A simplified representation of the temperature distribution in the solar photosphere is proposed: 0 (v0) = 00 --01 log r0. An expression is derived for the emergent continuous spectrum from the simple model. The limitations and applications of the simple model are discussed.
โฆ LIBER โฆ
A simplified model
โ Scribed by P.E. Lisseter; A.C. Fowler
- Book ID
- 103674815
- Publisher
- Elsevier Science
- Year
- 1992
- Tongue
- English
- Weight
- 588 KB
- Volume
- 18
- Category
- Article
- ISSN
- 0301-9322
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