Abstract In this paper the latest neutral and ionospheric models of the upper Martian atmosphere, created on the Viking data are used. For the calculations of the photoelectron spectra the Hinteregger's measurements of the solar flux together with the theoretical photoelectron distribution are also used.
Spectra of fresh photo-electrons in the Martian atmosphere
Advances in Space Research ; 1 , 8 ; 155-160
01.01.1981
6 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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