The ionization equilibrium in the solar corona for the electron power distribution

被引：25

作者：

Dzifcakova, E ^{[1
]}

机构：

[1] Comenius Univ, Fac Math & Phys, Dept Astron & Astrophys, Bratislava 84215, Slovakia

来源：

SOLAR PHYSICS | 1998年 / 178卷 / 02期

关键词：

D O I：

10.1023/A:1005087731100

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The influence of an electron non-Maxwellian distribution (power distribution) on the ionization equilibrium of Fe in the solar corona is demonstrated. The results can be used for specific applications in the solar corona, especially in the description of the ionization state of plasma during the impulsive phase of solar flares, where deviations from the Maxwellian distribution may be significant.

引用

页码：317 / 339

页数：23

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