Theincreasingly high flux predicted to the violet of 4500 ~ by many model solar atmospheres stands in contradiction to the observations. Since one possible cause of the disagreement is that the solar 'windows' by which the observed continuum is established might be obscured by line wings, we have ma
Semi-empirical solar line blanketing
โ Scribed by J. P. Mutschlecner; Charles F. Keller
- Book ID
- 104669851
- Publisher
- Springer
- Year
- 1970
- Tongue
- English
- Weight
- 866 KB
- Volume
- 14
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
A preliminary theoretical solar model is presented that produces closer agreement with observation than has been heretofore possible. The qualitative advantages and shortcomings of this model are discussed and projected improvements are outlined.
Line blanketing due to both the neutral and ionized metals is treated here by the modified picket-fence method and applied to the case of a homogeneous model solar photosphere in strict radiative equilibrium. Improvement in fitting the observed photospheric radiation field is noted over a model in w