ELEMENTARY FLARE BURSTS EXPLAINED BY EXPLOSIVE COALESCENCE

被引：14

作者：

DEJAGER, C ^{[1
]}

SAKAI, J ^{[1
]}

机构：

[1] TOYAMA UNIV,DEPT APPL MATH & PHYS,TOYAMA 930,JAPAN

来源：

SOLAR PHYSICS | 1991年 / 133卷 / 02期

关键词：

D O I：

10.1007/BF00149897

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The observed burst durations of Elementary Flare Bursts (5 - 25 s), as well as the related other flare characteristics, such as the temperature (30-50 MK), the electron density (log ne = 10 to 11) and the magnetic field strengths (100 G to 200 G) can be explained quantitatively by the mechanism of explosive coalescence.

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收藏

页码：395 / 398

页数：4

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