A weakly nonlinear analysis of the magnetorotational instability in a model channel flow
arXiv:astro-ph/0608374 · doi:10.1103/PhysRevLett.98.034501
Abstract
We show by means of a perturbative weakly nonlinear analysis that the axisymmetric magnetorotational instability (MRI) of a viscous, resistive, incompressible rotating shear flow in a thin channel gives rise to a real Ginzburg-Landau equation for the disturbance amplitude. For small magnetic Prandtl number (), the saturation amplitude is and the resulting momentum transport scales as , where is the {\em hydrodynamic} Reynolds number. Simplifying assumptions, such as linear shear base flow, mathematically expedient boundary conditions and continuous spectrum of the vertical linear modes, are used to facilitate this analysis. The asymptotic results are shown to comply with numerical calculations using a spectral code. They suggest that the transport due to the nonlinearly developed MRI may be very small in experimental setups with .
arXiv commentAccepted to Physical Review Letters - Nov. 30, 2006. In final form
References in corpus (9)
- Enhanced Angular Momentum Transport in Accretion Disks
- Experimental observation and characterization of the magnetorotational instability
- Magnetorotational Instability in a Rotating Liquid Metal Annulus
- On magnetic field generation in Kolmogorov turbulence
- The onset of a small-scale turbulent dynamo at low magnetic Prandtl numbers
- Hydrodynamic stability of rotationally supported flows: Linear and nonlinear 2D shearing box results
- Magnetorotational Instability in Liquid Metal Couette Flow
- Turbulence and its parameterization in accretion discs
- Simulations of Magnetorotational Instability in a Magnetized Couette Flow
Cited by in corpus (28)
- Impact of dimensionless numbers on the efficiency of MRI-induced turbulent transport
- Aspect ratio dependence in magnetorotational instability shearing box simulations
- On the Saturation of the Magnetorotational Instability via Parasitic Modes
- Angular Momentum Transport in Protoplanetary and Black-Hole Accretion Disks: The Role of Parasitic Modes in the Saturation of MHD Turbulence
- On the viability of the shearing box approximation for numerical studies of MHD turbulence in accretion disks
- Dust Settling in Magnetorotationally-Driven Turbulent Discs I: Numerical Methods and Evidence for a Vigorous Streaming Instability
- Binary interactions with high accretion rates onto main sequence stars
- Transition to magnetorotational turbulence in Taylor--Couette flow with imposed azimuthal magnetic field
- On the nonlinear saturation of the magnetorotational instability near threshold in a thin-gap Taylor-Couette setup
- Local and global aspects of the linear MRI in accretion disks
- On the Anisotropic Nature of MRI-Driven Turbulence in Astrophysical Disks
- The weakly nonlinear magnetorotational instability in a local geometry
- Numerical Study of the Magnetorotational Instability in Princeton MRI Experiment
- Microphysical dissipation, turbulence and magnetic fields in hyper-accreting discs
- Growing pseudo-eigenmodes and positive logarithmic norms in rotating shear flows
- Stochastically driven instability in rotating shear flows
- The weakly nonlinear magnetorotational instability in a global, cylindrical Taylor-Couette flow
- Non-Dissipative Saturation of the Magnetorotational Instability in Thin Disks
- Turbulence in particle laden midplane layers of planet forming disks
- Origin of nonlinearity and plausible turbulence by hydromagnetic transient growth in accretion disks: Faster growth rate than magnetorotational instability
- Quasi-two-dimensional nonlinear evolution of helical magnetorotational instability in a magnetized Taylor-Couette flow
- Low magnetic-Prandtl number flow configurations for cold astrophysical disk models: speculation and analysis
- Hydrodynamical activity in thin accretion disks
- Resonant instability of the nonlinearly-saturated magnetorotational mode in thin Keplerian discs
- The Magneto-Rotational Decay Instability in Keplerian Disks
- Study of MRI in stratified viscous plasma configuration
- The magneto-rotational instability near threshold: spatio-temporal amplitude equation and saturation
- Explosive magnetorotational instability in Keplerian disks