
the rmolumine s cence light sum on the exposure, the exposure rate,
and the exposure time can qualitatively be described by the first
order process model, modified by a broad energy distribution of
the electron trap depths. Some applications are discussed. The
cheapness of the dosimeters, the convenient read-out, and the
broad range of measurable exposures suggest that CaSO,:Mn can
be a valuable complement to other dosimetry systems.
Printed and distributed in June 1963.
LIST OF CONTENTS
Page
1. Introduction 3
1.1. Thermoluminescence 3
.1.2. The thermoluzainophor CaSO,:Mn 5
2. Experimental 5
2. 1. Preparation of the CaSO4;Mn 5
2.2. The luminophor samples and the read-out
apparatus 7
3. Results 9
3, 1. Emission spectrum 9
3.2. Glow curve 9
3, 3. Stability of the thermoluminescence signal 9
3. 4. Light yield 1 1
3,5. Electron shielding 14
3. 6. Variation of the sensitivity with the photon
energy 15
3, 7. Dependence of the sensitivity on exposure,
exposure rate,and exposure time 16
3. 8. Influence of large exposures on the sensitivity 19
3,9. Influence of the irradiation temperature 19
3. 10. Background phenomena 19
4. Discussion 20
References 22
Table I 24
Figures 25
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1. Introduction
This report deals with the properties of the CaSCK:Mn thermo-
luminescence dosimeter. These have been studied in connection with
an effort to develop a system for measurements of small exposures
of gamma radiation. A preliminary notice on the latter subject has
been given [ i] o
1. 1. Thermoluminescence
Thermoluminescence is a special aspect of phosphorescence. A
phosphorescent material emits light after exposure to ultraviolet light,
ionizing radiation, or some other exciting agent. The properties of
this phosphorescence can often be described with a simple model, in
which the excited electrons are trapped in metastable states, from
which they can escape and return to ground state under emission of
luminescence photons. The probability that an electron, which is caught
in such a trap, leaves it in unit time is
p = v eXp (-E/kT) (1).
Here k is Bolzmann's constant, T is the absolute temperature, and
v and E are parameters of the trap. E is identified as the trap depth
and v is a frequency factor, which can be assumed to be independent
of the temperature T.
If n is the number of electrons in (monoenergetic) traps in a
phosphor sample, n will vary with the time t and the temperature T as
^ = - n . P(T) (2).
If the probability that a photon is emitted when an electron leaves
a trap is c, the number of photons emitted per unit time by the phos-
phor sample is
I=~ c | S = C e n . p ( T ) ( 3 )
- 4
If the temperature of the sample is raised, the value of p in-
creases. This results in a momentarily increased phosphorescence
emission, provided that c, the number of photons emitted per emptied
trap, is temperature independent. In this way the phosphorescence
can be thermally stimulated. A special case occurs when the tempe-
rature of the sample must be raised considerably above the tempera-
ture during the excitation for the phosphorescence light to be emitted.
This kind of thermally stimulated phosphorescence is generally called
the rmolumine s cence.
According to eq. (2) the number of trapped electrons at the time
t is, if the temperature T has been constant,
n(t) = nQ exp (-pt) = nQ exp (-vt e"E/kT) (4)
where n is the number of trapped electrons when the excitation was
finished at t = 0. If the temperature now is raised sufficiently, all
these electrons will leave their traps in a comparatively short time.
The associated number of photons or a fraction of them can be measu-
red as a "thermoluminescence signal". This signal is independent of
the temperature variation T(t) of the sample, if the number of emitted
photons per escaping electron is 'ndependent of the temperature. Of
course, the variation of the emission with time will be different for
different temperature cycles T(t).
A special way of heating the luminophor sample is when the
temperature increases linearily with time. The variation of the light
emission with temperature is then called a "glow curve". This curve
shows one or more "glow peaks", corresponding to the emptying of
electron traps of different depths. The interpretation of glow curves
is generally complicated by continuous and often broad distributions
of the trapping levels.
