Abundances from solar flare line spectroscopy

Details Abundances from solar flare line spectroscopy Abundances from solar flare line spectroscopy

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989stin...9132022m&link_type=abstract

Final Report Universities Space Research Association, Washington, DC.

Other

Abundance, Computer Programs, Gamma Rays, Line Spectra, Solar Flares, Spectroscopy, Angular Distribution, Data Processing, Gamma Ray Spectrometers, Particle Interactions, Solar Maximum Mission

Scientific paper

Updating and improvement of computer codes used in the abundance analyses of solar-flare gamma-ray data are described. These modifications are itemized in detail. The abundance analysis technique was then applied to data obtained by the Gamma-Ray Spectrometer of the Solar Maximum Mission spacecraft for the 27 April 1981 solar flare to set constraints on the interacting-particle angular distribution. The results are presented. Research in several other areas was also performed and they are discussed.

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