Observational Results of Full-Disc Helioseismology: Implications for Seismology of Sun-like Stars

Details Observational Results of Full-Disc Helioseismology: Implications for Seismology of Sun-like Stars Observational Results of Full-Disc Helioseismology: Implications for Seismology of Sun-like Stars

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004soph..220..261n&link_type=abstract

Solar Physics, Volume 220, Issue 2, pp.261-268

Physics

2

Scientific paper

A brief review of observational full-disc helioseismology is carried out with emphasis on issues of interest in the developing field of seismology of Sun-like stars. The frequency precision obtained from extended full-disc helioseismic data sets and the activity cycle variation of solar p-mode parameters are summarised and related to recent and potential asteroseismic studies. The potential advantages of sharing approaches to the analysis of real and simulated data between helio- and astero-seismology groups are discussed.

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