Published May 20, 2017 | Version v1
Journal article

The Weakly Nonlinear Magnetorotational Instability in a Global, Cylindrical Taylor–Couette Flow

  • 1. Department of Astronomy, Columbia University, New York, NY 10027 (United States)
  • 2. Department of Physics and Astronomy, Bates College, Lewiston, ME 04240 (United States)

Description

We conduct a global, weakly nonlinear analysis of the magnetorotational instability (MRI) in a Taylor–Couette flow. This is a multiscale, perturbative treatment of the nonideal, axisymmetric MRI near threshold, subject to realistic radial boundary conditions and cylindrical geometry. We analyze both the standard MRI, initialized by a constant vertical background magnetic field, and the helical MRI, with an azimuthal background field component. This is the first weakly nonlinear analysis of the MRI in a global Taylor–Couette geometry, as well as the first weakly nonlinear analysis of the helical MRI. We find that the evolution of the amplitude of the standard MRI is described by a real Ginzburg–Landau equation (GLE), whereas the amplitude of the helical MRI takes the form of a complex GLE. This suggests that the saturated state of the helical MRI may itself be unstable on long spatial and temporal scales.

Availability note (English)

Available from http://dx.doi.org/10.3847/1538-4357/aa6ff6

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
841
Journal Issue
1
Journal Page Range
[13 p.]
ISSN
0004-637X
CODEN
ASJOAB