Abstract The results from observations of auroral emissions within the wavelength band 115–135 nm are presented. The experiment was carried out on board the satellite “Cosmos-900”, launched on March 30, 1977, to an almost circular polar orbit. We assume that the precipitating fluxes of protons and electrons were the sources of excitation, according to the theory.
Observations of the aurora in the far ultraviolet from “Cosmos-900”
Advances in Space Research ; 1 , 12 ; 77-80
1981-01-01
4 pages
Article (Journal)
Electronic Resource
English
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