- 5 -
1. 2« The thermoluminophor CaSO :̂Mn
CaSCKsMn has a siraple glow curve. Above room temperature
there is only a single glow peak, which lies at about 100 C, which
implies that the decay of the excited thermoluminescence signal is
considerable already at room t-jmperature. This limits the number of
possible applications in dosimetry but is not solely a disadvantage
since the read-out temperature can be moderate, which simplifies
the read-out procedure as well as the dosimeter construction. Other
advantages of CaSO4:Mn are that it has a high sensitivity to ionizing
radiation and that it is simple to prepare, CaSO ,!Mn has a mean atomic
number that is high compared to that of air, and a rather strong depen-
dence of the signal per unit exposure on the photon energy can be ex-
pected,
CaSO.sMn was one of the first thermoluminophors used for
dosimetry of ionizing radiation. Its thermoluminescent properties
were known before 1900, and it had been used for measurements of
ultraviolet radiation, e.g. by Watanabe [2] , when Burger, Lehmann
and Mayer [ 3J in 1954 tried it for dose measurements in radiation
therapy,
Paterson and Friedman[ 4] found CaSO.sMn favourable for
milliroentgen dosimetry, and Nosenko, Revzin,and laskolko measured
5 mR of gamma radiation with CaSO4:Mn powder [ 5] » Archangelskaja,
Weinberg and Razumova devised a method to propare monocrystals
of CaSO ,;Mn [ 6j , Recently, Spurny used monocrystals of CaSO .:Mn
in an emergency dosimeter [ 7J .
2, Experimental
2, 1, Preparation of the CaSO,sMn
Several methods to prepare thermolumine scent CaSO.;Mn have
been described in the literature. The one that has been most commonly
used [ 2, 8] is to heat a mixture of CaSO,. 2HOQ and MnSO ,• H_O to
- 6 -
about 1000 C, The activating Mn ions are captured in and possibly
also diffused into the anhydrite crystals as these grow at the elevated
temperature. In common with the precipitation technique of Medlin [ 9l,
this method gives a powder of small crystals. Monocrystals of CaSO,;Mn
can be grown in a melt of CaSO,, MnSO, and NaCl [6, 7J .
The CaSO^:Mn used in this investigation was prepared by heating
a mixture of the sulphatess This method was chosen at an early stage
because it was simple and gave the largest sensitivity in a series of
samples prepared with the three methods. This result is far from de-
finite, however, since the Influence of the preparation variables on the
sensitivity was not investigated at this time.
Such a study was made only for the glow method. As a whole the
results agree with those of other Investigators. As recommended by
Watanabe [ 2] it was found favourable to mix the sulphates with diluted
sulphuric acid. If the heat treatment is performed in a slightly reducing
atmosphere, as was used by Peter [ 8] , the sensitivity can be made
3 - 4 times higher than if the sample is heated in air. The optimum
Mn concentration was found to be about one mole MnSO * per hundred
moles of CaSO,. This figure applies to the original mixture of the sul-
phates. Only a fraction of the Mn ions present is incorporated in the
crystals formed L.9I » but no effort was made to determine this fraction»
The following preparation method has been used for the CaSO ,;Mn
with which this investigation has been performed. The ingredients have
been of pro analysi purity.
CaSO.»2H«O and one mole percent MnSO.»H?O are mixed with
dilute (25 %) H-SO, to a slurry. The mixture is left at room temperature
for 16 hours. The water is driven off at 80-90 C and the sulphuric acid
at 250 - 300 °C. The mixture.is then heated at 900 °C for 45 minutes in
a slightly reducing atmosphere (N~ and SO_). The crucible is rapidly
cooled and the powder ground by hand In a mortar.
— 7 -
A glow temperature between 900 and 1000 C gives the best re-
sult and in this temperature region the glow time is not critical within
1 5 to 135 minutes. At higher temperature or longer glow time the sen-
sitivity of the luminophor decreases. This is due to the formation of
manganese oxides, which give the powder a brownish tone. When these
oxides are washed away, the sensitivity of the powder increases some-
what, but the washing has no effect for powders prepared under opti-
mum conditions.
Most of the crystals prepared in this way have a largest size of
about 50 [i. No difference in sensitivity with the size could be detected
for crystals from the same preparation. Small spots of a sample of the
crystalline powder show a greater brightness than the rest of the sample
when heated after irradiation. No satisfactory explanation for this has
been found. Evidently the sensitivity varies considerably between cry-
stals of the same preparation, but this is not determined by the dif-
ferences in size. From this it can be suspected that the sensitivity of
the luminophor can be increased, presumably with a method that allows
more sharply defined values of the preparation variables, as the mo-
nocrystal method does.
The CaSO.:Mn powder was fastened to 0. 1 mm thick Kanthal '
strips, 53 mm by 20 mm, with silicon resin (Dow Corning MC 805).
The powder was mixed with the diluted re.sin, and the slurry was pain-
ted onto the Kanthal strip. The solvent was allowed to evaporate at
room temperature for at least an hour. The phosphor samples were
then baked at 200 C for some hours. This layer is not damaged by
the heating during read-out, provided that the temperature does not
exceed 250 C.
The luminophor has been heated during read-out by a current
Kanthal is an alloy of Fe, Cr, Al and Co. The quality used has aresistivity of 1.35 ohm. mm /m.
