Simulating the ionospheric dynamo-I. Simulation model and flux tube integrated conductivities

Details Simulating the ionospheric dynamo-I. Simulation model and flux tube integrated conductivities Simulating the ionospheric dynamo-I. Simulation model and flux tube integrated conductivities

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jastp..61..913d&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 61, Issue 12, p. 913-923.

Physics

6

Scientific paper

An updated version of the equivalent circuit model for simulating the ionospheric dynamo process is described. The contributions of the E and F regions to the flux tube integrated conductivities are compared. The results confirm that the ionospheric electric process is controlled by the E region during daytime but by the F region during nighttime. The F region has a larger effect on the dynamo processes during solar maximum than at solar minimum, and during equinox than in solstice.

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