Analysis of the optical spectra of solar flares. I - The flare of April 30, 1976

Details Analysis of the optical spectra of solar flares. I - The flare of April 30, 1976 Analysis of the optical spectra of solar flares. I - The flare of April 30, 1976

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...47..485a&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 47, Mar. 1982, p. 485-503. Research supported by the Consiglio Nazionale del

Astronomy and Astrophysics

Astrophysics

7

Emission Spectra, Optical Emission Spectroscopy, Solar Flares, Solar Spectra, Spectral Energy Distribution, Line Spectra, Solar Maximum Mission, Solar X-Rays, Tables (Data)

Scientific paper

A novel interactive method for the reduction of solar flare spectra is described which permits the determination of values in the continuum emission of the flare, as well as such line emission parameters as wavelength, line maximum emission intensity, halfwidth, total emissivity within the line, and line identification. The procedure has been tested on existing observational material, and results are presented for the case of the April 30, 1976 flare spectra.

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