Delay in the escape of high energy solar protons into interplanetary space

Details Delay in the escape of high energy solar protons into interplanetary space Delay in the escape of high energy solar protons into interplanetary space

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kosis..23..748v&link_type=abstract

(Kosmicheskie Issledovaniia, vol. 23, Sept.-Oct. 1985, p. 748-753) Cosmic Research (ISSN 0010-9525), vol. 23, no. 5, March 1986,

Physics

1

Energetic Particles, Interplanetary Space, Solar Protons, Time Lag, High Energy Interactions, Interplanetary Magnetic Fields, Lines Of Force, Particle Acceleration, Solar Atmosphere, Solar Flares

Scientific paper

The first measurements which drew attention to a delay in the arrival of high-energy solar protons at the earth were measurements by ground neutron monitors. In space, the delay of high-energy solar protons was first discovered by the Prognoz-2 satellite for the solar event on August 7, 1972. Measurements of the delay in the arrival of energetic protons at the earth have yielded identical values for the mean delay time (10-20 min) whether the particles from solar flares have been recorded by neutron monitors or by satellite. For flares on the western hemisphere of the sun, the value of the time delay is independent of the flare longitude.

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