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The effects of stark broadening in the radio recombination line temperatures

✍ Scribed by Janet P. Simpson


Publisher
Springer Netherlands
Year
1973
Tongue
English
Weight
821 KB
Volume
20
Category
Article
ISSN
0004-640X

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πŸ“œ SIMILAR VOLUMES


The Zeeman broadening of highnsolar reco
✍ A. Greve πŸ“‚ Article πŸ“… 1975 πŸ› Springer 🌐 English βš– 580 KB

The Zeeman broadening of high n lines is derived. While in areas of the quiet Sun with field strengths of ~ 1 G the upper boundary of the observable frequency region of recombination lines is defined by electron impact broadening, in active regions with field strengths >~ 25 G the Zeeman broadening