Computer Science
Scientific paper
Mar 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40..539s&link_type=abstract
(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Samarkand, Uzbek SSR, Oct. 29-31, 1975.) Akademiia Nauk SSSR, Izvest
Computer Science
Cosmic Rays, Gamma Rays, Mars Atmosphere, Mars Surface, Mars 5 Spacecraft, Nuclear Interactions, Chemical Composition, Computerized Simulation, Least Squares Method, Satellite-Borne Instruments, Spectrum Analysis, Structural Properties (Geology)
Scientific paper
The spectrum of gamma radiation resulting from the interaction of gamma rays with the atmosphere and surface of Mars was investigated, using data transmitted by the interplanetary probe Mars-5. The components due to uranium, thorium, and calcium were separated on the basis of data from accelerator modelization studies. Estimates of the contribution due to the atmosphere were made from two sets of data: results of accelerator studies of a model Mars atmosphere, consisting of 40% argon and 60% carbon dioxide, and measurements obtained by high altitude balloons, corrected for differences between the thickness and assumed composition of the atmospheres of Mars and the earth. The component of the gamma spectrum due to interaction of cosmic rays with the surface of Mars indicates the presence of basalt-like materials.
Borodin A. M.
Khariukova V. P.
Moskaleva L. P.
Surkov Iu. A.
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