AbstractCoronal magnetic field and nonthermal electrons are very important parameters for understanding of the global heliophysical processes. A flare on November 1, 2004 is selected for self-consistent calculations of coronal magnetic field parallel and perpendicular to the line-of-sight, and density of nonthermal electrons from Nobeyama observations. Both of the diagnosis methods and results are discussed in this paper.
Diagnosis of coronal magnetic field and nonthermal electrons from Nobeyama observations of a simple flare
Advances in Space Research ; 41 , 8 ; 1191-1194
2007-06-12
4 pages
Article (Journal)
Electronic Resource
English
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