Longitudinal factor in the spatial distribution of energetic solar flares

被引:1
|
作者
Yazev, S. A. [1 ,2 ]
机构
[1] Russian Acad Sci, Inst Solar Terr Phys, Siberian Branch, Irkutsk 664033, Russia
[2] Irkutsk State Univ, Irkutsk 664033, Russia
关键词
Flare; Southern Hemisphere; Solar Rotation; Longitudinal Distribution; Active Longitude;
D O I
10.1134/S0016793209070081
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Discrete location of large flares near zero Carrington longitude results in artificial breaks within physically related flare clusters. This effect is eliminated by using the data presentation algorithm, which results in the conclusion that drifting zones of intensified sunspot formation (concentrated cores of activity complexes) and energetic flare generation exist in either hemisphere. The indicated L zone is hypothetically related to a non-asymmetric relic solar magnetic field or to the regions where large-scale convective cells, extending to the convective zone bottom, originate.
引用
收藏
页码:871 / 878
页数:8
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