Strong line wings and the V-reversal in umbral countours of Fe~ 6302.5/~ and similar lines have been explained earlier by inhomogeneous magnetic models. It is shown that both effects may also be explained assuming a homogeneous magnetic field and homogeneous umbral model atmospheres. A discussion o
Zeeman splitting of molecular lines in sunspot spectra
β Scribed by E. A. Mallia
- Publisher
- Springer
- Year
- 1970
- Tongue
- English
- Weight
- 190 KB
- Volume
- 14
- Category
- Article
- ISSN
- 0038-0938
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