Structure and Evolution of Magnetic Fields Leading to Solar Flares

Details Structure and Evolution of Magnetic Fields Leading to Solar Flares Structure and Evolution of Magnetic Fields Leading to Solar Flares

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..369..449w&link_type=abstract

New Solar Physics with Solar-B Mission ASP Conference Series, Vol. 369, proceedings of the conference held 8-11 November, 2005 a

Physics

3

Scientific paper

In this paper, I review the observations of preflare magnetic conditions. The following topics will be discussed: (1) Static non-potential magnetic topology before flares, such as high magnetic gradient, strong magnetic shear and large twist and electric current. (2) Dynamic pre-flare conditions such as new flux emergence, helicity injection and shear/converging flows. (3) The evolution of these magnetic structures leading to and following flares. Unprecedented vector magnetograms from Solar-B, with high resolution, cadence, stability, will certainly make breakthroughs in this research area.

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