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The rise and fall of sunspot group 18962 - A case of magnetic submergenceNormal sunspot groups emerge from below the surface as a big arch; the footpoints form a dipole that moves apart and the fields eventually diffuse and disappear. BBSO 18962 was a small dipole with elements which, after spreading apart in the first day of existence, drew back together and disappeared below the surface. It is proposed that the flux loop was pulled back down by magnetic tension and submerged. The circumstances suggest that this behavior may not be uncommon. It implies that some dipoles do not decouple from subsurface fields.
Document ID
19850052494
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Zirin, H.
(California Institute of Technology Pasadena, CA, United States)
Date Acquired
August 12, 2013
Publication Date
April 15, 1985
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 291
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
85A34645
Funding Number(s)
CONTRACT_GRANT: NSF ATM-82-11002
CONTRACT_GRANT: NGL-05-002-034
Distribution Limits
Public
Copyright
Other

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