Magnetohydrodynamic turbulence and implications for solar coronal heating

被引：82
|
作者：
Hendrix, DL
VanHoven, G
机构：
[1] Department of Physics and Astronomy, University of California, Irvine
来源：
ASTROPHYSICAL JOURNAL | 1996年 / 467卷 / 02期
关键词：
methods; numerical; MHD; Sun; corona; turbulence;
D O I：
10.1086/177663
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
During the course of an investigation of coronal heating, we have performed three-dimensional numerical simulations using the model proposed by Parker (1972, 1994), and have studied its ultimate dynamic magnetic-reconnection dissipation mechanism. Our findings suggest that magnetohydrodynamic turbulence plays an important role in the form of the energy spectrum and, hence, in the ohmic heating.
引用
收藏
页码：887 / 893
页数：7
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