- 8 -
through, the Kanthal strip. The temperature increase of the sample
was not measured directly; it was found to be sufficient to maintain
constant the current in the strip by manual regulation. The tempera-
ture of the sample increases with time to a limiting value that nor-
mally has been about ZOO C. The temperatu
30 seconds after the current is switched on.
mally has been about ZOO C. The temperature reaches 100 C about
The light that is emitted by the heated sample has been detected
by an EMI type 6097 S photomultiplier, selected for its relatively
small dark current. Normally the anode current of the multiplier has
been integrated by a polystyrene condenser, the voltage of which has
been measured with a Keithley model 610 electrometer. In some spe-
cial cases (glow curves, large exposures) the anode current was
amplified by the Keithley instrument and recorded. The area under
the curve was then graphically evaluated. All measurements have
been intended to integrate the thermally stimulated emission of .light
from .all the traps associated with the 100 C glow peak, i.e. a repea-
ted read-out for the same dosimeter should give a signal that is
negligible compared to the first one.
By means of a slide the sample strip was introduced in a light-
proof box containing the photomultiplier. The strip was then clamped
to the two heating current electrodes in a well reproducible position
beneath the photocathode, - The reproducibility of the measurements
of the thermoluminescent signals was within;! 3 % with condenser
integration. For large exposures the sensitivity of the photocathode
may change because of the heavy illumination. This effect was studied
and corrected for, but some uncertainty remains and with graphical
integration, used for large exposures, the reproducibility was within
:t 8 %.
- 9 -
3, Resu l t s • • • .
3, 1, Emission spectrum
The spectrum of the thermally stimulated phosphorescence of
CaSO ,:Mn in the region of visible light was studied with a spectrq-
photometer (Zeiss type PMQ II), As is' shown by Figure 1 the emission
spectrum extends from about 4500 A to about 5900 A with a maximum
at 4970 Å. The full width at half maximum, is about 500 Å. Archangelskaja
et alii [ 10] reported a very similar spectral distribution, only some-
what broader. This might be caused by different temperatures of the
samples during the measurements. In our case the temperature was
about 80 °C..
Our CaSO ŝMn shows however a small component of light with
maximum intensity at about 5400 A, which has a considerably higher
thermal stability than the main phosphorescence. It showed up in the
spectrum recordings only when the main phosphorescence had decayed.
3,2, Glow.curve
The glow curve of our CaSO. :Mn was registered with the EMI
6097 S photomultiplier. The temperature of the sample was measured
with a thermocouple and the heating rate was manually adjusted. The
results agree with those of other inve stigator ss e.g. Medlin[9l»A
single glow peak with maximum at about 100 C Was found. From
the results with the spectrophotometer the glow peak associated with
the 5400 A emission was expected to show up slightly under 400 C.
However, it could not be separated from the main peak and the back-
ground of red heat glow. Probably it is identical with the peaks re-
ported by Moore [ 1 11 at about 350 C.
3. 3. Stability of the thermoluminescence signal
As was mentioned above there is an appreciable decay of the
excited thermoluminescence signal of CaSO.tMn at room tempera-
ture. This decay manifests itself as a phosphorescence. If the num-
ber of photons emitted per released electron is independent of the
- 10 -
temperature, the phosphorescent light emission is exactly equal to
the rate of decrease of the thermoluminescence light sum. Experi-
mentally, this was found to be the case for the phosphorescence at
room temperature, - The phosphorescence of CaSO .;Mn has been
studied by Medlin [l2] ,
The most important parameter for the decay of the thermolu-
minescent signal, i.e. for the phosphorescent light emission, is
the temperature after the irradiation. Because of the broad energy
distribution of the relatively shallow traps, the irradiation tempera-
ture, time, and exposure influence the rate of decay. So does the
time that has elapsed since the irradiation. Figure 2 illustrates how
the signal decays at 25 and 37 C. The initial rates of decay are 6
and 15 % per hour respectively. At -25 C the decay is very smallj
less than 10 % are lost during the first 70 hours. These data were
obtained with short irradiation times (5 minutes), the irradiation
temperature 22 C, and an exposure of 300 mR, If 10 hours are
used to give the same exposure, the initial rate of signal decay is
less than 1 % per hour at room temperature. This shows the depen-
dence of the decay on the irradiation time, and it reflects how the
distribution of trapped electrons is shifted to deeper traps when the
irradiation time increases. - The influence of the dose with constant
irradiation times was not large enough to be measured and therefore
should be negligible for most purposes.
