Determination of the transport mean free path and intensity of primary protons for different phases of solar cosmic-ray bursts

Details Determination of the transport mean free path and intensity of primary protons for different phases of solar cosmic-ray bursts Determination of the transport mean free path and intensity of primary protons for different phases of solar cosmic-ray bursts

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ge%26ae..14..192g&link_type=abstract

(Geomagnetizm i Aeronomiia, vol. 14, Mar.-Apr. 1974, p. 192-195.) Geomagnetism and Aeronomy, vol. 14, no. 2, 1974, p. 161-163. T

Physics

Mean Free Path, Proton Flux Density, Solar Cosmic Rays, Solar Flares, Solar Protons, Transport Properties, Particle Trajectories, Satellite Observation, Solar Flux Density, Venera 4 Satellite

Scientific paper

(Previously cited in issue 14, p. 2010, Accession no. A74-30852)

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