The solar flux influence on quiet time conductances in the auroral ionosphere

Details The solar flux influence on quiet time conductances in the auroral ionosphere The solar flux influence on quiet time conductances in the auroral ionosphere

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993georl..20..971m&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 20, no. 10, p. 971-974.

Physics

38

Auroral Zones, Ionospheric Conductivity, Solar Flux, Solar Terrestrial Interactions, Atmospheric Models, Hall Effect

Scientific paper

Hall and Pedersen conductances derived from EISCAT Common Program 1 (CP-1) data during half a solar cycle are presented. The data set consists of nine quiet summer days with 10.7-cm solar flux ranging from solar minimum to solar maximum conditions. The solar flux and the solar zenith angle dependence of Hall and Pedersen conductances are well represented by given expressions. The results are in good agreement with the theoretical model calculations by Rasmussen et al. (1988) for solar minimum conditions. For higher solar activity levels, however, our model gives consistently higher conductance values than older models.

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