Effect of the IMF on the daytime trough according to Cosmos-900 data

Details Effect of the IMF on the daytime trough according to Cosmos-900 data Effect of the IMF on the daytime trough according to Cosmos-900 data

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..865a&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, Sept.-Oct. 1989, p. 865-867. In Russian.

Computer Science

Sound

Atmospheric Ionization, Interstellar Magnetic Fields, Ionospheric Sounding, Troughs, Cosmos Satellites, Daytime, Diurnal Variations

Scientific paper

An analysis of Cosmos-900 data for 1978-1979 showed that ionization troughs in the postmidday sector are observed under arbitrary levels of magnetic activity. A dependence of the trough location on the IMF was found under quiet conditions: i.e., as the northward component of the IMF (Bz greater than 0) increases, the trough moves toward higher latitudes. This dependence is pronounced only when By is less than 0, and is no longer valid when By is greater than 0.

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