Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3677m&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
Scientific paper
Particle acceleration at shocks and fluid compressions is examined by numerically solving pitch angle transport equations for various magnetic field angles. The recently discovered jump in the steady-state particle density just upstream of an oblique shock is much stronger for lower energy particles or greater shock obliquity. For narrow, oblique compressions the analogous feature is a peak in particle density in the compression region. We refer to both as "mirroring peaks" because for a compression we clearly see that the peak arises from magnetic mirroring and reflection of particles. Steady-state spectra of particles accelerated at an oblique shock or compression are hardened at low energy in association with the mirroring peak; magnetic mirroring leads to more effective acceleration. The spectral index at a given particle energy increases approximately linearly with compression width. Steady-state spectra from compression regions can also harden at high energy.
Chuychai Piyanate
Klappong Kamonporn
Leerungnavarat Kanokporn
Malakit K.
Ruffolo David
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