Asymmetry of the diurnal variation of E-region electron density at large solar zenith angles and the time equation

Details Asymmetry of the diurnal variation of E-region electron density at large solar zenith angles and the time equation Asymmetry of the diurnal variation of E-region electron density at large solar zenith angles and the time equation

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ge%26ae..33..166p&link_type=abstract

Geomagnetizm i Aeronomiya (ISSN 0016-7940), vol. 33, no. 3, p. 166-169.

Physics

Diurnal Variations, E Region, Ionospheric Electron Density, Solar Position, Zenith, Earth Ionosphere, Electromagnetic Radiation, Horizon, Perturbation Theory

Scientific paper

It is shown that the appearance of an asymmetry in the diurnal variation of E-region electron density at solar zenith angles greater than 60 deg is due to the conventional method of calculating zenith angles from the mean solar time. This method is insufficiently accurate. When the true solar time, determining the position of the sun above the horizon, is used, the asymmetry at large zenith angles does not occur.

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