SYNTHETIC SOLAR CORONAL HEATING ON CURRENT SHEETS

被引：14
作者：
Wang, Xiao-Gang [1 ]
Ren, Li-Wen [1 ,2 ]
Wang, Jia-Qi [1 ,2 ]
Xiao, Chi-Jie [1 ]
机构：
[1] Peking Univ, Sch Phys, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China
[2] Dalian Univ Technol, Sch Phys & Optoelect Technol, Lab Mat Modificat Laser Ion & Elect Beams, Dalian 116024, Peoples R China
来源：
ASTROPHYSICAL JOURNAL | 2009年 / 694卷 / 02期
关键词：
MHD; plasmas; Sun: corona; Sun: magnetic fields; Sun:; X-rays; gamma rays; waves; KINETIC ALFVEN WAVES; RESONANT ABSORPTION; MAGNETIC-FIELDS; POWER SPECTRUM; MODEL; RECONNECTION; TURBULENCE; DISSIPATION; DYNAMICS; EVOLUTION;
D O I：
10.1088/0004-637X/694/2/1595
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Synthetic heating of solar coronal loops combining Joule and wave-heating mechanisms on current sheets is proposed. The formation of singular current structures such as current sheets can be caused not only by magnetic reconnection and footpoint convection of coronal loops, but also Alfven resonance induced by shear flows. On the other hand, with the two-fluid effect, the kinetic Alfven wave can also be excited on such current structures. Therefore, a synthetic energy dispassion process of both collisional and wave-heating mechanisms on the current structures may lead to a better understanding of the coronal-heating problem.
引用
收藏
页码：1595 / 1601
页数：7
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