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20162026
most citedMRI turbulence in accretion discs at large magnetic Prandtl numbers

20 citations · 133 across the 24 of their papers we have counts for

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physics.flu-dyn2026

Magnetic Dynamo Driven by Inertial Waves

A. Mishra, G. Mamatsashvili, M. Le Bars +2

We demonstrate, by studying precession-driven flows, that inertial wave hydrodynamic turbulence can drive a robust magnetic dynamo action. Motivated by the stronger damping of larg…

physics.flu-dyn2025

The effect of split endcaps on the flow dynamics in a tall Taylor-Couette setup

A. Mishra, P. Personnettaz, G. Mamatsashvili +2

The effects of axial boundaries, or endcaps are of fundamental interest in many Taylor-Couette (TC) flow experiments. A main challenge in those experiments has been to minimize the…

physics.flu-dyn2025

Strong and weak dynamo regimes in Taylor-Couette flows

A. Mishra, G. Mamatsashvili, F. Stefani

We reveal a nonlinear magnetic dynamo in a Taylor-Couette flow at small magnetic Prandtl numbers , which has been previously believed to exist only at higher $Pm\gtrsim 1…

physics.flu-dyn2023★ 1 cited

Dynamo action driven by precessional turbulence

V. Kumar, F. Pizzi, G. Mamatsashvili +3

We reveal and analyze an efficient magnetic dynamo action due to precession-driven hydrodynamic turbulence in the local model of a precessional flow, focusing on the kinematic stag…

physics.flu-dyn2023★ 1 cited

Non-axisymmetric modes of magnetorotational and possible hydrodynamical instabilities in the upcoming DRESDYN-MRI experiments -- linear and nonlinear dynamics

A. Mishra, G. Mamatsashvili, F. Stefani

The quest for an unambiguous detection of magnetorotational instability (MRI) in experiments is still ongoing despite recent promising results. To conclusively identify MRI in the…

physics.flu-dyn2022★ 2 cited

Nonlinear evolution of magnetorotational instability in a magnetized Taylor-Couette flow: scaling properties and relation to upcoming DRESDYN-MRI experiment

A. Mishra, G. Mamatsashvili, F. Stefani

Magnetorotational instability (MRI) is the most likely mechanism driving angular momentum transport in astrophysical disks. However, despite many efforts, a conclusive experimental…

physics.flu-dyn2022★ 14 cited

Interplay between geostrophic vortices and inertial waves in precession-driven turbulence

F. Pizzi, G. Mamatsashvili, A. J. Barker +2

The properties of rotating turbulence driven by precession are studied using direct numerical simulations and analysis of the underlying dynamical processes in Fourier space. The s…

physics.flu-dyn2021★ 1 cited

From helical to standard magnetorotational instability: predictions for upcoming liquid sodium experiments

A. Mishra, G. Mamatsashvili, F. Stefani

We conduct a linear analysis of axisymmetric magnetorotational instability (MRI) in a magnetized cylindrical Taylor-Couette (TC) flow for its standard version (SMRI) with a purely…

physics.flu-dyn2021★ 8 cited

Convective, absolute and global azimuthal magnetorotational instabilities

A. Mishra, G. Mamatsashvili, V. Galindo +1

We study the convective and absolute forms of azimuthal magnetorotational instability (AMRI) in a Taylor-Couette (TC) flow with an imposed azimuthal magnetic field. We show that th…

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.…

physics.flu-dyn2017★ 3 cited

Magnetic field dynamos and magnetically triggered flow instabilities

Frank Stefani, Thomas Albrecht, Rainer Arlt +13

The project A2 of the LIMTECH Alliance aimed at a better understanding of those magnetohydrodynamic instabilities that are relevant for the generation and the action of cosmic magn…