Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003jgra..108.1295d&link_type=abstract
Journal of Geophysical Research Space Physics, Volume 108, Issue A7, pp. SSH 8-1, CiteID 1295, DOI 10.1029/2002JA009571
Physics
4
Interplanetary Physics: Mhd Waves And Turbulence, Interplanetary Physics: Plasma Waves And Turbulence, Interplanetary Physics: Solar Wind Plasma, Magnetospheric Physics: Mhd Waves And Instabilities
Scientific paper
We investigate the structure of nonlinear stationary waves propagating transverse and obliquely to the magnetic field in a cold plasma consisting of two ion populations, protons and alpha particles. By using the constants of motion which follow from the multifluid equations, the system may be described by a single first-order differential equation for the transverse case and four coupled first-order differential equations in the case of oblique propagation. In the transverse case solitons exist if the wave speed lies between the Alfven speed, based on the total mass density, and the Alfven speed modified by the density and charge ratios. At speeds in excess of this latter velocity, periodic solutions exist in which protons and alphas gyrate around each other. An analog of Rankine-Hugoniot type relations for the amplitude of the solitons and periodic waves is found for structures propagating transverse to the magnetic field. In the case of an oblique stationary wave it is shown that the tip of the proton (alpha ion) flow velocity vector moves on the surface of a sphere whose radius is determined only by the obliquity and the wave speed. Soliton solutions representing both compressions and rarefactions in the ion fluids exist in specific windows in the ``Alfven Mach number-obliquity'' space. In other windows, solutions characterized by both oscillating and soliton properties (``oscillitons'') exist. Critical Mach numbers and critical propagation angles limit the size of the windows in which smooth solitons can be constructed.
Chanteur Gerard
Dubinin Edik
McKenzie James F.
Sauer Ken
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