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

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

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 axia...

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Bibliographic Details
Main Authors: A Guseva, A P Willis, R Hollerbach, M Avila
Format: Article
Language:English
Published: IOP Publishing 2015-01-01
Series:New Journal of Physics
Subjects:
magnetorotational instability
Taylor–Couette flow
MHD
Online Access:https://doi.org/10.1088/1367-2630/17/9/093018

Internet

https://doi.org/10.1088/1367-2630/17/9/093018

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