Numerical Validation and Comparison of Three Solar Wind Heating Methods by the SIP-CESE MHD Model
Numerical Validation and Comparison of Three Solar Wind Heating Methods by the SIP-CESE MHD Model
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SIP-CESE MHD 模型对三种太阳能风加热方法的数值验证和比较
DOI：
10.1088/0256-307x/28/3/039601
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发表时间：
2011-02
影响因子：
3.5
通讯作者：
中科院分区：
文献类型：
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作者：
We conduct simulations using the three-dimensional (3D) solar-interplanetary conservation element/solution element (SIP-CESE) magnetohydrodynamic (MHD) model and magnetogram data from a Carrington rotation (CR) 1897 to compare the three commonly used heating methods, i.e. the Wentzel-Kramers-Brillouin (WKB) Alfven wave heating method, the turbulence heating method and the volumetric heating method. Our results show that all three heating models can basically reproduce the bimodal structure of the solar wind observed near the solar minimum. The results also demonstrate that the major acceleration interval terminates about 4R(S) for the turbulence heating method and 10R(S) for both the WKB Alfven wave heating method and the volumetric heating method. The turbulence heating and the volumetric heating methods can capture the observed changing trends by the WIND satellite, while the WKB Alfven wave heating method does not.
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DOI：
10.1086/185635
发表时间：
1990-01
期刊：
The Astrophysical Journal
影响因子：
--
作者：
D. Hassler;G. Rottman;E. C. Shoub;T. Holzer
通讯作者：
D. Hassler;G. Rottman;E. C. Shoub;T. Holzer
影响因子：
4.9
作者：
Sheeley, NR;Wang, YM;Biesecker, DA
通讯作者：
Biesecker, DA
DOI：
10.1086/511154
发表时间：
2007-01
期刊：
The Astrophysical Journal Letters
影响因子：
--
作者：
O. Cohen;I. Sokolov;I. Roussev;C. Arge;W. Manchester;T. Gombosi;R. Frazin;H. Park;M. Butala;F. Kamalabadi;M. Velli
通讯作者：
O. Cohen;I. Sokolov;I. Roussev;C. Arge;W. Manchester;T. Gombosi;R. Frazin;H. Park;M. Butala;F. Kamalabadi;M. Velli
DOI：
10.1086/166015
发表时间：
1988-02
期刊：
The Astrophysical Journal
影响因子：
--
作者：
G. Withbroe
通讯作者：
G. Withbroe
DOI：
10.1088/0004-637x/710/1/676
发表时间：
2009-12
期刊：
The Astrophysical Journal
影响因子：
--
作者：
S. Cranmer
通讯作者：
S. Cranmer