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Inferring solar structure variations from photometric and helioseismic observationsPresent large scale photometric and helioseismic data may be related to spatial and temporal deviations from an otherwise static, spherical solar convection zone (SCZ). New space experiments combine precise photometric, helioseismic, and magnetic observational capabilities (like SOHO and MDI) and will provide data needed to understand the interaction of magnetic fields and global scale circulation in the SCZ. Even simple physical arguments make it clear that the anticipated accuracy of these new experiments virtually guarantees new constraints on models of the SCZ.
Document ID
19910049472
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kuhn, J. R.
(Michigan State University East Lansing, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1991
Publication Information
Publication: of the COSPAR 28th Plenary Meeting, The Hague, Netherlands, June 25-July 6, 1990. A91-34076 13-92) Advances in Space Research
ISSN: 0273-1177
Subject Category
Solar Physics
Accession Number
91A34095
Funding Number(s)
CONTRACT_GRANT: NSF PHY-89-04035
CONTRACT_GRANT: NSF ATM-89-06640
Distribution Limits
Public
Copyright
Other

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