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.
Solar Ciiresonance line profiles
โ Scribed by R. A. Berger; E. C. Bruner; R. J. Stevens
- Publisher
- Springer
- Year
- 1970
- Tongue
- English
- Weight
- 824 KB
- Volume
- 12
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
The profiles of thesolar C It resonance doublet 21334.6 ]~ are presented. Possible broadening mechanisms are discussed.
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