Auger electrons in bombardment of the upper atmosphere by an X-ray pulse

Details Auger electrons in bombardment of the upper atmosphere by an X-ray pulse Auger electrons in bombardment of the upper atmosphere by an X-ray pulse

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977kosis..15..313a&link_type=abstract

Kosmicheskie Issledovaniia, vol. 15, Mar.-Apr. 1977, p. 313-315. In Russian.

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Auger Effect, Electron Energy, Photoelectrons, Upper Atmosphere, X Ray Irradiation, Electron Energy, Nitrogen, Oxygen, Point Sources, Spectral Energy Distribution

Scientific paper

The influence exerted by the Auger effect on the spectral distribution of photoelectrons generated as a burst of X-ray emission impinges on the outer atmosphere is estimated by considering a prompt point source at a height 400 km up with an isotropic initial Planck spectral distribution and effective radiation temperature 1 keV. Computational results were narrowed down near the K-absorption edges at 23 A for oxygen and at 31 A for nitrogen (maximum Auger cross sections). The Auger electron energies fall within narrow ranges of 315-367 eV for nitrogen and 456-509 eV for oxygen.

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