Coronal heating and the solar wind acceleration

被引：0

作者：

Hirayama, T ^{[1
]}

机构：

[1] Meisei Univ, Tokyo 1988655, Japan

来源：

RECENT INSIGHTS INTO THE PHYSICS OF THE SUN AND HELIOSPHERE: HIGHLIGHTS FROM SOHO AND OTHER SPACE MISSIONS | 2001年 / 203期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We propose a coronal heating theory based on the magnetic twisting, which inevitably produces charge imbalance. The resulting electric field creates supra-thermal electron beams. Beams are then thermalized by classical collisions. The dissipation rate is enough to heat the corona and to accelerate the solar wind.

引用

页码：495 / 497

页数：3

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