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With the recent establishment of the GONG network of helioseismic observatories and the launch of the SOHO solar observatory, 1996 was an ideal time to organise a workshop on the relationship between solar oscillations and convection.
The reviews in these proceedings provide overviews of the current status of studies of solar and stellar structure and the radiative magnetohydrodynamics of solar convection, presenting and incorporating the newest results from numerical hydrodynamic simulations and helioseismic observations. The contributed papers present the very latest developments in each of these fields.
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1
SCORe'96: Solar Convection and Oscillations and their Relationship (Astrophysics and Space Science Library)
January 31, 1998, Springer
Hardcover
in English
- 1 edition
0792348524 9780792348528
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2
SCORe '96: Solar Convection and Oscillations and their Relationship
1997, Kluwer Academic Publishers
in English
0792348524 9780792348528
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Book Details
First Sentence
"The outer solar convection zone extends over 29 % of the solar radius and contains about 2 % of the mass of the Sun (e.g. Christensen-Dalsgaard, Gough & Thompson 1991; Kosovichev & Fedorova 1991)."
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