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Spectral lines observed in solar flares between 171 and 630 angstroms
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1978
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Terrestrial Gamma-ray FlashesPhotometrySolar FlaresSolar VariabilityFe XxiPhysicsSolar Terrestrial EnvironmentSolar ConvectionEngineeringNatural SciencesSpace PhysicSpectral LinesSolar-terrestrial InteractionSpace WeatherSolar PhysicSolar ActivitySunspot StudiesAstrophysics
view Abstract Citations (260) References (21) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Spectral lines observed in solar flares between 171 and 630 Angstroms. Dere, K. P. Abstract Several hundred spectral lines emitted in solar flares between 171 and 630 A have been recorded by the Naval Research Laboratory spectroheliograph aboard Skylab. The wavelengths, identifications, and intensity estimates of these lines are presented, based on measurements of all of the suitable flare plates. Nearly 100 new and unidentified lines have been observed. Identifications of three Fe XXI and two Fe XVII lines are suggested. Publication: The Astrophysical Journal Pub Date: May 1978 DOI: 10.1086/156110 Bibcode: 1978ApJ...221.1062D Keywords: Line Spectra; Solar Flares; Solar Spectra; Doppler Effect; Skylab Program; Spectroheliographs; Solar Physics; Extreme UV:Solar Flares; Solar Flares: Line Identifications full text sources ADS |