The variation in the strength of low-l solar p-modes - 1981-92

Details The variation in the strength of low-l solar p-modes - 1981-92 The variation in the strength of low-l solar p-modes - 1981-92

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.265..888e&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 265, p. 888

Astronomy and Astrophysics

Astronomy

36

Solar Interior, Solar Cycles, Solar Flux, Solar Oscillations, Solar Magnetic Field, Stellar Models, Power Spectra

Scientific paper

The acoustic eigenmodes of the sun are a well-recognized probe of the structure of the solar interior. We report here on a measurement of the strength of the low-l p-mode oscillations throughout a solar cycle. There is an increase of 35 +/-5 percent in the strength of the modes from solar maximum to solar minimum, consistent for all the l-values measured. The observations were made with the Birmingham Solar Oscillations Network.

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