Observational results of full-disc helioseismology: implications for seismology of Sun-like stars

NEW, R. (2004). Observational results of full-disc helioseismology: implications for seismology of Sun-like stars. Solar Physics, 220 (2), 261-268.

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Link to published version:: https://doi.org/10.1023/B:SOLA.0000031387.19463.a4
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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.

    Item Type: Article
    Additional Information: 25th General Assembly of the International-Astronomical-Union, JUL, 2003, Sydney, AUSTRALIA
    Research Institute, Centre or Group - Does NOT include content added after October 2018: Materials and Engineering Research Institute > Thin Films Research Centre > Nanotechnology Centre for PVD Research
    Identification Number: https://doi.org/10.1023/B:SOLA.0000031387.19463.a4
    Page Range: 261-268
    Depositing User: Ann Betterton
    Date Deposited: 19 May 2010 17:00
    Last Modified: 18 Mar 2021 09:45
    URI: http://shura.shu.ac.uk/id/eprint/2077

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