Empirical model of the relative ion composition of the upper ionosphere

Details Empirical model of the relative ion composition of the upper ionosphere Empirical model of the relative ion composition of the upper ionosphere

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..311i&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Mar.-Apr. 1985, p. 311-313. In Russian.

Computer Science

Atmospheric Models, Ionospheric Ion Density, Solar Activity Effects, Upper Ionosphere, Altitude, Solar Terrestrial Interactions

Scientific paper

An empirical model of the ion composition of the upper ionosphere for the altitude range of 400-1000 km is developed which can be used in the IRI-78 model in the IONDEN procedure. This simple model of relative ion composition above the F2-layer maximum agrees on the whole with the IRI-78 model for Phi = 30-35 deg. The empirical model does have the following advantages over IRI-78: it takes into account N(+) ions and the dependence of composition on solar activity, and it provides for an improved determination of the dependence on latitude and solar zenith angle.

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