Radial distribution of galactic cosmic rays at solar maximum

被引:0
作者
Morales-Olivares, O. G. [1 ]
Caballero-Lopez, R. A. [1 ]
机构
[1] Univ Nacl Autonoma Mexico, Inst Geofis, Mexico City 4510, DF, Mexico
关键词
Cosmic ray modulation; Termination shock; Gradient; Spectrum; WIND TERMINATION SHOCK; OUTER HELIOSPHERE; MAGNETIC-FIELDS; MODULATION; HELIOSHEATH; GRADIENT; PARTICLE; VOYAGER;
D O I
10.1016/j.asr.2012.02.032
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
In this paper we analyze the spatial distribution of galactic cosmic rays during periods of maximum solar activity of the cycles 21, 22 and 23. We have used a two dimensional model to solve the cosmic ray transport equation. This model includes all relevant physical processes: diffusion, convection, drift and shock effects on cosmic ray propagation inside the heliosphere. We focused on the study of the radial distribution of galactic cosmic rays, and compare our results with the spacecraft observations for two energies (175 MeV H and 265 MeV/n He). Although the radial intensities of galactic cosmic rays can be explained qualitatively with all three local interstellar spectra (LISs) used in this work, we applied a reduced chi-squared analysis to investigate the best LIS that could fit the data. (C) 2012 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:1653 / 1659
页数:7
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