Alfvén wave collisions, the fundamental building block of plasma turbulence. II. Numerical solution
- Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa 52242 (United States)
- Department of Physics, University of Maryland, College Park, Maryland 20742-3511 (United States)
This paper presents the numerical verification of an asymptotic analytical solution for the nonlinear interaction between counterpropagating Alfvén waves, the fundamental building block of astrophysical plasma turbulence. The analytical solution, derived in the weak turbulence limit using the equations of incompressible MHD, is compared to a nonlinear gyrokinetic simulation of an Alfvén wave collision. The agreement between these methods signifies that the incompressible solution satisfactorily describes the essential dynamics of the nonlinear energy transfer, even under the weakly collisional plasma conditions relevant to many astrophysical environments.
- OSTI ID:
- 22227940
- Journal Information:
- Physics of Plasmas, Vol. 20, Issue 7; Other Information: (c) 2013 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 1070-664X
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
70 PLASMA PHYSICS AND FUSION TECHNOLOGY
79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
ALFVEN WAVES
ANALYTICAL SOLUTION
ASTROPHYSICS
ASYMPTOTIC SOLUTIONS
COLLISIONAL PLASMA
COMPARATIVE EVALUATIONS
DIFFERENTIAL EQUATIONS
ENERGY TRANSFER
MAGNETOHYDRODYNAMICS
NONLINEAR PROBLEMS
NUMERICAL ANALYSIS
NUMERICAL SOLUTION
PLASMA SIMULATION
PLASMA WAVES
TURBULENCE
79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
ALFVEN WAVES
ANALYTICAL SOLUTION
ASTROPHYSICS
ASYMPTOTIC SOLUTIONS
COLLISIONAL PLASMA
COMPARATIVE EVALUATIONS
DIFFERENTIAL EQUATIONS
ENERGY TRANSFER
MAGNETOHYDRODYNAMICS
NONLINEAR PROBLEMS
NUMERICAL ANALYSIS
NUMERICAL SOLUTION
PLASMA SIMULATION
PLASMA WAVES
TURBULENCE