Flux instability of cosmic rays in the outer heliosphere

Details Flux instability of cosmic rays in the outer heliosphere Flux instability of cosmic rays in the outer heliosphere

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..401d&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, May-June 1991, p. 401-404. In Russian.

Physics

Energetic Particles, Galactic Cosmic Rays, Heliosphere, Magnetohydrodynamic Stability, Magnetohydrodynamic Waves, Relativistic Particles, Interplanetary Magnetic Fields, Particle Diffusion, Plasma Turbulence, Plasma-Particle Interactions, Solar Wind

Scientific paper

The paper presents a theoretical study of the kinetic flux instability of MHD waves arising in connection with the penetration of galactic cosmic rays into the heliosphere. It is shown that the turbulence level established in this case is, in principle, sufficient to cause the diffusion of particles with energies from 100 MeV to 10 GeV to distances of at least 40 AU from the sun.

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