ION AND RELATIVISTIC ELECTRON-TRANSPORT IN SOLAR-FLARES

被引：15
作者：
RAMATY, R
MILLER, JA
HUA, XM
LINGENFELTER, RE
机构：
[1] UNIV MARYLAND,DEPT PHYS & ASTRON,COLLEGE PK,MD 20742
[2] UNIV CALIF SAN DIEGO,CTR ASTROPHYS & SPACE SCI,LA JOLLA,CA 92093
来源：
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 1990年 / 73卷 / 02期
关键词：
Gamma rays: general; Hydromagnetics; Particle acceleration; Sun: flares; Sun: particle emission;
D O I：
10.1086/191452
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We review recent models for ion and relativistic electron transport in solar flare magnetic loops. We discuss the depth distributions of gamma-ray production, the attenuation of gamma-ray lines, the time dependences of the various emissions, and the angular distribution of the bremsstrahlung.
引用
收藏
页码：199 / 207
页数：9
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