High-energy (10 to the 7th to 10 to the 8th eV) secondary electrons in near-earth space

Details High-energy (10 to the 7th to 10 to the 8th eV) secondary electrons in near-earth space High-energy (10 to the 7th to 10 to the 8th eV) secondary electrons in near-earth space

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kosis..26..563g&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 26, July-Aug. 1988, p. 563-568. In Russian.

Physics

Earth Orbital Environments, High Energy Electrons, Primary Cosmic Rays, High Energy Interactions, Mesons, Radiation Belts, Stratosphere

Scientific paper

It is shown that, at altitudes up to 500-600 km, cosmic rays interact inelastically with the residual atmosphere, with the generation of pi(+/-) and K(+/-) mesons, whose decay yields high-energy electrons. When the density of the residual density is low, high-energy electrons are formed through the decay of radioactive fragments of cosmic-ray nuclei, generated through the interaction of primary nuclei in the stratosphere.

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