Propagation of solar cosmic radiation from the October 3, 1971 and September 1, 1971 solar flares, based on Kosmos-426 satellite data

Details Propagation of solar cosmic radiation from the October 3, 1971 and September 1, 1971 solar flares, based on Kosmos-426 satellite data Propagation of solar cosmic radiation from the October 3, 1971 and September 1, 1971 solar flares, based on Kosmos-426 satellite data

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975kosis..13..844k&link_type=abstract

Kosmicheskie Issledovaniia, vol. 13, Nov.-Dec. 1975, p. 844-850. In Russian.

Physics

Cosmos Satellites, Proton Flux Density, Solar Cosmic Rays, Solar Flares, Solar Protons, Particle Diffusion, Particle Trajectories, Satellite-Borne Instruments

Scientific paper

Propagation of solar flare protons detected by Kosmos-426 satellite instruments is discussed. A model providing a long-lived source of particles observable from the earth's environs: a jam-packed force tube generating a flare corotating with the sun - is proposed. The data on the two flares show different time variations of intensity at more or less equal distances from the sun-earth line of force. A diffusion model postulating uniform diffusion followed by isotropic diffusion, and accounting for rotation of a particle-filled centroid, is proposed.

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