Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998a%26a...330..381c&link_type=abstract
Astronomy and Astrophysics, v.330, p.381-388 (1998)
Astronomy and Astrophysics
Astrophysics
6
Shock Waves, Acceleration Of Particles, Magnetic Fields, Interplanetary Medium
Scientific paper
We analyse the behaviour of protons reflected off supercritical, quasi-parallel shock waves in the presence of large amplitude magnetic field fluctuations with a magnetic field compression larger than the background magnetic field (1 <= Delta B/B_0 <= 2.5). These so-called SLAMS (short large-amplitude magnetic field structures) have originally been observed in the quasi-parallel region of the earth's bow shock. In general, the characteristics of the particle motion depend on the amplitude, the phase and the propagation direction of the SLAMS convected back to the shock front. Numerically calculated test particle trajectories show that in case of small gyroradii these dependencies reduce to pure geometrical conditions. In this case the computations can be simplified using results from adiabatic theory. Furthermore, it can be seen that the presence of SLAMS prevents the reflected ions from escaping into the upstream region of the shock. Although the shock geometry is quasi-parallel, some of the upstream moving ions return back to the shock front and subsequently penetrate into the downstream region. Because of their reflection at the incoming SLAMS these ions have a larger energy than their starting energy and can thus contribute to downstream heating and thermalisation. As a possible application we present an interpretation of cold ion bunches observed in connection with supercritical, quasi-parallel shock waves.
Classen H.-T.
Mann Gottfried
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