Helium resonance lines in the flare of 15 June 1973

Time sequences of He I and He II resonance line intensities at several sites within the flare of June 15, 1973 are derived from observations obtained with Naval Research Laboratory's Slitless Spectroheliograph on Skylab. The data are compared with predictions in six model flare atmospheres base...

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Veröffentlicht in:Solar physics 1989-01, Vol.120 (2 19), p.309-341
Hauptverfasser: Porter, Jason G., Gebbie, Katharine B., November, Laurence J.
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Sprache:eng
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