Transition to magnetorotational turbulence in Taylor-Couette flow with imposed azimuthal magnetic field

Guseva A, Willis AP, Hollerbach R, Avila M (2015)


Publication Type: Journal article

Publication year: 2015

Journal

Publisher: Institute of Physics Publishing

Book Volume: 17

Pages Range: 15p

Journal Issue: 9

DOI: 10.1088/1367-2630/17/9/093018

Abstract

The magnetorotational instability (MRI) is thought to be a powerful source of turbulence and momentum transport in astrophysical accretion discs, but obtaining observational evidence of its operation is challenging. Recently, laboratory experiments of Taylor-Couette flow with externally imposed axial and azimuthal magnetic fields have revealed the kinematic and dynamic properties of the MRI close to the instability onset. While good agreement was found with linear stability analyses, little is known about the transition to turbulence and transport properties of the MRI. We here report on a numerical investigation of the MRI with an imposed azimuthal magnetic field. We show that the laminar Taylor-Couette flow becomes unstable to a wave rotating in the azimuthal direction and standing in the axial direction via a supercritical Hopf bifurcation. Subsequently, the flow features a catastrophic transition to spatio-temporal defects which is mediated by a subcritical subharmonic Hopf bifurcation. Our results are in qualitative agreement with the PROMISE experiment and dramatically extend their realizable parameter range. We find that as the Reynolds number increases defects accumulate and grow into turbulence, yet the momentum transport scales weakly.

Authors with CRIS profile

Involved external institutions

How to cite

APA:

Guseva, A., Willis, A.P., Hollerbach, R., & Avila, M. (2015). Transition to magnetorotational turbulence in Taylor-Couette flow with imposed azimuthal magnetic field. New Journal of Physics, 17(9), 15p. https://doi.org/10.1088/1367-2630/17/9/093018

MLA:

Guseva, Anna, et al. "Transition to magnetorotational turbulence in Taylor-Couette flow with imposed azimuthal magnetic field." New Journal of Physics 17.9 (2015): 15p.

BibTeX: Download