Interplanetary acceleration of energetic particles at 1 and 5 AU

Details Interplanetary acceleration of energetic particles at 1 and 5 AU Interplanetary acceleration of energetic particles at 1 and 5 AU

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..85...99m&link_type=abstract

Astrophysics and Space Science, vol. 85, no. 1-2, July 1982, p. 99-120. Research supported by the Science Research Council, Bri

Astronomy and Astrophysics

Astrophysics

9

Energetic Particles, Interplanetary Medium, Particle Acceleration, Computerized Simulation, Diffusion Coefficient, Interplanetary Magnetic Fields, Kinetic Energy, Particle Trajectories

Scientific paper

Energetic particle (0.1 to 100 MeV protons) acceleration is investigated on the basis of high-resolution IMF and plasma measurements at 1 AU (HEOS 2) and at 5 AU (Pioneer 10). It is shown that considerable particle acceleration occurs throughout the interplanetary medium, both in the corotating interaction regions (5 AU) and in quiet regions (1 AU). Although shocks may contribute to acceleration, it is suggested that statistical acceleration within corotating interaction regions is sufficient to explain most energetic particle observations.

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