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Testing a solar coronal magnetic field extrapolation code with the Titov-Demoulin magnetic flux rope
[期刊论文] 作者:Chao-Wei Jiang,Xue-Shang Feng,
来源:天文和天体物理学研究:英文版 年份:2016
In the solar corona, the magnetic flux rope is believed to be a fundamental structure that accounts for magnetic free energy storage and solar eruptions. Up to...
[期刊论文] 作者:Chao-Wei Jiang,Xue-Shang Feng,,
来源:天文和天体物理学研究:英文版 年份:2017
With SDO observations and a data-constrained magnetohydrodynamics(MHD)model,we identify a confined multi-ribbon flare that occurred on 2010 October 25 in solar...
[期刊论文] 作者:Wen-Bin Song Xue-Shang Feng Fa,
来源:天文和天体物理学研究:英文版 年份:2010
在太阳的色球层的温度曲线很长时间难倒了天文学家。指 supergranular 房间的结构,我们建议一个引入的加热模型。它主要包括下列三步。(1 ) 一个小规模的发电机在 supergranul...
[期刊论文] 作者:Wen-Bin Song,Xue-Shang Feng,Fa,
来源:天文和天体物理学研究 年份:2004
The temperature curve in the solar chromosphere has puzzled astronomers for a long time.Referring to the structure of supergranular cells,we propose an in ducti...
Identification of slow magnetosonic wave trains and their evolution in 3D compressible turbulence si
[会议论文] 作者:Lei Zhang,Li-Ping Yang,Jian-Sen He,Chuan-Yi Tu,Ling-hua Wang,Eckart Marsch,Xue-Shang Feng,
来源:2014年中国地球科学联合学术年会 年份:2014
In solar wind,slow mode magnetosonic waves are scarce to be identified,but their dissipation plays one of key roles in heating the solar wind,and the wave mode contributes essentially to the solar win...
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