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The cancellation of magnetic flux. II - In a decaying active regionH-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.
Document ID
19860047775
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Martin, S. F.
(California Inst. of Tech. Pasadena, CA, United States)
Livi, S. H. B.
(California Inst. of Tech. Pasadena, CA, United States)
Wang, J.
(California Institute of Technology Pasadena, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Publication Information
Publication: Australian Journal of Physics
Volume: 38
ISSN: 0004-9506
Subject Category
Solar Physics
Accession Number
86A32513
Funding Number(s)
CONTRACT_GRANT: NGL-05-002-034
CONTRACT_GRANT: NSF ATM-82-11002
CONTRACT_GRANT: AF-AFOSR-82-0018
Distribution Limits
Public
Copyright
Other

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