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Molecular line haze opacity in sunspots
Authors:V P Gaur  M C Pande  M Sah
Institution:(1) Uttar Pradesh State Observatory, Naini Tal, India
Abstract:It has been shown that bound-bound opacity due to electronic transitions of molecules CN, CaH, MgH, and TiO explains, in a first approximation, the line haze opacity postulated by Zwaan (1974) for the region 0.5 mgrm to 0.9 mgrm of the umbral spectrum.
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