Physics
Scientific paper
Apr 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ge%26ae..33..156g&link_type=abstract
Geomagnetizm i Aeronomiya (ISSN 0016-7940), vol. 33, no. 2, p. 156-160.
Physics
Energy Spectra, Ionizing Radiation, Ionospheric Electron Density, Kinetic Equations, Solar Flares, High Energy Electrons, Plasma Dynamics
Scientific paper
A numerical solution of the nonstationary kinetic equation for photoelectrons, Auger electrons, and secondary electrons formed during an X-ray burst is obtained. At the initial stage of scattering (t = 0.01 s) energetic Auger electrons escape the atmosphere that are primarily formed in the 300-400-km altitude range. Subsequently (on time intervals of 0.1 s) the flux of escaping electrons is sustained by low-energy secondary electrons and photoelectrons.
Gefan Grigorii D.
Gorbachev O. A.
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