Theoretical line intensities from MgVI, SiVIII, and SX coronal ions

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1990 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 172, pages 47-50 (issn: 0004-640X, eissn: 1572-946X,

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Authors: B. N. Dwivedi;

doi: 10.1007/bf00645557

Theoretical line intensities from MgVI, SiVIII, and SX coronal ions

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Abstract

Emission line intensities from MgVI, SiVIII, andSX ions of nitrogen sequence have been computed by use of the model atmosphere of Kopp and Orrall (1976) for the quiet Sun and coronal holes and compared with observational data available from rocket and satellite.

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Banaras Hindu University
India

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