Electron densities in a solar flare derived from X-ray spectra

Details Electron densities in a solar flare derived from X-ray spectra Electron densities in a solar flare derived from X-ray spectra

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982stin...8325647m&link_type=abstract

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Computer Science

Electron Density (Concentration), Line Spectra, Solar Flares, Bragg Angle, X Ray Spectra

Scientific paper

A major solar flare was observed with the RAP crystal of the SOLEX B spectrometer. The spectra were obtained by scanning back and forth between Bragg angles of 17.4 deg and 61.7 deg (7.8 to 23 A) at a rate of 0.525 degrees-.15. A full scan took 84.5 sec. A line list identifying more than 100 lines observed in this flare was compiled. Measurements of the density sensitive O 7 lines near 22 A are discussed.

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