From an analysis of Stokes parameter profiles measured in a unipolar sunspot, properties of its large-scale magnetic field structure have been derived. With due allowance for our present knowledge about the Wilson effect and the height of line formation, an expression for the field strength distribu
The profiles of fraunhofer lines in the presence of zeeman splitting
โ Scribed by J. M. Beckers
- Publisher
- Springer
- Year
- 1969
- Tongue
- English
- Weight
- 760 KB
- Volume
- 9
- Category
- Article
- ISSN
- 0038-0938
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๐ SIMILAR VOLUMES
A self-contained summary of the generalized Unno theory of LTE line formation in solar magnetic fields and its application to the numerical computation of Stokes parameter profiles is given. Within this context, computational details of general interest are described and numerical results for sunspo
We derive the conditions under which the profile of a weak Fraunhofer line can be described as the convolution of the separate profiles of damping, thermal and non-thermal motions at the average depth of formation of the line. The average velocity distribution along the line of sight, rather than it