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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