In the measurements described below, the normal procedure
has been to read out the dosimeters one hour after the end of the
irradiation. This time includes the transport from the irradiation
laboratory, which has taken about 10 minutes at an approximate tem-
perature of 22 C. During the rest of the time the dosimeters have
been stored at 25 C. If the dosimeters for some reason could not be
read immediately after this standard storing procedure, they were
deposited at -25 C until read-out, though never for more than 8 hours.
~ 11 -
3. 4. Light
The amount of light per unit exposure that is emitted by an irra-
diated dosimeter per unit coated area must increase with the thickness
of the layer up to a saturation value. To study this, and especially to
find out at which thickness saturation occurs, a set of dosimeters were2
prepared with varying amounts of CaSO ,:Mn covering an area of 1 cm .137These dosimeters were irradiated with gamma radiation from Cs .
After the normal storing at 25 C for 1 hour, the dosimeters were
heated and the light emitted in the forward direction was measured with
a photomultiplier. The amount of light emitted through the surface of
the layer per unit mass of the luminophor varies with the thickness
of the layer in the way shown by Figure 3. It is constant for thin layers,
increases to a maximum level, and finally decreases as the thick-
ness of the layer is increased. The increase must be the result of
reflection of light by underlying grains, and the final decrease is
caused by absorption of light within the grains and in the remains of
the silicone resin. This absorption is not large. Above 100 mg/cm ,
which was the thickest layer studied, the emission per unit area con-
tinues to increase when the layer is made thicker, which means that
light from the deepest portions of the layer still reaches the surface. -
The dosimeters were covered with 4 mm perspex. during the irradiation
(cf. below)o Qualitatively the same behaviour as in Figure 3 for Cs
gamma radiation was measured for roentgen radiation with the half
value layer thickness 3. 2 mm aluminium.
For very thin layers the reflections by neighbouring grains can
be neglected. The effective reflection factor for the Kanthal support,
which was measured separately, was also found to be negligible. This
makes it possible to determine with a simple method the number of
photons emitted by the luminophor per unit exposure,
A photomultiplier was calibrated against a 1 candle tungsten
wire lamp with the colour temperature 2700 K , The solid angle of
the photocathode, which has the effective area S, could be written
as S/b steradians for the distance b used between the cathode and the
i) The lamp was calibrated by Lumalampan AB, Stockholm
- 12 -
.wire of the lamp. A current I amperes was measured. It can be shown
that
g(X) dX(5).
N(X) V(X) dX
Here N(X) is the photon spectrum of the lamp* g(X) is the spectral
sensitivity of the photomultiplier in coulombs/photon, and V(X) is the
spectral sensitivity of the eye in lumen, sec/photon. L, finally," is the
source intensity of the lamp in candles.
A thin luminophor sample was then heated in front of the photo-
multiplier. The solid angle of the cathode was in this case S/a • Since
the reflection of the luminescence photons by support and grains can
be neglected, n. S/a photons reach the photocathode if n photons are
emitted per unit solid angle. The photomultiplier gives a charge Q
coulombs at the anode and
n o (X) g(X) d\ (6)
where n (X) is the photon spec t rum of the luminescence , normal i sed
to one photon totally.
From eqs. (5) and (6)
,CN{X) g(X)
i b
2 ,CN{X) g(X) dX L. J_; ^
J N(X) V(X) dX U (X) g(X) dX
In this way the light yield of the CaSO. ,'Mn was de termined. The
function V(X) was calculated from data in a r e p o r t by Condas [ i 3 j ,
- 13 -
the function g(^) was taken from data in EMI's manuals, and. the spectrum
of the lamp N(X) was calculated from data in de Vos's tables [ 14J . For
g(X.) and N(\) the absolute magnitude drops from the final results, which
simplifies the calculations. The luminescence spectrum was taken from
Figure 1 „
12The light yield was found to be 0. 31 x tO photons emitted per;60 •
gram and roentgen of Co gamma radiation. During the irradiation
the phosphor strip was covered with a 4 mm thick per spex sheet. The
normal storing at 25 C for t hour preceeded the measurement, and
6 % of the stored light has been emitted during this time (Fig. 2).
For Co gamma radiation most of the excitation is caused by
electrons, generated in the perspex but passing into the CaSO.:Mn.
