Computer Science
Scientific paper
Oct 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..743k&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Sept.-Oct. 1985, p. 743-749. In Russian.
Computer Science
Electron Energy, Energy Spectra, Ionospheric Electron Density, Line Spectra, Photoelectrons, Solar Terrestrial Interactions, Spectral Line Width
Scientific paper
Dependences of photoelectronic line (PL) widths at 22.2-27.2 eV on the ionospheric parameters n sub e, T sub e, n, and T are obtained, and fluxes in the photoelectronic lines are calculated for heights of 190-320 km. An analysis is made of the effect of the instrument function on the profile, area, and magnitude of the flux in the PL maximum. This is important in the diagnostics of neutral and charged components of the ionosphere, and solar radiation in the 304-A line on the basis of PL parameters.
Kiselev Alexander V.
Mikirov A. E.
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