Model representation of electron density distribution in the topside midlatitude ionosphere using Intercosmos-19 data

Details Model representation of electron density distribution in the topside midlatitude ionosphere using Intercosmos-19 data Model representation of electron density distribution in the topside midlatitude ionosphere using Intercosmos-19 data

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kosis..25..410b&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 25, May-June 1987, p. 410-420. In Russian.

Other

Atmospheric Models, Density Distribution, Ionospheric Electron Density, Midlatitude Atmosphere, Satellite Observation, Intercosmos Satellites, Signal Analysis, Solar Activity Effects, Summer, Vertical Distribution

Scientific paper

An analysis of Intercosmos-19 data and other published information is used to develop a model for the vertical electron density distribution in the midlatitude topside ionosphere for daytime summer conditions and a wide range of solar-activity variations (F10.7 = 60-300). The model has the form of an exponential formula where the coefficients and the Nm and Hm parameters depend linearly on solar activity. The model, which covers all the longitude sectors of the globe, makes it possible to calculate the electron density for any level h not less than hm or directly on the basis of the linear dependence of N on F10.7. It is concluded that this model may be used in the further development of the IRI.

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