High dielectronic satellite lines in solar flare spectra

Details High dielectronic satellite lines in solar flare spectra High dielectronic satellite lines in solar flare spectra

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jphys..40....1s&link_type=abstract

Journal de Physique, vol. 40, Feb. 1979, Supplement, p. C1-98 to C1-101.

Physics

Atomic Physics

17

Atomic Physics, Atomic Spectra, Electron Energy, Solar Flares, Solar Physics, Solar Spectra, Electron Transitions, Energy Levels, High Resolution, Iron

Scientific paper

Resonance lines of highly ionized H and He-like ions and their associated satellite lines are used to determine the electron temperature and the transient state of the plasma in solar flares. The intensity ratio of the satellite lines 1s(2)nl-1s2pl to the resonance line 1s(2)-1s2p has been calculated for the n equals 2, 3 and 4 shells of Fe XXIV. The results have enabled the identification of many lines in the only available high resolution solar flare iron spectrum and give a good estimate of the spectral intensity in the resonance line by evaluating the contribution due to the blending of the satellites with n not less than 3.

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