Solar flare X-ray spectra between 7.8 and 23.0 angstroms

Details Solar flare X-ray spectra between 7.8 and 23.0 angstroms Solar flare X-ray spectra between 7.8 and 23.0 angstroms

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...241..409m&link_type=abstract

Astrophysical Journal, Part 1, vol. 241, Oct. 1, 1980, p. 409-416.

Astronomy and Astrophysics

Astrophysics

89

Line Spectra, Solar Flares, Solar X-Rays, X Ray Spectroscopy, Iron, Metal Ions, Oxygen Spectra

Scientific paper

The high-resolution X-ray spectra taken during a large solar flare on 1979 June 10 are presented. Many lines of highly ionized iron are resolved and identified for the first time in solar spectra. Lines with a wide range of excitation temperatures have similar time development during the flare's rapid rise phase. The density sensitive line ratios in Fe XXI and Fe XXII are discussed.

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