ORNL-1771 - Oak Ridge National Laboratory
ORNL-1771 - Oak Ridge National Laboratory
ORNL-1771 - Oak Ridge National Laboratory
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11. SHIELDING ANALYSIS<br />
J. E. Faulkner<br />
H. E. Hungerford<br />
Theoretical analyses have been made so that an<br />
understanding of the air and ground scattering<br />
measurements at the Tower Shielding Facility could<br />
be obtained and the attenuation in the side wall of<br />
an aircraft crew shield could be determined. In<br />
connection with the air and ground scattering analy-<br />
ses, special attention was given to the calculation<br />
of the reduction of air scattering due to ground<br />
interruption and to the effects of multiple scattering.<br />
The gamma-ray slant penetration has been calcu-<br />
lated for the side wall of an aircraft crew shield,<br />
and the variation of radiation intensity throughout<br />
the crew volume has been briefly explored.<br />
SLANT PENETRATION OF COMPOSITE<br />
SLAB SHIELDS BY GAMMA RAYS<br />
C. D. Zerby<br />
The total radiation dose in the crew compartment<br />
of an airplane is partially dependent on the gamma-<br />
ray flux penetrating the compartment shield. To<br />
obtain a fundamental, but practical, knowledge of<br />
the gamma-ray penetrations, the problem has been<br />
treated theoretically by using stochastic, or Monte<br />
Carlo methods.<br />
The problem was programed for solution on the<br />
ORACLE and was arranged for investigating the<br />
effects of the variations of all the parameters in-<br />
volved. The shield was taken as a composite slab<br />
of two materials comprising a thick layer of Compton<br />
scattering material' followed by a thin layer of<br />
lead. In each of many cases the initial incident<br />
photons were taken as monoenergetic and incident<br />
on the slab at a particular angle with the normal to<br />
the slab. The stochastic process used the exacf<br />
physical analog of the probability laws known to<br />
govern the life of a photon.<br />
'In the range of energy considered, the Compton<br />
scatterer has approximately the same physical charoc-<br />
terlstics relative to a photon passing through it as does<br />
coricrete or polyethylene (CH2).<br />
E. P. Blizard<br />
F. H. Murray<br />
C. D. Zerby<br />
Physics Division<br />
H. E. Stern<br />
Consolidated Vu1 tee Aircraft Corporation<br />
The parameters and their variations that have<br />
been investigated to date are listed below:<br />
Thickness of Compton<br />
Thickness of lead, in.<br />
in. 3, 9, 15<br />
bo, 3/10, Y2<br />
3<br />
Initio1 photon energy, mc2 units 2, 6<br />
Initial angle of incidence, deg<br />
0, 30, 60<br />
All combinations of these parameters were investi-<br />
gated.<br />
The following solution of a typical problem indi-<br />
cates part of the information obtained:<br />
Initial Conditions<br />
Results<br />
Thickness of Compton scatterer 3 in.<br />
Thickness of lead<br />
Initial photon energy<br />
>,o in.<br />
6 mc 2<br />
Initial angle of incidence 60 deg<br />
Fraction of initial energy<br />
1. reflected 0.0234<br />
2. absorbed in the Compton scatterer owing<br />
to scattering collisions<br />
0.318<br />
3. absorbed in lead owing to scattering<br />
collisions<br />
0.0568<br />
4. absorbed In lead awing to absorption<br />
cat I is ions<br />
0.0515<br />
5. penetrating shield 0.550<br />
6. penetrating shield without being<br />
degraded in energy<br />
0.435<br />
Energy build-up factor 1.265<br />
The energy spectrum for the reflected photons<br />
was also obtained in this typical problem. The<br />
spectra for the photons penetrating the shield were<br />
obtained in the angle intervals 0 to 15, 15 to 30,<br />
30 to 45, 45 to 60, and 60 to 90 deg. These spectra<br />
will be available in a forthcoming report.<br />
_____ ...... .............<br />
2The electron density of the Compton scatterer was<br />
taken as the same as that for polyethylene.<br />
3Multiply mc 2 units by 0.5108 to obtain MeV.<br />
157