Particle acceleration in modified oblique non-relativistic shocks

Details Particle acceleration in modified oblique non-relativistic shocks Particle acceleration in modified oblique non-relativistic shocks

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..264..177b&link_type=abstract

In: Particle acceleration in cosmic plasmas; Proceedings of the Workshop, Bartol Research Inst., Newark, DE, Dec. 4-6, 1991 (A93

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Cosmic Plasma, Nonrelativistic Mechanics, Oblique Shock Waves, Particle Acceleration, Shock Wave Interaction, Energetic Particles, Monte Carlo Method

Scientific paper

Previous applications of the Monte Carlo technique at the quasiparallel earth bow shock has motivated the extension of this technique to oblique shock geometries typical of those found in most astrophysical shock environments. In addition, such a generalization will permit the thorough examination of theoretical predictions of rapid acceleration times at quasi-perpendicular shocks. Therefore, we have embarked on the modification of our existing Monte Carlo code and in this paper outline the major technical aspects involved in developing a simulation of cosmic-ray acceleration at modified oblique nonrelativistic shocks.

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