Relationship between the precipitation level of high-energy electrons and magnetic disturbances

Details Relationship between the precipitation level of high-energy electrons and magnetic disturbances Relationship between the precipitation level of high-energy electrons and magnetic disturbances

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26..958s&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, Nov.-Dec. 1986, p. 958-962. In Russian.

Physics

Auroral Zones, Electron Precipitation, High Energy Electrons, Magnetic Disturbances, Electron Flux Density, Polar Substorms

Scientific paper

A joint analysis of magnetic and riometer data indicates that the precipitation intensity of high-energy (e.g., 40-150 keV) electrons in the auroral zone is closely connected with the amplitude of midlatitude magnetic bays. The precipitations are insignificant during periods of quasi-stationary magnetic activity. The appearance of excess fluxes of high-energy electrons depends primarily on the 'switch-on' of the induction electric field during the explosive substorm phase.

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