On positron radiation belt in the Earth's magnetosphere

被引:18
|
作者
Gusev, AA [1 ]
Jayanthi, UB
Martin, IM
Pugacheva, GI
Spjeldik, WN
机构
[1] Univ Estadual Campinas, Inst Fis, DRCC, BR-13083970 Campinas, SP, Brazil
[2] Inst Nacl Pesquisas Espaciais, BR-12201 Sao Jose Dos Campos, SP, Brazil
[3] Weber State Univ, Dept Phys, Ogden, UT 84408 USA
关键词
D O I
10.1590/S0103-97332000000300017
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The ratio of positron/electron fluxes originated in nuclear spallation reactions in the Earth's magnetosphere is considered. It is supposed that positrons as well as electrons are produced in the decay of charged pions (pi(+/-) --> mu(+/-) --> e(+/-)) born in nuclear collisions of trapped relativistic inner zone protons with the residual atmosphere. These positrons and electrons are captured in the magnetosphere and create positron and electron radiation belts of nuclear origin. The positron/electron trapped magnetospheric fluxes formed with this mechanism are simulated and the resulting computed e(+)/e(-) flux ratio approximate to 4 appears in agreement with the recent observations. This ratio is significantly different from the ratio approximate to 1 obtained from the primary cosmic ray source through the same mechanism.
引用
收藏
页码:590 / 593
页数:4
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