Modelling the variation of solar p-mode frequencies

Details Modelling the variation of solar p-mode frequencies Modelling the variation of solar p-mode frequencies

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..511d&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 511-512 (SEE N89-25819 19-92)

Physics

1

Frequency Measurement, P Waves, Solar Oscillations, Stellar Models, Sun, Green'S Functions, Solar Constant, Solar Cycles, Solar Diameter

Scientific paper

A Green's function technique to study long-term variations of the Sun (with characteristic time scales from one month to millions of years) is presented. The method is the combination of two previous analyses carried out independently by Gough and by Dappen. The study was motivated by observational progress on solar p-mode frequency variations.

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