Searching for G-MODES at the Solar Limb

Details Searching for G-MODES at the Solar Limb Searching for G-MODES at the Solar Limb

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997spd....28.0209t&link_type=abstract

American Astronomical Society, SPD meeting #28, #02.09; Bulletin of the American Astronomical Society, Vol. 29, p.894

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Scientific paper

The detection and measurement of solar g-modes is of significant importance in the study of the internal structure of the Sun. The g-mode signal in intensity is predicted to peak very close to the solar limb. To enhance the probability of detecting g-modes, we have tried to reduce the solar background ``noise'' signal by differencing the signal in a narrow annulus at the solar limb from the signal in an adjacent (interior) annulus. We will present some preliminary results from a study of Ca K-line intensity observations obtained at the South Pole during the austral summer of 1995/95.

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