Relative distribution of "hot" and "cold" coronal matter.

Details Relative distribution of "hot" and "cold" coronal matter. Relative distribution of "hot" and "cold" coronal matter.

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990bsold..11...92m&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 11/90, p. 92 - 95

Physics

Solar Corona: Temperatures

Scientific paper

During October-December, 1983, the spectrograms of the coronal lines λ5303 Å and λ6374 Å have been obtained at the 20-cm coronograph. The instrumental profile of the spectrograph was ≍0.4 Å. Influence of the height and the latitude on the intensity ratio of these lines was investigated. Using this investigation and some assumptions it was established that hot matter-cold matter ratio increased with height. The value of this ratio was 2.5 - 4.0 with the height intervals 33 - 97″and the latitude intervals 5°N - 20°S.

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