Solar Physics

, Volume 220, Issue 2, pp 261–268

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

  • Roger New

DOI: 10.1023/B:SOLA.0000031387.19463.a4

Cite this article as:
New, R. Solar Physics (2004) 220: 261. doi:10.1023/B:SOLA.0000031387.19463.a4


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.

Copyright information

© Kluwer Academic Publishers 2004

Authors and Affiliations

  • Roger New
    • 1
  1. 1.School of Science and MathematicsSheffield Hallam UniversitySheffieldU.K.

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