Calculations of the umbral profile of the Zeeman triplet 25250.22 are presented. We have taken into account the effect of a molecular blend from TiO at 25250.24 causing an apparent ncomponent even for longitudinal magnetic fields. Also included is the depression of the spot continuum due to line win
Calculation of 5250.216 Å line profiles in sunspots
✍ Scribed by A. R. Dunn
- Publisher
- Springer
- Year
- 1972
- Tongue
- English
- Weight
- 154 KB
- Volume
- 26
- Category
- Article
- ISSN
- 0038-0938
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📜 SIMILAR VOLUMES
A generalized equation was obtained for calculation of line profiles of solar formations in the assumption of their inhomogeneity. Line profiles of homogeneous formations are a particular consequence of this equation. Analysis of the equation and line profiles calculated from it was carried out.
In two recent papers W6hl (1969) and Mallia (1970) reported on observations of Zeeman splittings of molecular lines within sunspots. Particularly splittings of the MgH line at 5190 2k were measured and the resulting magnetic field strengths H were compared with those from the line FeI 25250.2 ]~ whi