Radial and latitudinal gradients of galactic cosmic rays in the heliosphere at solar maximum

被引:8
|
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; Transport equation; Gradient; OUTER HELIOSPHERE; MODULATION; WIND;
D O I
10.1016/j.asr.2010.06.033
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Our understanding of galactic cosmic ray (GCR) modulation has advanced greatly in the last three decades. However, we still need an appropriate knowledge of the GCR intensity gradient. Numerical simulations of the transport particle equation allow interpretation of cosmic ray intensities in the heliosphere. We use the numerical solution of the GCR transport equation during solar maximum epoch to compute the radial and latitudinal gradients. Our analysis indicates that adiabatic energy loss plays an important role in the radial distribution of GCR in the inner heliosphere, while in the outer region the diffusion and convection are the relevant processes. The latitudinal gradient is small. (C) 2010 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:1313 / 1317
页数:5
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