Behavior of the ionosphere in the region of the main ionospheric trough during magnetic disturbances

Details Behavior of the ionosphere in the region of the main ionospheric trough during magnetic disturbances Behavior of the ionosphere in the region of the main ionospheric trough during magnetic disturbances

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ge%26ae..25..211g&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 25, Mar.-Apr. 1985, p. 211-218. In Russian.

Computer Science

F Region, Ionospheric Disturbances, Ionospheric Electron Density, Magnetic Storms, Solar Activity Effects, Troughs, Interplanetary Magnetic Fields, Magnetic Disturbances, Solar Wind

Scientific paper

Data from the network of ionospheric stations in the Northern Hemisphere are used to investigate the behavior of the ionosphere in the region of the main trough during three magnetic storms during 1979-1980. A number of distinctive features in the behavior of the trough are identified, including the correlation of the motion of the equatorial wall with the Bz component of the interplanetary magnetic field. It is hypothesized that the rotational discontinuity of the solar wind affects the behavior of the main ionospheric trough.

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