Interaction of a thin shock with turbulence. I. Effect on shock structure: Analytic model
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作者:
Ao, Xianzhi
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Univ Calif Riverside, Dept Phys, Riverside, CA 92521 USA
Univ Calif Riverside, Inst Geophys & Planetary Phys, Riverside, CA 92521 USA
Ctr Space Plasma & Aeron Res, Huntsville, AL 35805 USAUniv Calif Riverside, Dept Phys, Riverside, CA 92521 USA
Ao, Xianzhi
[1
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Zank, Gary P.
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Univ Calif Riverside, Dept Phys, Riverside, CA 92521 USA
Univ Calif Riverside, Inst Geophys & Planetary Phys, Riverside, CA 92521 USA
Ctr Space Plasma & Aeron Res, Huntsville, AL 35805 USAUniv Calif Riverside, Dept Phys, Riverside, CA 92521 USA
Zank, Gary P.
[1
,2
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]
Pogorelov, Nikolai V.
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Univ Calif Riverside, Inst Geophys & Planetary Phys, Riverside, CA 92521 USA
Ctr Space Plasma & Aeron Res, Huntsville, AL 35805 USAUniv Calif Riverside, Dept Phys, Riverside, CA 92521 USA
Pogorelov, Nikolai V.
[2
,3
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Shaikh, Dastgeer
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Univ Calif Riverside, Inst Geophys & Planetary Phys, Riverside, CA 92521 USA
Ctr Space Plasma & Aeron Res, Huntsville, AL 35805 USAUniv Calif Riverside, Dept Phys, Riverside, CA 92521 USA
Shaikh, Dastgeer
[2
,3
]
机构:
[1] Univ Calif Riverside, Dept Phys, Riverside, CA 92521 USA
[2] Univ Calif Riverside, Inst Geophys & Planetary Phys, Riverside, CA 92521 USA
[3] Ctr Space Plasma & Aeron Res, Huntsville, AL 35805 USA
A two-dimensional magnetohydrodynamical model describing the interaction of thin shock waves with turbulence is developed by adopting a multiscale perturbation analysis. The interaction is found to be governed by a two-dimensional inviscid Burgers' equation that includes "perturbation terms." Initially prescribed perturbation profiles are explored with numerical simulations to show how the shock front is modified by turbulence. Our numerical simulations show that magnetic field perturbations play a very important role in modifying the structure of perpendicular and parallel shocks. While turbulence can balance the nonlinear steepening of a shock wave at some regions, it can also help to create a larger jump in physical quantities such as the magnetic field at other regions. The plasma medium in these regions can therefore experience a higher compression, which will result in a downstream state that differs from the usual Rankine-Hugoniot state. (C) 2008 American Institute of Physics. [DOI:10.1063/1.3041706]
机构:
Univ Paris Cite, Univ Paris Saclay, CEA, AIM,CNRS, F-91191 Gif Sur Yvette, FranceUniv Paris Cite, Univ Paris Saclay, CEA, AIM,CNRS, F-91191 Gif Sur Yvette, France
机构:
Johns Hopkins Univ, Baltimore, MD 21218 USA
Los Alamos Natl Lab, Theoret Div CNLS T 5, Los Alamos, NM 87545 USAJohns Hopkins Univ, Baltimore, MD 21218 USA