Spectrum synthesis of EUV solar flare line profiles

Details Spectrum synthesis of EUV solar flare line profiles Spectrum synthesis of EUV solar flare line profiles

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980wsco.rept.....t&link_type=abstract

Final Report Weber State Coll., Ogden, UT. Dept. of Physics.

Physics

Chromosphere, Solar Flares, Spectrographs, Solar Spectra

Scientific paper

A classic double ribbon flare of importance 1B occurred at approximately 1405 UT on June 15, 1973, reached an H alpha maximum at 1413 UT, and ended at 1455 UT. The flare occurred in an old and simplifying bipolar region at N18 W32. This flare was studied due to the extensive temporal data available. A total of 136 spectra of wavelength ranges from 1100 to 3000 A were taken during the flare's duration by the Naval Research Laboratory normal incidence slit spectrograph. Using this data the nature of the solar chromosphere of a flare event as a function of time was determined.

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