A non-Fermi model of cosmic ray acceleration - The Vector-V X Vector-B

Details A non-Fermi model of cosmic ray acceleration - The Vector-V X Vector-B A non-Fermi model of cosmic ray acceleration - The Vector-V X Vector-B

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....2...33p&link_type=abstract

In: International Cosmic Ray Conference, 16th, Kyoto, Japan, August 6-18, 1979, Conference Papers. Volume 2. (A81-12386 02-93) T

Computer Science

Cosmic Rays, Crossed Fields, Fermi Surfaces, Magnetic Flux, Particle Acceleration, Vector Dominance Model, Electric Fields, Interstellar Magnetic Fields, Magnetohydrodynamic Waves, Particle Collisions, Plasma Acceleration

Scientific paper

The Fermi model of cosmic ray acceleration is incomplete and frequently internally inconsistent in situations in which particles gradient B or curvature drift in a Vector-V x Vector-B electric field while interacting with moving magnetic field irregularities. In such situations particles can gain orders of magnitude more energy per reflection than predicted by the Fermi model.

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