NASA NTRS · 19840036244
Detection of solar gravity mode oscillations
Abstract
An 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
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Delache, P., Scherrer, P. H.. 1983-12-15. Detection of solar gravity mode oscillations. https://ntrs.nasa.gov/citations/19840036244
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