This can be seen from Figure 4. Some of these electrons are back-
scattered by the Kanthal support. This effect was studied with beta
•radiation and the increase in excitation because of the presence of the
Kanthal support should be less than 10 %. The dose to the luminophor
layer can be estimated as
D. = D • -g . l u m . . . (8)lum perspex S
if the backscattering of electrons is. neglected. D is the dose per unit
exposure and S is the mass stopping power for electrons, Perspex
can be considered as air equivalent, and the dose per unit exposure
D is then 0, 88 rad/R. The ratio of stopping powers has beenperspex ' ^r & *
estimated to 0. 92. The energy absorbed by the CaSO,:Mn when a
dosimeter is irradiated with 1 R of Co gamma radiation is then
0. 81 rad, and the yield of the luminophor is
120.31 x 10 2_photons/g.R 1 , . / , ,
- _• £ /-&:.— = _ — photons/eV.0.81 rad/R f ö
- 14 -
Since the energy of a luminescence photon is about 2. 5 eV and. one
photon is emitted per 160 eV absorbed, the energy yield is about
1.5 %, i.e. 1.5% of the energy absorbed is re-emitted as visible
light.
For LiF, Morehead and Daniels [i5J determined that 0. 005 %
of the gamma radiation energy absorbed was stored in electron traps.
Our comparisons between CaSO ,:Mn and L.iFj like that of Morehead
and Daniels from Harshaw Chemical Inc. but of a later date (1962),
give the same figure. A natural fluorite, modified by MBLE in Brussels
and kindly put at our disposal, was found to give 1. 6 times as much
light (sum of three glow peaks) as our CaSO^Mn. This figure agrees
with the results of measurements at MBLE that 100 eV are absorbed
per emitted photon for the fluorite [ 16] .
3, 5, Electron shielding
For measurements of exposures it is important that the response
of the dosimeter is determined by the flux of photons through the boundary
surfaces of the dosimeter. The electrons that pass through these sur-
faces from outside must not be allowed to give any contribution to the
signal. If they do, the signal per unit exposure will be influenced by
the geometrical arrangements of the irradiation. This is a principle
that is sometimes overlooked. Figure 4 can be used as an illustration.
It shows the signal per unit exposure for a luminophor strip covered
by various thicknesses of perspex in a collimated and in an uncollimated
beam of gamma radiation. The high value without covering perspex for
the uncollimated beam is due to electrons, generated in the environment
by the gamma radiation. The curves show that it is necessary to use
some kind of covers, thick enough to stop the most energetic electrons
present in an irradiation experiment. We have used 4 mm thick perspex
covers in all irradiations described below.
- 15 -
3, 6. Variation. of_the_ sensitivity with the photon energy
The variation of the sensitivity, i. e. signal per unit exposure,
with the energy of the electromagnetic radiation for a CaSO.sMn dosi-
meter, consisting of a Kanthal strip coated with luminophor and co-
vered with perspex, is complicated by the discontinuities in medium.
Let us restrict the discussions to the case when the photons are incident
perpendicularly upon the phosphor coated side of the strip. At low photon
.energies the exciting electrons are generated within the luminophor, but
at high photon energies, say t MeV, most of the exciting electrons are
generated within the perspex (Fige 4). However, it can be shown that
the ratio between the sensitivities for 1,25 MeV radiation (Co ) and
0.027 MeV radiation (I )[i7] is approximately given by the same re-
lation as would have been valid if the sample had been irradiated under
electron equilibrium conditions in both cases?
' °27)airs(0.027)
Here (J. is the mass energy absorption coefficient, and it is
assumed that the light yield of the luminophor is energy independent
and that the nuclear electron backscattering by the Kanthal support
can be neglected. The measured ratio between the sensitivities is
about 10 % larger than the value calculated from_eqt, .{9), The diffe-
rence can partly be ascribed to the influence of electron backscat-
tering, and it can be concluded that the light yield of the CaSO.jMn
is practically energy independent between 25 keV and 1.25 MeV.
With the 4 mm thick perspex covers, the sensitivity has a
maximum at about 30 keV that is ten times that for 1 MeV photons.
This large sensitivity for low energy photons can in some appli-
cations be annoying. It can be depressed by surrounding the dosi-
meter in its perspex cover with a metal filter» In Table I are listed
the relative sensitivities for various primary radiations with 4 mm
perspex covers and with 4 mm perspex and a 1 mm tin filter.
- 16 -
3. 7, Dependence of the sensitivity on exposure, exposure rate, and
Let us assume that a phosphor sample contains N monoenergetic
electron traps of which n are filled. This sample is irradiated with
the exposure rate R roentgens/sec. The differential equation for the
increase in the number of trapped electrons can be supposed to be
| £ ~ = aR(N-n) - np (10).
Defined by eq. (t), p is the probability that a filled trap is
emptied per unit time. The constant a can be interpreted as the frac-
tion of empty traps filled per unit exposure.
