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Molecular line haze opacity in sunspots

✍ Scribed by V. P. Gaur; M. C. Pande; M. Sah

Publisher: Springer
Year: 1979
Tongue: English
Weight: 221 KB
Volume: 62
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00150134

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✦ Synopsis

It has been shown that bound-bound opacity due to electronic transitions of molecules CN, Call, MgH, and TiO explains, in a first approximation, the line haze opacity postulated by Zwaan (1974) for the region 0.5 ~m to 0.9 ixm of the umbral spectrum. ZSM-74 were calculated using the formulations by Golden (1967) (cf. also Kipper, 1973). The molecular data used by us is summarised in Table I.

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