FAST WAVE EVANESCENCE IN SOLAR CORONA

被引：33

作者：

HOLLWEG, JV

机构：

来源：

GEOPHYSICAL RESEARCH LETTERS | 1978年 / 5卷 / 08期

关键词：

D O I：

10.1029/GL005i008p00731

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

Using a horizontally stratified model of the solar atmosphere, we argue that appreciable fast wave fluxes of solar origin may not be able to propagate into the solar wind. Fast waves may thus not be a significant source of extended heating and acceleration of the solar wind. This conclusion could be altered by nonlinearity and/or by complex structure of the solar atmosphere, however. Copyright 1978 by the American Geophysical Union.

引用

页码：731 / 733

页数：3

共 21 条

[1] COLLISIONLESS HEATING OF SOLAR-WIND PLASMA .I. THEORY OF HEATING OF COLLISIONLESS PLASMA BY HYDROMAGNETIC WAVES [J].