The use of 1356-A emission intensity to determine parameters of the F-region

Details The use of 1356-A emission intensity to determine parameters of the F-region The use of 1356-A emission intensity to determine parameters of the F-region

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982kosis..20..736s&link_type=abstract

Kosmicheskie Issledovaniia, vol. 20, Sept.-Oct. 1982, p. 736-741. In Russian.

Physics

Electron Density Profiles, F Region, Ionospheric Electron Density, Oxygen Spectra, Ultraviolet Radiation, Line Spectra, Satellite Observation, Solar Activity Effects

Scientific paper

Methods are proposed for the correct determination of the planetary distribution of maximum electron densities (NmF), the corresponding critical frequencies (f0F), the heights of these densities (hmF), and one of the most characteristic parameters describing the international reference profile Ne(h) of the F-region. The determination relies upon measurements of the 1356-A and 6300-A lines, and on a local measurement of electron density. Necessary orbital parameters for conducting pertinent satellite experiments are indicated; and accurate expressions are derived for the intensity of the 1356-A line; and some inaccuracies in the determination of NmF and hmF on the basis of intensity measurements of the two aforementioned oxygen lines are discussed.

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