Abstract A method to determine parameters of precipitating auroral electrons with energy E > 10–30 keV producing the auroral absorption is presented. The variation of total electron flux and energy spectrum is examined during different phases of the substorm.
High-latitude plasma densities in the middle atmosphere and characteristics of precipitating electrons during an auroral absorption substorm
Advances in Space Research ; 13 , 4 ; 99-104
1993-01-01
6 pages
Article (Journal)
Electronic Resource
English
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