EVOLUTIONARY AND FLARE-ASSOCIATED MAGNETIC SHEAR VARIATIONS OBSERVED IN A COMPLEX, FLARE-PRODUCTIVE ACTIVE-REGION

Citation
A. Ambastha et al., EVOLUTIONARY AND FLARE-ASSOCIATED MAGNETIC SHEAR VARIATIONS OBSERVED IN A COMPLEX, FLARE-PRODUCTIVE ACTIVE-REGION, Solar physics, 148(2), 1993, pp. 277-299
Citations number
26
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ISSN journal
00380938
Volume
148
Issue
2
Year of publication
1993
Pages
277 - 299
Database
ISI
SICI code
0038-0938(1993)148:2<277:EAFMSV>2.0.ZU;2-P
Abstract
Evolution of nonpotential structures in a complex, flare-productive ac tive region NOAA AR 6555 has been studied during the period March 23-2 6, 1991, using a quantitative description of the degree of magnetic sh ear at both local and regional scares. Distinct shear evolution in fou r subareas of AR 6555 is inferred from daily variation of their shear indices. Subareas which showed significant evolution in their overall magnetic structure are found to be most active. Ha Bare ribbons mostly formed bordering, and not within, areas of large shear and expanded o ver areas of lower shear. Magnetic shear changes are also detected dur ing several flares, including a major X4.7/4B hare. Out of the 14 even ts for which temporally contiguous magnetograms were available, a decr ease, or dip, in area-averaged shear index around flare onset time fol lowed by an increase was observed in eight cases. There were two event s with increase, three events with continuous decrease, and one event with no change in the shear index during the flare.