On the identification of Fe ix and Ni xi lines from coronal spectral

descriptionPublicationkeyboard_double_arrow_right Article 01 Mar 1975 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 41, pages 109-113 (issn: 0038-0938, eissn: 1573-093X,

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Authors: Fran�oise Magnant-Crifo;

doi: 10.1007/bf00152961

On the identification of Fe ix and Ni xi lines from coronal spectral

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Abstract

Identifications of coronal lines with transitions of Fe ix and Ni xi, as proposed by Wagner and House, and Svensson, Ekberg and Edlen, are checked by means of line intensity ratios, from observations obtained at the 1965 eclipse. All the suggestions of Svensson, Ekberg and Edlen are suitable.

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