Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.196..907d&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 196, Sept. 1981, p. 907-910. Research supported by the Smithsonian Inst
Astronomy and Astrophysics
Astronomy
16
Calcium, Iron, Lithium, Metal Ions, Solar Flares, X Ray Astronomy, Helium, Ion Production Rates, Ion Recombination, Solar Corona, X Ray Spectra
Scientific paper
A reinterpretation of the high resolution X-ray spectra of Ca XIX and Fe XXV, observed during a solar flare on March 25, 1979, is presented. New ionization fractions for Ca XVIII, Ca XIX, Fe XXIV, and Fe XXV are used, and it is shown that the new calculations substantially change the interpretation of the spectra. It is implied that the flare plasma was ionizing during the early phases of the flare, and recombining during the decay phase.
Doyle Gerry J.
Raymond John C.
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