Analysis of solar flares optical spectra. III - The line emission of the June 4, 1980 white light flare

Details Analysis of solar flares optical spectra. III - The line emission of the June 4, 1980 white light flare Analysis of solar flares optical spectra. III - The line emission of the June 4, 1980 white light flare

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26as...55..425d&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 55, March 1984, p. 425-438. Research supported by the Consig

Astronomy and Astrophysics

Astrophysics

Optical Emission Spectroscopy, Solar Flares, Solar Spectra, Abundance, Radiant Flux Density, Spectral Line Width

Scientific paper

The spectra of the white light flare of June 4, 1980 observed with the Universal Spectrograph of the Sacramento Peak Observatory have been presented in paper II of this series. The authors give here all the parameters (central peak wavelength and intensity, width at half maximum, total power radiated in the line and so on) obtained from the line emission analysis for central part of the flare kernel.

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