Behavior of electron density at the E-layer maximum for large solar zenith angles

Details Behavior of electron density at the E-layer maximum for large solar zenith angles Behavior of electron density at the E-layer maximum for large solar zenith angles

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..497p&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, May-June 1985, p. 497-499. In Russian.

Physics

E Region, Ionospheric Electron Density, Periodic Variations, Solar Position, Zenith, Angles (Geometry), Maxima, Midlatitude Atmosphere

Scientific paper

It is shown that relative variations of the electron density at the E-layer maximum on solar zenith angle chi for large values of chi can be explained if variations of the Chapman function with the height of the maximum are taken into account. Expressions for the relative variations are obtained which can be used to predict critical frequencies for chi = 75-90 deg.

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