GLOBAL ALFVEN WAVES IN SOLAR PHYSICS - CORONAL HEATING

被引：0

作者：

DEAZEVEDO, CA ^{[1
]}

DEASSIS, AS ^{[1
]}

机构：

[1] UNIV ESTADO RIO DE JANEIRO,BR-20550 RIO DE JANEIRO,BRAZIL

来源：

REVISTA MEXICANA DE ASTRONOMIA Y ASTROFISICA | 1990年 / 21卷 / SI期

关键词：

HYDROMAGNETICS; SUN-CORONA;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

It has been shown that the Discrete Alfven wave can power at least 20% of the required coronal energy flux density congruent-to 10(-3) erg cm-3 s-1. Discrete Alfven waves are a new class of Alfven waves which can be described by the model with the inclusion of finite ion cyclotron frequency (omega/omega-ci not-equal-to theta) and the equilibrium plasma current effects as shown by Appert, Vaclavik and Villar 1984.

引用

页码：545 / 548

页数：4

共 10 条

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