Magnetic Evolution of NOAA Active Region 8210

Details Magnetic Evolution of NOAA Active Region 8210 Magnetic Evolution of NOAA Active Region 8210

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.5509l&link_type=abstract

American Astronomical Society, 194th AAS Meeting, #55.09; Bulletin of the American Astronomical Society, Vol. 31, p.911

Astronomy and Astrophysics

Astronomy

Scientific paper

NOAA Active Region 8210 produced a number of large flares in April - May 1998. The Imaging Vector Magnetograph at the Mees Solar Observatory, Haleakala made several day-long movies of this region. Large-scale helicity in the active region magnetic structure was complicated by continuing flux emergence. Much of the new flux appeared to emerge from directly beneath the main sunspot cluster. Rapid, directed flow of the new flux carried much of it far from the spots, to along locations close the the sheared neutral line. We will report on quantitative measures of the magentic properties of AR8210. This work was supported by NASA grant NAG5-4914.

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