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

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Abstract

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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  1. School of Science and Mathematics, Sheffield Hallam University, Howard Street, Sheffield, S1 1WB, U.K.

    Roger New

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New, R. Observational Results of Full-Disc Helioseismology: Implications for Seismology of Sun-like Stars. Solar Physics 220, 261–268 (2004). https://doi.org/10.1023/B:SOLA.0000031387.19463.a4

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