Provided that n = 0 for t = 0 and that the irradiation temperature
and the exposure rate are constant, this equation has the solution
or, if the exposure D = Rt is introduced,
n = N , -i 1 - exp l-aD(i+p/aR) | }• (12)
1 + p/aR ' r \ \ if/ i i i \ i
For large doses (aD»l) and/or long irradiation times
(aDp/aR = p t» l ) n approaches a saturation value that depends on
the exposure rate as well as the irradiation temperature. This sa-
turation value is
l i m i t 1 + p/aR
On the other hand, for small exposures (aD«i) and short
- 17 -
/irradiation times (pt«i) eq.'(12) can be approximated with
NaD (1 + p/aR) = aDN (14).
1 + p/aR
The sensitivity of this ideal luminophor with monoenergetic
traps is independent of exposure rate as well as irradiation tempera-
ture if the dose is small and the irradiation time short.
However, the CaSO.iMn has traps of a broad energy distribution.
This would not have caused any deviation from the behaviour suggested
by the equations above, if the value p = v . exp(uE/kT) had been very
small for all traps at the irradiation temperature. But this condition is
not fulfilled when CaSO t̂Mn is irradiated at or above room temperature.
To study these conditions, the constant a in eq« (10) was first de-
termined. From eq. (12) it follows that at high exposure rates, the
response can be supposed to vary with the dose as
S = constant, i 1 - «xp(-aD) 1- (15)
Dosimeters were irradiated with an exposure rate of 134 R/sec
in a Co gamma irradiation cell. The thermoluminescence signal
after the standard storing was measured. It increases with the expo-
sure according to Figure 5. The experimental points suggest a function
S = constant . j l - exp (-3. 5 x 1 0~ D) >•
where D is the exposure in roentgens. Since p is of the order of magni-
tude 0, 06 hr (Fig» 2) and R = 134 R/sec» the requirements for the
use of the approximation eqe (1 5) are fulfilled and consequently
a = 3.5 x 10~5 R~1.
- 18 -
Figure 6 shows values of the response per unit exposure, S/D,
as a function of the irradiation time for high and low exposure rates.
The solid lines are calculated from eq. (T2), For the high exposure«g , ...
rate, the choice of p is not critical since aR = 3,5x 10 x 134>0
- 19 -
3. 8, Influence of large exposures_qnj;he_sens_itivity
Bräunlich and Scharman E 1 8] found that the sensitivity of ther-
moluminescent LiF increased considerably for a sample that had been
irradiated with a gamma exposure exceeding 500 R, When the LiF sample
was subjected to a heat treatment (700- C for 1 hour) the sensitivity re-
turned to the original value.
To discover whether a similar effect exists for CaSO.sMn a set
of dosimeters were calibrated with a small exposure, irradiated with
Co gamma radiation with exposures up to 70 MR, carefully zeroed,
and re-calibrated. The new values agreed with the originals within the
measuring error» which in this case was about-- 8 %. If present at all,
the effect is cured by the zeroing process, which consisted of heating
at 300 C for a few minutes and at 250 °C for 2 hours. Since no devia-
tion from linearity between signal and exposure other than that implied
by eq. (12) has been detected, it can be concluded that the effect does
not exist for CaSO4:Mn.
temperature
The' irradiation temperature can influence the sensitivity in two
ways. When the temperature changes, the probability that an electron
is released per unit time changes. There is also a possibility that the
probability that an excited electron is trapped changes with the tempe-
rature.
Dosimeters vere irradiated with a standard dose at temperatures
between -20 and +50 C. The signal was measured immediately after
the excitation. The exposure time was short (3 minutes). No change of
the signal with the temperature during the irradiation could be detected^
and the probability that an excited electron is trapped can be assumed
to be temperature independent in this interval.
3^10. Backgroundj>henomena
One of the possible applic?tions of CaSO,sMn in dosimetry is for
measurements of small exposures. It is possible to measure 50 fiR of
1 MeV gamma radiation [ 1] . The factors governing the minimum mea-
- 20 -
surable exposure are the dark current of the photomultiplier, the
emission of incandescent light from the dosimeter when heated for
read-out, and excitation by light and mechanical disturbancies (tri-
bothermoluminescence). The dark current can be reduced by various
means; the most efficient are cooling of the photomultiplier and mo-
dulation of the light signal. The influence of the incandescent light
emission of the dosimeter can be reduced with optical filters. Exci-
tation by light and by mechanical disturbancies seems to give signals
not exceeding the equivalent of 1 mR, but make certain precautions
necessary [ 11.
