Coronal propagation of solar flare particles observed by satellite

Details Coronal propagation of solar flare particles observed by satellite Coronal propagation of solar flare particles observed by satellite

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..301k&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 301-304 (SEE N85-34729 23-92)

Physics

Particle Diffusion, Solar Corona, Solar Cosmic Rays, Solar Flares, Interplanetary Magnetic Fields, Interplanetary Medium, Interplanetary Space, Models, Scattering

Scientific paper

Propagation of solar flare particles in corona was studied using the satellite data at the geostationary orbit. by selecting very fast rise time events only, the interplanetary propagation were assumed to be scatter free arrival. The results show that the propagation in corona does not depend on particle energy in 4 to 500 MeV protons, and the time delays from optical flare do not depend on the distance between the flare site and the base of the interplanetary magnetic field which connects to the Earth.

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