Mapping of the auroral oval to the tail

Details Mapping of the auroral oval to the tail Mapping of the auroral oval to the tail

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991esasp.330..113g&link_type=abstract

In ESA, Cluster Dayside Polar Cusp p 113-117 (SEE N92-26294 17-46)

Mathematics

Flux Density, Geomagnetic Tail, Magnetic Fields, Magnetic Storms, Mapping, Auroral Zones, Earth Ionosphere, Mathematical Models, Satellite Observation

Scientific paper

Three different cases of mapping between the ionosphere and the magnetotail are discussed. It has become possible to use multisatellite measurements to study auroral substorms. Global satellite images of the auroral can be combined with simultaneous particle and field measurements at geosynchronous altitude and in the magnetotail. The main tool to relate observations on different regions of the magnetosphere is a magnetic field model and it is, therefore, of crucial importance in studies of substorm phenomena. These studies indicate the development of and the need for further improvements for the auroral source regions in the tail.

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