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Perspectives in Helioseismology

Gough1, Leibacher, Scherrer

  • 1D. O. Gough is with the Institute of Astronomy, University of Cambridge, Cambridge, CB3 OHA UK. J. W. Leibacher is with the National Solar Observatory, Tucson, AZ, USA. P. H. Scherrer is with the Department of Physics, Stanford University, Stanford, CA, USA. J. Toomre is with JILA, University of Colorado, Boulder, CO, USA.

Science (New York, N.Y.)
|May 31, 1996
PubMed
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Helioseismology uses solar oscillation frequencies to study the Sun's interior. New data from Global Oscillation Network Group (GONG) and Solar and Heliospheric Observatory (SoHO) advance our understanding of stellar physics.

Area of Science:

  • Solar physics
  • Stellar astrophysics
  • Helioseismology

Background:

  • Helioseismology offers a unique laboratory for studying physical processes under extreme conditions.
  • Understanding the Sun's interior is crucial for comprehending stellar operation.

Purpose of the Study:

  • To probe the Sun's interior structure and dynamics with high precision.
  • To utilize solar oscillation frequencies for detailed analysis.

Main Methods:

  • Observing nearly 10 million resonant modes of oscillation in the solar atmosphere.
  • Utilizing continuous, high-cadence imaging data from Global Oscillation Network Group (GONG) and Solar and Heliospheric Observatory (SoHO).

Main Results:

  • High-accuracy frequency measurements of solar oscillations are essential for interior modeling.

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  • Early results from GONG are resolving existing issues and posing new theoretical questions.

    • Conclusions:

    • The combination of GONG and SoHO data marks a new era in helioseismology.
    • Further theoretical work is needed to interpret findings and understand solar operation.