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NASA NTRS ยท 19890054024

Numerical studies of multiple-encounter shock drift acceleration

Abstract

Test particle simulation is performed to examine the mechanism previously proposed by Chiueh for particle acceleration by a nearly perpendicular shock where only downstream MHD turbulence is present. A nonnegligible fraction of low-energy particles is observed gaining energy by more than three orders of magnitude in a few hundred cyclotron periods. Criteria for effective acceleration given previously are examined and confirmed. The numerical results suggest that in the nonrelativistic energy range, a power-law particle energy spectrum, with the power index determined by the degree to which the criteria are satisfied, may form.

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BibTeXRIS

Chiueh, Tzihong. 1989-06-01. Numerical studies of multiple-encounter shock drift acceleration. https://ntrs.nasa.gov/citations/19890054024

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