Origin of the high energy proton component below the geomagnetic cutoff in near earth orbit

被引:29
作者
Derome, L
Buénerd, M
Barrau, A
Bouchet, A
Menchaca-Rocha, A
Thuillier, T
机构
[1] Inst Nucl Sci, IN2P3, F-38026 Grenoble, France
[2] IFUNAM, Inst Fis, Mexico City, DF, Mexico
关键词
D O I
10.1016/S0370-2693(00)00914-X
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The high flux proton component observed by AMS below the geomagnetic cutoff can be well accounted for by assuming these particles to be secondaries originating from the interaction of cosmic ray protons with the atmosphere. Simulation results are reported. (C) 2000 Published by Elsevier Science B.V.
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页码:1 / 8
页数:8
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