High-resolution observations of X-ray transitions in Fe XXV-XXIII

Details High-resolution observations of X-ray transitions in Fe XXV-XXIII High-resolution observations of X-ray transitions in Fe XXV-XXIII

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985jphb...18l.797s&link_type=abstract

Journal of Physics B - Atomic and Molecular Physics (ISSN 0022-3700), vol. 18, Dec. 14, 1985, p. L797-L801. NASA-supported resea

Physics

5

Atomic Spectra, Electron Transitions, Iron, Solar X-Rays, X Ray Spectra, High Resolution, Resonance Lines, Solar Flares, Solar Spectrometers, Spectrum Analysis

Scientific paper

The wavelengths of X-ray transitions in Fe XXV-XXIII have been measured using a high-resolution spectrum reflected from the Ge(13-1) planes. A number of transitions have been resolved for the first time in solar flare spectra, and the contributions of the Fe XXIV n = 3 satellites to the Fe XXV parent lines are discussed. The QED contributions to the wavelengths of the Fe XXIV n = 3 satellite transitions have been determined.

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