Theoretical emission line strengths for Ovcompared to EUV solar observations
โ Scribed by F. P. Keenan; G. A. Warren; J. G. Doyle; K. A. Berrington; A. E. Kingston
- Publisher
- Springer
- Year
- 1994
- Tongue
- English
- Weight
- 461 KB
- Volume
- 150
- Category
- Article
- ISSN
- 0038-0938
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๐ SIMILAR VOLUMES
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A comparison of Skylab S082A observations for several solar flares with calculations of the electron temperature sensitive emission line ratio R l = I(2s2p lp \_ 2s 2 1S)/i(2s2 p 3p1 \_ 2s 2 IS) = = 1(256.68 ~)/I(491.45 A,) in Be-like S xnI reveals good agreement between theory and experiment, which
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