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20152017
most citedTransition to magnetorotational turbulence in Taylor--Couette flow with imposed azimuthal magnetic field

31 citations · 79 across the 5 of their papers we have counts for

collaborators

5 papers

physics.flu-dyn2017★ 24 cited

Dynamo Action in a Quasi-Keplerian Taylor-Couette Flow

Anna Guseva, Rainer Hollerbach, Ashley P. Willis +1

We numerically compute the flow of an electrically conducting fluid in a Taylor-Couette geometry where the rotation rates of the inner and outer cylinders satisfy $Ω_o/Ω_i=(r_o/r_i…

physics.flu-dyn2017★ 6 cited

Quasi-two-dimensional nonlinear evolution of helical magnetorotational instability in a magnetized Taylor-Couette flow

G. Mamatsashvili, F. Stefani, A. Guseva +1

Magnetorotational instability (MRI) is one of the fundamental processes in astrophysics, driving angular momentum transport and mass accretion in a wide variety of cosmic objects.…

astro-ph.SR2017★ 12 cited

Transport properties of the Azimuthal Magnetorotational Instability

Anna Guseva, Ashley P. Willis, Rainer Hollerbach +1

The magnetorotational instability (MRI) is thought to be a powerful source of turbulence in Keplerian accretion disks. Motivated by recent laboratory experiments, we study the MRI…

astro-ph.SR2016★ 6 cited

Nonaxisymmetric MHD instabilities of Chandrasekhar states in Taylor-Couette geometry

M. Gellert, G. Rüdiger, M. Schultz +2

We consider axially periodic Taylor-Couette geometry with insulating boundary conditions. The imposed basic states are so-called Chandrasekhar states, where the azimuthal flow $U_ϕ…

physics.flu-dyn2015★ 31 cited

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

A. Guseva, A. P. Willis, R. Hollerbach +1

The magnetorotational instability (MRI) is thought to be a powerful source of turbulence and momentum transport in astrophysical accretion discs, but obtaining observational eviden…