Detection of solar gravity mode oscillations

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

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sses.nasa..173s&link_type=abstract

In JPL Solar Seismology from Space. p 173-182 (SEE N85-25060 14-92)

Physics

9

Fourier Transformation, Power Spectra, Solar Gravitation, Solar Oscillations, Approximation, Asymptotic Methods, Doppler Effect

Scientific paper

An 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 μHz (160 to 370 minutes) and
are interpreted as internal gravity modes of degree l = 1 and l = 2.

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