Numerical Study of the Magnetorotational Instability in Princeton MRI Experiment
arXiv:0804.0044 · doi:10.1086/590366
Abstract
In preparation for an experimental study of magnetorotational instability (MRI) in liquid metal, we present non-ideal axisymmetric magnetohydrodynamic simulations of the nonlinear evolution of MRI in the experimental geometry. The simulations adopt fully insulating boundary conditions. No-slip conditions are imposed at the cylinders. A clear linear phase is observed with reduced linear growth rate. MRI results in an inflowing "jet" near the midplane and enhances the angular momentum transport at saturation.
22 pages, 12 figures, ApJ 684, 515 (2008). Minor changes according to referee's report
References in corpus (10)
- Hydrodynamic turbulence cannot transport angular momentum effectively in astrophysical disks
- Experimental observation and characterization of the magnetorotational instability
- Experimental evidence for magnetorotational instability in a helical magnetic field
- Helical Magnetorotational Instability in Magnetized Taylor-Couette Flow
- Experiments on the magnetorotational instability in helical magnetic fields
- A weakly nonlinear analysis of the magnetorotational instability in a model channel flow
- Traveling waves in magnetized Taylor-Couette flow
- On the nonlinear saturation of the magnetorotational instability near threshold in a thin-gap Taylor-Couette setup
- Magnetized Ekman Layer and Stewartson Layer in a Magnetized Taylor-Couette Flow
- Reduction of boundary effects in spiral MRI experiment PROMISE
Cited by in corpus (4)
- Magnetohydrodynamic experiments on cosmic magnetic fields
- Numerical simulations of the Princeton magneto-rotational instability experiment with conducting axial boundaries
- Taylor-Couette flow for astrophysical purposes
- Quasi-two-dimensional nonlinear evolution of helical magnetorotational instability in a magnetized Taylor-Couette flow