On the possibility of spontaneous generation of turbulent Alfven waves in solar plasma by heavy ions

被引：14

作者：

Wu, C. S. ^{[1
,2
,4
]}

Zhao, G. Q. ^{[1
,3
]}

Chen, L. ^{[1
]}

Wu, D. J. ^{[1
]}

机构：

[1] Chinese Acad Sci, Purple Mt Observ, Nanjing, Jiangsu, Peoples R China

[2] Natl Cent Univ, Inst Space Sci, Zhongli, Taiwan

[3] Univ Chinese Acad Sci, Beijing, Peoples R China

[4] Univ Maryland, Inst Phys Sci & Technol, College Pk, MD 20742 USA

来源：

PHYSICS OF PLASMAS | 2013年 / 20卷 / 08期

关键词：

DISSIPATION; CORONA;

D O I：

10.1063/1.4817265

中图分类号：

O35 [流体力学]; O53 [等离子体物理学];

学科分类号：

070204 ; 080103 ; 080704 ;

摘要：

In this paper, we discuss spontaneous generation of Alfven waves. The discussion is motivated by the study of the solar transition region. We show that the heavy ions in this region can play critical roles. A quasilinear theory is derived. On the basis of this theory, we can discuss the saturation level of the wave spectral energy associated with each species of ions. Several essential issues relevant to the transition region are also discussed. (C) 2013 AIP Publishing LLC.

引用

页数：7

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