A model of the convection zone is presented which matches an empirical model atmosphere (HSRA) and an interior model. A mixing length formalism containing four adjustable parameters is used. Thermodynamical considerations provide limits on two of these parameters. The average temperature-pressure re
β¦ LIBER β¦
A map of the horizontal flows in the solar convection zone
β Scribed by Frank Hill
- Publisher
- Springer
- Year
- 1990
- Tongue
- English
- Weight
- 587 KB
- Volume
- 128
- Category
- Article
- ISSN
- 0038-0938
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