Propagation model of high-energy solar cosmic rays in interplanetary space and Green function
Huang YN(黄永年) ; Wang ZD(王志丹) ; Wang YL(王永利)
刊名Science in China Series a-Mathematics Physics Astronomy
1998
卷号41期号:11页码:1197-1205
关键词solar cosmic ray Green function coronal particle source protons
ISSN号1006-9283
通讯作者北京8701信箱
英文摘要Based on main observational characteristics of solar flare particle transport in the coronal, a mathematical description of coronal transport is proposed. A model is presented for solar cosmic-ray propagation in solar-terrestrial space of infinite, homogeneous orthotropic medium. A Green function to the propagation equation with source is found. The integral solution to the propagation equation with the source, as well as the analytical solution to the equation for a pulse point source, is obtained by using the Green function in the medium.
学科主题空间物理
收录类别SCI
原文出处://000076532900010
语种英语
内容类型期刊论文
源URL[http://ir.cssar.ac.cn/handle/122/1001]  
专题国家空间科学中心_空间科学部
推荐引用方式
GB/T 7714
Huang YN,Wang ZD,Wang YL. Propagation model of high-energy solar cosmic rays in interplanetary space and Green function[J]. Science in China Series a-Mathematics Physics Astronomy,1998,41(11):1197-1205.
APA 黄永年,王志丹,&王永利.(1998).Propagation model of high-energy solar cosmic rays in interplanetary space and Green function.Science in China Series a-Mathematics Physics Astronomy,41(11),1197-1205.
MLA 黄永年,et al."Propagation model of high-energy solar cosmic rays in interplanetary space and Green function".Science in China Series a-Mathematics Physics Astronomy 41.11(1998):1197-1205.
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