Solar soft X-ray flare spectra from OSO-4

descriptionPublicationkeyboard_double_arrow_right Article 01 Jul 1970 English Publisher:Springer Science and Business Media LLCJournal:Solar Physics, volume 13, pages 198-212 (issn: 0038-0938, eissn: 1573-093X,

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Authors: J. F. Meekins; G. A. Doschek; H. Friedman; T. A. Chubb; R. W. Kreplin;

doi: 10.1007/bf00963952

Solar soft X-ray flare spectra from OSO-4

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Abstract

Solar flare spectral data, covering the wavelength range 0.7–8.5 A, are derived from the NRL Bragg crystal spectrometers aboard OSO-4. A detailed analysis of the soft X-ray spectra for the 3b flare of 16 November 1967 (2140 UT) is presented, and it is found that electron temperatures derived from continua and emission lines are compatible with a two or more component plasma, differing in temperature by 6–10 × 106K.

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

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