Molecules in the solar photosphere

descriptionPublicationkeyboard_double_arrow_right Article 01 Apr 1969 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 7, pages 17-21 (issn: 0038-0938, eissn: 1573-093X,

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Authors: M. C. Pande; V. P. Gaur; B. M. Tripathi;

doi: 10.1007/bf00148399

Molecules in the solar photosphere

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Abstract

A consideration of the dissociation equilibrium of diatomic molecules in the Utrecht Reference Photosphere leads us to conclude that SH, SiO, CS, HF and HCl may show up in enough concentrations in the solar atmosphere. The number above photosphere for these molecules is comparable with or more than that of MgH.

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