Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975mnras.171....1f&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 171, Apr. 1975, p. 1-7.
Astronomy and Astrophysics
Astronomy
18
Electron Transitions, Emission Spectra, Iron, Line Spectra, Solar Flares, Solar Spectra, Atomic Energy Levels, Luminous Intensity, Solar Activity, Spaceborne Astronomy, Wavelengths
Scientific paper
Solar flare emission lines due to 2s/n/2p/k/-2s/n-1/2p/k+1/ transitions of Fe XVIII to Fe XXIII are identified in the spectral region between 66 and 140 A. The published solar flare spectra from the Goddard Space Flight Center experiment on OSO 5 were used for this analysis. Line classifications are based on data acquired from recent laboratory observations and theoretical extrapolations from these data. Previous identifications are revised and observations which may permit the measurement of solar flare densities are discussed.
Cowan Robert D.
Fawcett B. C.
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