Cosmic rays in the solar system

被引：0

作者：

O'Brien, Keran ^{[1
]}

机构：

[1] No Arizona Univ, Dept Phys & Astron, Flagstaff, AZ 86011 USA

来源：

NATURAL RADIATION ENVIRONMENT | 2008年 / 1034卷

关键词：

cosmic rays; shock acceleration; heliosphere; transport theory;

D O I：

暂无

中图分类号：

Q6 [生物物理学];

学科分类号：

071011 ;

摘要：

Calculations of cosmic-ray propagation through the heliosphere, in the terrestrial atmosphere using a combination of a modified version of the adjoint Monte Carlo code, ATROPOS, and a suitably modified version of the deterministic transport code, PLOTINUS. ATROPOS solves the Parker heliospheric transport code in one and two dimensions in a 3-dimensional heliosphere and provides cosmic-ray spectra to be used by PLOTINUS to determine the radiation effects of interest. Other cosmic-ray properties, such as the deceleration time (related to the so-called deceleration potential) and the angular distribution of cosmic rays at earth orbit will also be described.

引用

页码：86 / 92

页数：7

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