Recombination edges observed in solar soft X-ray flare spectra

descriptionPublicationkeyboard_double_arrow_right Article 01 Jul 1970 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 13, pages 213-219 (issn: 0038-0938, eissn: 1573-093X,

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Authors: J. F. Meekins; G. A. Doschek;

doi: 10.1007/bf00963953

Recombination edges observed in solar soft X-ray flare spectra

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Abstract

Edges in the solar soft X-ray flare continuum have been observed with the NRL Bragg crystal spectrometer aboard OSO-4. The edges near 2.06 A, 2.8 A, and 4.46 A are interpreted to be due to an innershell dielectronic recombination process, details of which are presented. Two other edges, 3.59 A and 3.31 A, are interpreted to be due to recombination of the bare sulfur ion and innershell transitions of calcium.

Related Organizations

Naval Research Laboratory Optical Sciences Division
United States
United States Naval Research Laboratory
United States

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