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The cooling time scales of growing sunspotsThe evolution of brightness and magnetic fields of growing sunspots is studied. Growing sunspots are found to be brighter (or less dark) than stable sunspots with the same magnetic field strength. From comparison of brightness and magnetic fields of a growing sunspot with those of stable sunspots, a dynamical parameter, the cooling time, of the growing sunspot is obtained. Ten growing sunspots are studied, and cooling times of 0.5 to 9 hr are found. Two models, the inhibition model and the Alfven wave model, give cooling times of about 0.05 hr, based on linear theory. The discrepancy between theory and observation may be due to the fact that the observed sunspots are in the nonlinear regime.
Document ID
19870043722
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Chou, Dean-Yi
(Big Bear Solar Observatory; California Institute of Technology Pasadena, United States)
Date Acquired
August 13, 2013
Publication Date
January 15, 1987
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 312
ISSN: 0004-637X
Subject Category
Solar Physics
Accession Number
87A30996
Funding Number(s)
CONTRACT_GRANT: NSF ATM-82-11002
CONTRACT_GRANT: NGL-05-002-034
Distribution Limits
Public
Copyright
Other

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