4. Discussion
The reproducibility of the exposure measurements with CaSO,:Mn
has during the course of this investigation been improved to about i 3 %
for exposures of the order of magnitude t R. The absolute accuracy of an
exposure measurement is limited by the energy and the angular dependanc«
of the sensitivity and is only exceptionally as good as the reproducibility.
Unless exposures less than 1 mR shall be measured, the CaSO.;Mn
dosimeters are very convenient to read out. This 'makes them useful in
many experiments where a wide range of measurable exposures is impor-
tant. Spurnf reported [7] that CaSO.tMn can be used for measurements
of gamma radiation in reactors, since the excitation because of neutron
irradiation is small. For such a use the Kanthal support is not well
suited, however.
The large sensitivity of CaSO,:Mn can be utilized in special appli-
cations. One of these is measurements of small exposuresC i] . Another
is to construct small dosimeters for measurements of exposures in the
usual radiation protection range. There is, for instance, a need for small
finger dosimeters that can be worn without inconvenience.
In such applications as those mentioned it is essential that the irra-
diation time is short or known. Otherwise the shallowness of the traps
complicates the evaluation of the exposure, as has been described above.
- 21 -
For personnel monitoring* the use of CaSO,;Mn is restricted to short
sampling periods of the order of magnitude of one day. On the other
hand the shallowness of the traps can be made use of in emergency do-
simeters* Irradiated at a constant and small exposure rate the thermo-
lumine scene e signal will reach a saturation level after some days. This
signal is about equal to the one that would have been excited if the ex-
posure during 100 hours had "been given momentaneously, This will
normally be an acceptable background for emergency purposes.
- 22 -
References
1. BJÄRNGARD BCaSO.(Mn) thermoluminescen.ee dosimeters for small dosesof gamma radiation.Rev. Sci0 Instr. 33 (1962) 1129
2. WATANABE KProperties of a CaSO^fMn phosphor under vacuum ultravioletexcitation.Phys. Rev0 83 (1951) 785-791
3. BURGER H, LEHMANN J and MAYER UDie Anwendung der Simultandosimetrie bei der intravaginalenRöntgenbestrahlung der Parametrien.Naturwiss. 4 (1954) 209-210
4. PATTERSON D A and FRIEDMAN HMilliroentgen dosimetry with thermoluminescence.J. Opt. Soc, Am. 47 (1957) 1136-1137
5. NOSENKO B M, REVZIN L. S and IASKOLKO VUse of CaSO,?Mn for dosiraetry,Soviet Phys.-Tech. Phys. 1 (1956) 1983-1985 (English transl.)
6. ARHANGEL^KAYA V A, VAYNBERG B I and RAZUMOVA T KThermoluminescent monocrystals of CaSO.-Mn.Opt. i Spektr. 4 (1958) 681-683 (In Russian)
7. SPURNY ZEin The rmolumine szenzdo sim eter.Kernenergie 5 (1962) 611-615
8. PETER HThe rmolumine szenz und Dosimetrie von samariumaktiviertemKalziumsulfat.Atomkernenergie 5 (i960) 453-455
9. MEDLIN W LThermoluminescence in anhydrite,J. Phys. Chem. Solids 18 (1961) 238-252
10. ARCHANGELSKAJA V A, VAJNBERG B I, KODJUKOV V Mand RAZUMOVA T KLiumineszenzdosimeter fiir yStrahlen, (3-Teilchen und Neutronenauf der Grundlage des Phosphors CaSO , . Mn.Kernenergie 4 (1961) 149-152 (German transl.)
1 1. MOORE L EThermolixminescence of sodium sulfate and lead sulfate andmiscellaneous sulfates, carbonates,and oxidesJ. Phys, Chem. 61 (1957) 636-639
- 23 -
12. MEDLIN W L,Decay of phosphorescence from a distribution of trappinglevels .Phys. Rev. 123 (1961) 502-509
13. CONDAS G ATechniques for evaluating the commercial photo cathode.UCRL-6740 (1962)
14. DE VOS J CThe émissivity of tungsten ribbon.Dissertation, Amsterdam 1953
15. MOREHEAD F f ana JJANIELS F °Storage of radiation energy in crystalline lithium fluorideand metamict materials.J. Phys. Chem. 56 (1952) 546-548
16. SCHAYES RPersonal communication.
17. BERONIUS P, FORBERG S, HENRIKSON C-O andSÖREMARK RThe use of iodine-125 as an X-ray source in roentgen diagnosis,Intern. J. Appl. Radiation Isotopes 13 (1962) 253-254
18. BRÄUNLICH P and S CHARM ANN ADosimetrie mit Hilfe der Thermolumineszenz von Lithium-fluorid.Nukleonik 4 (1962) 65-67
- 24 -
Table I
Relative sensitivity of a dosimeter for perpendicularly incident
radiation
radiation
I1 2 527keV1 %l
Cs 662 keV
Co60 1.25 MeV
Roentgen?
