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The cancellation of magnetic flux. II - In a decaying active region

Authors :
Martin, S. F
Livi, S. H. B
Wang, J
Source :
Australian Journal of Physics. 38
Publication Year :
1985
Publisher :
United States: NASA Center for Aerospace Information (CASI), 1985.

Abstract

H-alpha filtergrams and videomagnetograms are used to study an active region during its period of decay on August 3-8, 1984; the decay had been initiated by a fragmentation process in which very small knots of magnetic flux separated from larger concentration of flux. The disappearance of magnetic flux was always observed when the small fragments of flux encountered other small fragments or concentrations of flux of opposite polarity. Such 'cancellations' are shared by both polarities of magnetic field, and it is deduced that the disappearance of flux occurred either at or within 5 arcsec of the apparent dividing line between the opposite polarities. All of the 22 flares observed during the decay of this region were initiated around sites where magnetic flux was cancelling or was deduced to be cancelling during the flares. It is hypothesized that cancellation was one of the necessary conditions for flaring in this active region.

Subjects

Subjects :
Solar Physics

Details

Language :
English
ISSN :
00049506
Volume :
38
Database :
NASA Technical Reports
Journal :
Australian Journal of Physics
Notes :
NGL-05-002-034, , NSF ATM-82-11002, , AF-AFOSR-82-0018
Publication Type :
Report
Accession number :
edsnas.19860047775
Document Type :
Report