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Detection of Solar Gravity Mode OscillationsAn analysis of solar velocity data obtained at the Stanford Solar Observatory has shown the existence of solar global oscillations. The oscillations are in the range 45 to 105 micro Hz (160 to 370 minutes) and are interpreted as internal gravity modes of degree l=1 and l=2.
Document ID
19850016759
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Scherrer, P. H. (Stanford Univ. CA, 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
85N25070
Funding Number(s)
CONTRACT_GRANT: NGR-05-020-559
CONTRACT_GRANT: NAS5-24420
CONTRACT_GRANT: N00014-76-C-0207
CONTRACT_GRANT: NSF ATM-77-20580
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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