Detection of solar gravity mode oscillations

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

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983natur.306..651d&link_type=abstract

Nature (ISSN 0028-0836), vol. 306, Dec. 15, 1983, p. 651-653. Research supported by the Max C. Fleischmann Foundation, Centre Na

Physics

95

Fast Fourier Transformations, Gravitation, Oscillations, Power Spectra, Solar Physics, Velocity, Low Frequencies, Solar Spectra, Sun, Surfaces

Scientific paper

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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