On reflecting boundary behind the Earth's orbit at propagation of fast particles from solar flares

Details On reflecting boundary behind the Earth's orbit at propagation of fast particles from solar flares On reflecting boundary behind the Earth's orbit at propagation of fast particles from solar flares

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4..368n&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 4 p 368-371 (SEE N85-34729 23-92)

Physics

Interplanetary Magnetic Fields, Shock Fronts, Shock Wave Propagation, Solar Cosmic Rays, Solar Flares, Earth Orbits, Interplanetary Medium, Particle Flux Density, Solar Protons, Solar Wind, Wave Reflection

Scientific paper

The flares of solar cosmic rays (SCR) associated with the presence of shocks in interplanetary magnetic field and with their propagation at significant heliocentric distances were always of great interest. Some events and problems concerning the peculiarities of propagation of flare CR in the interplanetary medium are considered. The distinguishing feature of such events is the presence of shock front behind the Earth's orbit having formed either directly in the process of shock generation on the Sun or at large heliocentric distances as a result of the interaction of fast and slow quasistationary recurrent solar wind (SW) streams. Based on the experimental material it is shown that the significant nonlinear disturbances in IMF behind the Earth's orbit can yield the occurrence of the additional SCR flux from shock front region as a result of the interaction of flare flux with shock and a partial reflection from it.

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