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Fine Structure of Solar Acoustic Oscillations Due to RotationThe nature of the fine structure of high order, low degree five minute period solar oscillations following from various postulated forms of spherical rotation is predicted. The first and second order effects of rotation are included.
Document ID
19850016776
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Goode, P. R. (Arizona Univ. Tucson, AZ, United States)
Dziembowski, W. (Polish Acad. of Sci. Warsaw, United States)
Date Acquired
August 12, 2013
Publication Date
December 15, 1984
Publication Information
Publication: JPL Solar Seismology from Space.
Subject Category
Solar Physics
Accession Number
85N25087
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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