Secondary electron fluxes by precipitating electrons and the excitation of the atmospheric constituents in the daytime at midlatitude

Details Secondary electron fluxes by precipitating electrons and the excitation of the atmospheric constituents in the daytime at midlatitude Secondary electron fluxes by precipitating electrons and the excitation of the atmospheric constituents in the daytime at midlatitude

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974jatp...36.1733v&link_type=abstract

(International Association of Geomagnetism and Aeronomy, Symposium on Dynamics, Chemistry and Thermal Processes in the Ionospher

Physics

Atmospheric Radiation, Electron Flux Density, Electron Precipitation, Midlatitude Atmosphere, Photoelectrons, Angular Distribution, Atmospheric Ionization, Daytime, Energy Spectra, Secondary Emission

Scientific paper

Secondary electron fluxes within the energy range 5 to 20 eV for precipitating electron fluxes with energy 1 to 40 keV are calculated. The precipitating electron flux is assumed to have an isotropic angular distribution. The maximum of secondary electron fluxes occur at an altitude of about 150 km with the exception of the secondary electron flux with the energy 18 eV. Below 150 km secondary electron fluxes with the energy range 10 to 18 eV dominate photoelectron fluxes. Production rates for various excited species by secondary electrons are included.

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