Theoretical emission line strengths for
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F. P. Keenan; S. M. McCann; K. G. Widing
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Article
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1988
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Springer
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English
โ 328 KB
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