Detection of solar gravity mode oscillations

Physics

Scientific paper

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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.

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