Review of observations relevant to solar oscillations

Details Review of observations relevant to solar oscillations Review of observations relevant to solar oscillations

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pccv.conf...83s&link_type=abstract

Pulsations in Classical and Cataclysmic Variable Stars, Proceedings of the conference held 1-4 June 1982 in Boulder, CO. Edited

Physics

Acceleration (Physics), P Waves, Solar Activity Effects, Solar Oscillations, Velocity Measurement, Astronomical Models, Dilatational Waves, Magnetic Disturbances, Solar Observatories

Scientific paper

Recent solar oscillation observations and methods used are described. Integrated or almost integrated sunlight (Sun as a star observation) was observed. The most certain observations are in the 5 minute range. The p-mode and g-mode oscillations are expected from 3 to more than 300 minutes. The possible period ranges are described into the three intervals: (1) the 5 minute range for which the most dramatic and certain results are reported; (2) the 10 to 20 minute range for which solar diameter oscillations are reported; and (3) the 160 minute oscillation found in velocity and several other quantities.

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