Detection of solar gravity mode oscillations

Details Detection of solar gravity mode oscillations Detection of solar gravity mode oscillations

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983dsgm.book.....s&link_type=abstract

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Physics

Power Spectra, Solar Gravitation, Solar Oscillations, Solar Spectra, Solar Velocity, Velocity Distribution, Doppler Effect, Extremum Values, Fast Fourier Transformations, Line Spectra, Solar Activity, Solar Observatories, Spectrum Analysis, Sun

Scientific paper

An analysis of solar velocity data obtained at the Stanford Solar
Observatory has shown the existence of solar global oscillations
(Delache and Scherrer, Nature, in press). The oscillations are in the
range of 45 to 105 microHz (160 to 370 minutes) and are interpreted as
internal gravity modes of degree l=1 and l=2.

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