A Measure of Magnetic Field Discontinuity

被引:0
|
作者
Y.-J. Moon
H.S. Yun
S.W. Lee
J.-H. Kim
G.S. Choe
Y.D. Park
G. Ai
H.Q. Zhang
C. Fang
机构
[1] Korea Astronomy Observatory,Department of Astronomy
[2] Seoul National University,Department of Astronomy
[3] Tongmyong University of Information Technology,undefined
[4] Beijing Astronomical Observatory,undefined
[5] Chinese Academy of Science,undefined
[6] Nanjing University,undefined
来源
Solar Physics | 1999年 / 184卷
关键词
Flare; Bright Point; Magnetic Field Vector; Solar Observatory; Flare Activity;
D O I
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中图分类号
学科分类号
摘要
In this paper we introduce a measure of magnetic field discontinuity, MAD, defined as Maximum Angular Difference between two adjacent magnetic field vectors. To examine the characteristics of the MAD, we have considered several active region models having a quadrupolar field configuration and computed MADs over these active regions by approximating the 3-D magnetic fields as an ensemble of charge potential fields or linear force-free fields. The computed MAD fields are studied in comparison with other flare activity indicators such as separators. It is found that (1)  the region of high level MAD corresponds well with the separator, or practically the intersection of the separator with the plane of measurement, (2) it singles out local discontinuities of magnetic fields, and (3) the MAD can also be a measure of the evolutionary status of an active region.
引用
收藏
页码:323 / 338
页数:15
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