Physics
Scientific paper
May 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....95.6353m&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 95, May 1, 1990, p. 6353-6362.
Physics
15
Collisionless Plasmas, Plasma Heating, Plasma Waves, Shock Waves, Solar Terrestrial Interactions, Whistlers, Computerized Simulation, Equations Of State, Ion Acoustic Waves, Mach Number, Magnetohydrodynamics
Scientific paper
A simulation of quasi-parallel (QP) collisionless shock waves is used to deduce the dispersive and viscous scale lengths of QP shocks. The findings were found to be consistent with the observational results obtained by Scudder et al. (1984) and Kennel et al. (1984). It is shown that the upstream wavelength is the dispersive scale length which governs the magnetic-field structure of the shock. It is also shown that the two-stage ion heating obtained by Mandt and Kan (1988) is an intrinsic characteristic of the ion heating process in QP shocks.
Kan Joseph R.
Mandt M. E.
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