A measure of magnetic field discontinuity

Citation
Yj. Moon et al., A measure of magnetic field discontinuity, SOLAR PHYS, 184(2), 1999, pp. 323-338
Citations number
26
Categorie Soggetti
Space Sciences
Journal title
SOLAR PHYSICS
ISSN journal
00380938 → ACNP
Volume
184
Issue
2
Year of publication
1999
Pages
323 - 338
Database
ISI
SICI code
0038-0938(199902)184:2<323:AMOMFD>2.0.ZU;2-G
Abstract
In this paper we introduce a measure of magnetic field discontinuity, MAD, defined as Maximum Angular Difference between two adjacent magnetic field v ectors. To examine the characteristics of the MAD, we have considered sever al active region models having a quadrupolar field configuration and comput ed 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 ind icators such as separators. It is found that (1) the region of high level M AD corresponds well with the separator, or practically the intersection of the separator with the plane of measurement, (2) it singles out local disco ntinuities of magnetic fields, and (3) the MAD can also be a measure of the evolutionary status of an active region. An observational test has been made for 2-D MADs, using the Yohkol SXT obse rvation of a Bare in AR 6919 and the vector magnetogram taken at the Mees S olar Observatory during this flare activity. The high level contours of 2-D MAD are found to trace well the observed soft X-ray bright points, which i ndicates that the MAD could serve as a good flare activity indicator.