25 kV h. v. t.
50 kV h.v. t.
1 00 kV h. v. t.
145 kV h. v. t.
175 kV h. v. t.
190 kVh.v.t .
190 kV h.v.t .
0. 6 mm
T. 35 mm
3.2 mm
0.38 mm
1,04 mm
1, 8 mm
3,3 mm
Al
Al
Al
Cu
Cu
Cu
Cu
Cover
4 mm perspeX 41
9.6
1.00
1.00
5.06
5.85
6.05
4.78
3.06
1.98
1.07
mmmm
0.
0.
0,
0.
0.
0.
0.
0.
0.
perspextin
-
96
96
007
021
11
33
64
78
88
1) h. v. t. = half value thickness
B/E'L
4500 5000 5500Wavelength, A
6000
Fig. 1. Emission, spectrum of CaSO '̂.Mn at about 80 C
after excitation with 10 kR of gamma radiation.
j I T I T
0.3
0.2
0.1 -
0.0 - J I I I 1 I l _ _ J I 1 I I i500 1000 1500
Storing time, minutes
Fig. 2. The decay of the thermoluminescent signal.
Irradiation time 5 minutes, exposure 300mR.
10fo
u
teai?o1 05CL
"5
.2
QO
I | I | i i i i i i i I I i i
i i i i i i 1 i i i i i i t i
10Thickness of layer, mg/cm^
100
Fig. 3. The light emitted per unit area and per mg of
luminophor as a function of the thickness of
the luminophor layer.
0 100 200 300 400
Thickness of perspex, mg/cm2
Fig, 4. Relative signal per exposure unit of gamma radiation
from a Co source. A uncollimated, and B collimated
radiation.
102 103 K)« 10 5Exposure, roentgens
106
Fig. 5. The thermoluminescen.ee signal as a function of the
exposure at the exposure rate 134 R/sec. The circles
show experimental values, the solid line represents
S = constant. J 1 - exp(-aD) i- with a = 3. 5 x 10"5 R~ ,
1.0
10 102 103Irradiation time, minutes
Xfi
Fig, 6. The signal per unit exposure as a function of the expo-
sure time for two different exposure rates. The circles
are experimental values, the solid lines are calculated.
LIST OF PUBLISHED AE-REPORTS
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66. Critical and exponential experiments on 19-rod clusters (R3-fuel) in heavywater. By R. Persson, C-E. Wikdahl and Z. Zadworski. 1962. 34 p. Sw. cr.6:—.
67. On the calibration and accuracy of the Guinier camera for Ihe deter-mination of interplanar spacings. By M. Mölfer. 1962. 21 p. Sw. cr. 6:—.
68. Quantitative determination of pole figures with a texture goniometer bythe reflection method. By M. Möller. 1962. 16 p. Sw. cr. 6:—.
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70. An experimental study of pressure gradients for flow of boiling water ina vertical round duct, Part I I . By K.M. Becker, G. Hernborg and M. Bode.1962. 32 p. Sw. cr. 6:—.
71. The space-, time- and energy-distribulion of neutrons from a pulsedplane source. By A. Claesson. 1962. 16 p. Sw. cr. 6:—.
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74. Burnout conditions for flow of boiling water in vertical rod clusters.By Kurt M. Becker. 1962. 44 p. Sw. cr. 6:—.
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Half-life measurements of »He, « N , " O , mf, »Al, "Sem and '"Ag. By J.Konijn and S. Malmskog. 1962. 34 p. Sw. cr. 6:—.
Progress report for period ending December 1961. Department for ReactorPhysics. 1962. 53 p. Sw. cr. 6:—.
Investigation of the 800 fceV peak in the gamma spectrum of SwedishLaplanders. By I. ö . Andersson, I. Nilsson and K. Eckerstig. 1962. 8 p.Sw. cr. 6:—.
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Swedish studies on irradiation effects in structural materials. By M.Grounes and H. P. Myers. 1962. 11 p. Sw. cr. 6:—.
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Flame photometric determination of lithium contents down to 10-3 ppmin wafer samples. By G. Jönsson. 1963. 9 p. Sw. cr. 8:—.
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Förteckning över publicerade AES-rapporter
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Additional copies available at the library of AB Atomenergi, Sludsvik, Nykö-ping, Sweden. Transport microcards of the reports are obtainable throughthe International Documentation Center, Tumba, Sweden.
EOS-tryckerierna, Stockholm 1963