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

Abstract
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-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 -values measured. The observations were made with the Birmingham Solar Oscillations Network (‘BISON’).

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