Derivation of relativistic solar cosmic-ray spectra from the Baksan EAS array data

被引：1
|
作者：
Z. M. Karpova
Yu. V. Balabin
E. V. Vashenyuk
S. N. Karpov
机构：
[1] Russian Academy of Sciences,Institute for Nuclear Research
[2] Baksan Neutrino Observatory,Polar Geophysical Institute, Kola Research Center
[3] Russian Academy of Sciences,undefined
来源：
Bulletin of the Russian Academy of Sciences: Physics | 2007年 / 71卷 / 7期
关键词：
Neutron Monitor; Solar Proton; Solar Proton Event; Ground Level Enhancement; Bismuth Molybdate;
D O I：
10.3103/S1062873807070131
中图分类号：
学科分类号：
摘要：
Fifteen increases in the intensity of solar cosmic rays (SCRs) from 30 investigated ground level enhancement (GLE) events have detected by Baksan EAS arrays in the period from 1981 until now. These data make it possible to refine the high-energy part of the SCR spectra calculated previously according to the data of the world-wide network of neutron monitors. A method for obtaining SCR spectra and calculating the specific yield functions for the Andyrchi, Carpet, and BMD Baksan arrays is briefly described. The SCR spectra for different instants in the GLE event of January 20, 2005 are presented.
引用
收藏
页码：938 / 941
页数：3
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