Resonant three-wave interactions of solar g-modes

Details Resonant three-wave interactions of solar g-modes Resonant three-wave interactions of solar g-modes

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...277l..17g&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 277, Feb. 1, 1984, p. L17-L19.

Astronomy and Astrophysics

Astrophysics

9

Solar Oscillations, Solar Spectra, Wave Interaction, Coupled Modes, Resonant Frequencies

Scientific paper

The observed g-mode oscillation spectrum of the sun is compared with a plot of the number of possible resonant three-wave interactions of theoretical g-modes at a given period versus the frequency difference of the coupled modes. A very large peak is found near 160 minutes, corresponding to the well-known 160-minute solar oscillation. Peaks in the curve are also found to coincide with the recently identified g-mode data of Delache and Scherrer (1983).

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