The Relationship Between Solar Flare And Magnetic Field In AR 5229
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Abstract
Active region 5229 was studied during 13-18 November 1988 using Hδ filergrams and Fel 5324 Viedomagenetograms acquired at Huairou Solar Observing Station of Beijing Astronomical Observatory. Newly emerging flux, magnetic shear and magnetic flux cancellatoin was examined according to evolution of magnetic fields1. The preliminary results of the analysis were summarized in this paper.
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