Modeling the effects of a solar flare on the atmospheric electric field at high latitudes

Details Modeling the effects of a solar flare on the atmospheric electric field at high latitudes Modeling the effects of a solar flare on the atmospheric electric field at high latitudes

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ge%26ae..28..169b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 28, Jan.-Feb. 1988, p. 169-171. In Russian.

Mathematics

Atmospheric Electricity, Ionospheric Disturbances, Polar Regions, Solar Flares, Asymmetry, Diurnal Variations, Magnetospheric Instability, Mathematical Models, Solar Terrestrial Interactions

Scientific paper

A mathematical model is presented for perturbations of large-scale ionospheric fields due to solar flares on Ez variations near the earth surface at high latitudes. It is shown that the contribution of a magnetospheric source to the diurnal Ez variations can reach 50-55 percent of the contribution of UT variations of the ionospheric potential. The asymmetry of the diurnal variation of Ez changes not only as a function of magnetic activity and latitude but also as a function of the longitude of the observatory.

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