Investigation of primary cosmic rays at the Moon’s surface

被引：0
|
作者：
N. N. Kalmykov
A. A. Konstantinov
R. A. Muhamedshin
D. M. Podorozhniy
L. G. Sveshnikova
A. N. Turundaevskiy
L. G. Tkachev
A. P. Chubenko
O. A. Vasilyev
机构：
[1] Moscow State University,Skobeltsyn Institute of Nuclear Physics
[2] Russian Academy of Sciences,Institute for Nuclear Research
[3] Joint Institute for Nuclear Research,Lebedev Institute of Physics
[4] Russian Academy of Sciences,undefined
来源：
Physics of Atomic Nuclei | 2013年 / 76卷
关键词：
Atomic Nucleus; Lateral Distribution; Radio Emission; Lunar Regolith; Iron Nucleus;
D O I：
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中图分类号：
学科分类号：
摘要：
The possibility of experimentally studying primary cosmic rays at the Moon’s surface is considered. A mathematical simulations of showers initiated in the lunar regolith by high-energy particles of primary cosmic rays is performed. It is shown that such particles can in principle be recorded by simultaneously detecting three components of backscattered radiation (secondary neutrons, gamma rays, and radio emission).
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页码：80 / 87
页数：7
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