THE MAGNETIC EVOLUTION OF THE ACTIVITY COMPLEX AR-7260 - A ROADMAP

被引:29
作者
LEKA, KD
VANDRIELGESZTELYI, L
NITTA, N
CANFIELD, RC
MICKEY, DL
SAKURAI, T
ICHIMOTO, K
机构
[1] UNIV TOKYO,INST ASTRON,KISO OBSERV,MITAKE,NAGANO,JAPAN
[2] LOCKHEED PALO ALTO RES LABS,PALO ALTO,CA 94304
[3] APPL RES CORP,LANDOVER,MD 20785
[4] NATL ASTRON OBSERV,MITAKA,TOKYO 181,JAPAN
关键词
D O I
10.1007/BF00680598
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The active region NOAA 7260 rotated onto the north solar hemisphere as a mature bipole: a dominant negative-polarity sunspot with trailing plage and scattered small spots in attendance. The dominant p spot itself had strong magnetic fields and covered almost 400 x 10(-6) of a solar hemisphere. For a period of seven days beginning 14 August, 1992 this active region displayed rapid and drastic evolution: no fewer than 50 magnetic bipoles emerged in the area trailing the large sunspot, increasing the region's magnetic flux by more than 10(22) MX. This new group of sunspots formed a complex beta gamma delta configuration with two delta spots and a high degree of magnetic shear. This region was very well observed by Yohkoh and various ground-based instruments. It presented opportunities to study new emerging flux, flares, and also the decay of a large sunspot. For the benefit of later studies we present a description of the global characteristics of this active region, a detailed 'roadmap' of its evolution during disk passage including the development of the two delta regions. We compare proper motion trends and Baring activity to observations of other delta-spots reported in the Literature. We also comment on the observed outflow of magnetic elements from the decaying p spot.
引用
收藏
页码:301 / 338
页数:38
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