Solar Flare X-Ray Spectra. II: Laboratory Reproduction in the Region of Fe XXV-XXVI Resonance Lines

Details Solar Flare X-Ray Spectra. II: Laboratory Reproduction in the Region of Fe XXV-XXVI Resonance Lines Solar Flare X-Ray Spectra. II: Laboratory Reproduction in the Region of Fe XXV-XXVI Resonance Lines

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...63..329k&link_type=abstract

Solar Physics, Volume 63, Issue 2, pp.329-335

Physics

4

Scientific paper

A comparison is given of the spectra in the region λ = 1.70 1.95 Å obtained aboard the ‘Intercosmos’ satellites with those observed in laboratory from a vacuum spark. Wavelengths of the reference He-like Fe ion resonance line (ω) and its j-satellite are reviewed. The difference of 0.0006 Å between measured and earlier calculated values is attributed to the Lamb shift of 1s-electron. A discussion is presented of the existence of the Kβ lines in the solar spectra.

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