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Detection of solar gravity mode oscillationsAn analysis of solar velocity data obtained at the Stanford Solar Observatory shows the existence of solar global oscillations in the range 45 to 105 microHz (160 to 370 minutes). These oscillations are interpreted as internal gravity modes of degree l = 1 and l = 2. A good estimate of the order of the modes has also been made. Previously announced in STAR as N84-11086
Document ID
19840036244
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1038/306651a0
Authors
Delache, P. (Stanford University Stanford, CA; Nice, Observatoire, Nice, France)
Scherrer, P. H. (Stanford University Stanford, CA, United States)
Date Acquired
August 12, 2013
Publication Date
December 15, 1983
Publication Information
Publication: Nature
Volume: 306
ISSN: 0028-0836
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0028-0836
Accession Number
84A19031
Funding Number(s)
CONTRACT_GRANT: N00014-76-C-0207
CONTRACT_GRANT: NGR-05-020-559
CONTRACT_GRANT: NSF ATM-77-20580
CONTRACT_GRANT: NAS5-24420
Distribution Limits
Public
Copyright
Other

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