Particle acceleration at the bow shock front

Details Particle acceleration at the bow shock front Particle acceleration at the bow shock front

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kosis..29..582b&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 29, July-Aug. 1991, p. 582-592. In Russian.

Computer Science

Numerical Analysis

12

Bow Waves, Particle Acceleration, Protons, Shock Fronts, Solar Terrestrial Interactions, Energy Spectra, Numerical Analysis, Time Dependence, Alfven Waves Generation

Scientific paper

The quasi-linear problem of proton acceleration at the front of the bow shock in the region of solar wind/earth magnetosphere interaction is solved numerically. The temporal evolution of the acceleration is investigated. The main feature of this evolution is a nonmonotonic character of the acceleration: in intermediate time intervals the particle density and the Alfven wave energy can exceed their steady-state values.

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