Delay in the arrival of high-energy protons from the solar flare of April 29, 1973

Details Delay in the arrival of high-energy protons from the solar flare of April 29, 1973 Delay in the arrival of high-energy protons from the solar flare of April 29, 1973

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978kosis..16...58v&link_type=abstract

(Kosmicheskie Issledovaniia, vol. 16, Jan.-Feb. 1978, p. 58-63.) Cosmic Research, vol. 16, no. 1, July 1978, p. 45-49. Translat

Physics

Proton Energy, Satellite Observation, Solar Flares, Solar Protons, Solar Wind Velocity, Ion Injection, Particle Telescopes, Solar Corona, Solar Physics, Trapped Particles

Scientific paper

The paper deals with a flare of importance, 2 B, which occurred in McMath 12322. Protons with energies between 100 and 500 MeV, recorded onboard the Prognoz 3 satellite were estimated to be retarded by approximately 40 min. In the present paper, the retardation is attributed either to containment of the accelerated particles in the solar corona, or to containment in a magnetic trap formed by magnetohydrodynamic shock waves originating from preceding flares.

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