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Intense magnetic fields and umbral dotsIntense magnetic fields (of one or two kilogauss) situated in a background of weak field and umbral dots (regions of weak field) situated in a background of intense field (the sunspot) have both received considerable, though largely unrelated, discussion in the recent literature. It is suggested that the two phenomena may in fact be less disparate than hitherto presumed. Applying a simple (hydrostatic) model calculation to both phenomena and assuming temperature differences to be constant with height, the depth of each of these structures can be estimated.
Document ID
19770040942
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Roberts, B.
(Chicago, University Chicago, Ill., United States)
Date Acquired
August 8, 2013
Publication Date
December 1, 1976
Publication Information
Publication: Solar Physics
Volume: 50
Subject Category
Solar Physics
Accession Number
77A23794
Funding Number(s)
CONTRACT_GRANT: NGL-14-001-001
Distribution Limits
Public
Copyright
Other

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