Semiempirical method for calculating stationary photoelectron fluxes

Details Semiempirical method for calculating stationary photoelectron fluxes Semiempirical method for calculating stationary photoelectron fluxes

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kosis..26..406k&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 26, May-June 1988, p. 406-412. In Russian.

Computer Science

Electron Flux Density, Photoelectrons, Semiempirical Equations, Upper Atmosphere, Boltzmann Transport Equation, Photoelectron Spectroscopy

Scientific paper

A method for calculating stationary photoelectron fluxes in the upper atmosphere is proposed which involves the determination of the relative spectrum according to a 'reduced' photoelectron spectrum; the calculation of the absolute value of the flux for a fixed energy on the basis of an analytical formula obtained via energy integration of the Boltzmann equation; and the calculation of the fine structure of the photoelectron spectrum on the basis of an exact solution of the initial equation. Calculation results for heights of 150-350 km and a dependence of 7-9-eV fluxes on the solar zenith angle are compared with AE-E satellite measurements.

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