Published February 1976
| Version v1
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Theories for convection in stellar atmospheres
- 1. Stockholm Univ. (Sweden). Institutionen foer Teoretisk Fysik
Description
A discussion of the fundamental differences between laboratory convection in a stellar atmosphere is presented. The shortcomings of laterally homogeneous model atmospheres are analysed, and the extent to which these shortcoming are avoided in the two-component representation is discussed. Finally a qualitative discussion on the scaling properties of stellar granulation is presented. (Auth.)
Availability note (English)
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7262067.pdf
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Additional details
Publishing Information
- Imprint Pagination
- 13 p.
- Report number
- USIP--76-04
INIS
- Country of Publication
- Sweden
- Country of Input or Organization
- Sweden
- INIS RN
- 7262067
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CONVECTION; SOLAR GRANULATION; STAR MODELS; STELLAR ATMOSPHERES
- Descriptors DEC
- ATMOSPHERES; ENERGY TRANSFER; HEAT TRANSFER; MATHEMATICAL MODELS; SOLAR ACTIVITY