Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.186..327h&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 186, Feb. 1979, p. 327-342. NSF-USAF-supported research.
Astronomy and Astrophysics
Astronomy
26
Astrometry, Limb Darkening, Solar Oblateness, Solar Oscillations, Photosphere, Power Spectra, Solar Gravitation, Stellar Models, Vibration Mode
Scientific paper
Solar oblateness observations made on seven days in September 1973 are analyzed. Power spectra are obtained for four solar-diameter measurements, and both power spectra and phase information are extracted from Fourier transforms of the data sets. Significant peaks are found in the averaged power spectrum at 0.25, 0.37, 0.41, 0.46, 0.54, and 0.61 mHz. Further analysis of the properties of these peaks reveals an impressive degree of phase coherency. It is proven that a significant fraction of the oscillatory power is produced by fluctuating changes in the apparent limb-darkening function. Possible nonsolar and solar mechanisms for producing effective fluctuating changes in the apparent limb-darkening function are considered. It is concluded that the detected oscillations are statistically significant, that a significant fraction of the oscillatory power is solar in origin, and that the oscillations are eigenmodes of the sun.
Caudell Thomas P.
Hill Adrian H.
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