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Convective dynamos for rotating starsGlobal dynamo theory is applied to the problem of why some stars have field reversing dynamos, and others do not. It is argued that convectively driven dynamos are the most likely source of magnetic fields in stars that have convection zones.
Document ID
19830012592
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Gilman, P. A. (National Center for Atmospheric Research Boulder, CO, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1981
Publication Information
Publication: Smithsonian Astrophysics Observatory 2nd Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Vol. 1
Subject Category
Astrophysics
Accession Number
83N20863
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19830012575Collected WorksSecond Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, volume 1
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