Abstract Electron density profiles measured by the EISCAT incoherent scatter radar are used to derive the Hall- and Pedersen conductances and the characteristic energy of the incoming particles during events of strong particle precipitation. A relationship is sought between the Hall- to Pedersen conductance ratio, R, and the root mean square energy, Erms, which can be expressed by: where A and B are constants to be determined in the text.
EISCAT studies of the auroral ionosphere conductances
Advances in Space Research ; 9 , 5 ; 35-38
1989-01-01
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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