The Grad-Shafranov reconstruction in twenty years: 1996-2016

被引:55
|
作者
Hu Qiang [1 ,2 ]
机构
[1] Univ Alabama Huntsville, Dept Space Sci, Huntsville, AL 35805 USA
[2] Univ Alabama Huntsville, CSPAR, Huntsville, AL 35805 USA
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
Grad-Shafranov equation; Magnetohydrodynamics; Magnetic clouds; Magnetic flux ropes; Magnetopause; Current sheets; Flux transfer events; Plasmoids; Solar flare; Coronal mass ejections; CORONAL MASS EJECTIONS; MAGNETIC-FLUX ROPES; 2-DIMENSIONAL COHERENT STRUCTURES; IN-SITU OBSERVATIONS; SOLAR-WIND; MAGNETOPAUSE STRUCTURES; MHD RECONSTRUCTION; SPATIAL STRUCTURE; INTERPLANETARY; RECONNECTION;
D O I
10.1007/s11430-017-9067-2
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We review and summarize the applications of the Grad-Shafranov (GS) reconstruction technique to space plasma structures in the Earth's magnetosphere and in the interplanetary space. We organize our presentations following the branches of the "academic family tree" rooted on Prof. Bengt U. O. Sonnerup, the inventor of the GS method. Special attentions are paid to validations of the GS reconstruction results via (1) the direct validation by co-spatial in-situ measurements among multiple spacecraft, and (2) indirect validation by implications and interpretations of the physical connection between the structures reconstructed and other related processes. For the latter, the inter-comparison and interconnection between the large-scale magnetic flux ropes (i.e., Magnetic Clouds) in the solar wind and their solar source properties are presented. In addition, we also summarize various GS-type (or -like) reconstruction and an extension of the GS technique to toroidal geometry. In particular, we point to a possible advancement with added complexity of "helical symmetry" and mixed helicity, in the hope of stimulating interest in future development. We close by offering some thoughts on appreciating the scientific merit of GS reconstruction in general.
引用
收藏
页码:1466 / 1494
页数:29
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