On the height variation of the intensities and the profile widths of the lines λ5303 Å and λ6374 Å in the solar corona.

Details On the height variation of the intensities and the profile widths of the lines λ5303 Å and λ6374 Å in the solar corona. On the height variation of the intensities and the profile widths of the lines λ5303 Å and λ6374 Å in the solar corona.

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990bsold..12...79m&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 12/90, p. 79 - 83

Physics

Solar Corona: Line Profiles, Solar Corona: Line Intensities

Scientific paper

Spectrograms of the coronal lines λ5303 Å and λ6374 Å have been received at the 20-cm coronograph at the latitudes 5°N - 20°S during October - December, 1983. The study of the spectrograms shows that the value of the intensity gradient decreased with the increase of the profile width of the lines. Also, the value of the intensity gradient of the line λ5303 Å decreased and the value of the intensity gradient of the line λ6374 Å increased with the increase of the region brightness. The widths of the line profiles.

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