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The seismic structure of the Sun from GONG
Published online by Cambridge University Press: 25 May 2016
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This paper is an interim report of our inferences about the hydrostatic structure of the Sun, following the first report of the GONG team in Science (Gough et al., 1996). That work confirms that the spherically averaged structure of the Sun is more or less in agreement with current standard solar models. However, there remain some significant deviations which we regard as important clues to the existence of dynamical phenomena which are not taken into account in standard solar modelling.
- Type
- Part II: Internal structure and rotation. Seismic inversions
- Information
- Symposium - International Astronomical Union , Volume 181: Sounding Solar and Stellar Interiors , 1997 , pp. 151 - 158
- Copyright
- Copyright © Kluwer 1997
References
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