Previous studies of the non-linear regime of the magnetorotational instability in one particular type of shearing box model - unstratified with no net magnetic flux - find that without explicit dissipation (viscosity and resistivity) the saturation amplitude decreases with increasing numerical resolution. We show that this result is strongly dependent on the vertical aspect ratio of the computational domain Lz/Lx. When Lz/Lx ≲ 1, we recover previous results. However when the vertical domain is extended Lz/Lx ≳ 2.5, we find the saturation level of the stress is greatly increased (giving a ratio of stress to pressure α ≳ 0.1), and moreover the results are independent of numerical resolution. Consistent with previous results, we find that satu...
Aims. This letter investigates the transport properties of MHD turbulence induced by the magnetorot...
Context. Strongly stratified hydromagnetic turbulence has previously been found to produce magnetic ...
We investigate magnetohydrodynamic turbulence driven by the magnetorotational instability (MRI) in K...
The magnetorotational instability (MRI) is an important process in sufficiently ionized accretion di...
Numerical simulations of the magnetorotational instability (MRI) with zero initial net flux in a non...
Aims.We study the influence of the choice of transport coefficients (viscosity and resistivity) on M...
International audienceMagnetohydrodynamic turbulence driven by the magnetorotational instability can...
International audienceMagnetohydrodynamic turbulence driven by the magnetorotational instability can...
Global three-dimensional magnetohydrodynamic (MHD) simulations of turbulent accretion disks are pres...
Aims.We study the properties of MHD turbulence driven by the magnetorotational instability (MRI) in ...
The saturation level of the magnetorotational instability (MRI) is investigated using three-dimensio...
We present a numerical study of turbulence and dynamo action in stratified shearing boxes with both ...
The magneto-rotational instability (MRI) is one of the most important processes in sufficiently ioni...
Context. MHD turbulence is known to exist in shearing boxes with either zero or nonzero net magnetic...
We study the saturation near threshold of the axisymmetric magnetorotational instability (MRI) of a ...
Aims. This letter investigates the transport properties of MHD turbulence induced by the magnetorot...
Context. Strongly stratified hydromagnetic turbulence has previously been found to produce magnetic ...
We investigate magnetohydrodynamic turbulence driven by the magnetorotational instability (MRI) in K...
The magnetorotational instability (MRI) is an important process in sufficiently ionized accretion di...
Numerical simulations of the magnetorotational instability (MRI) with zero initial net flux in a non...
Aims.We study the influence of the choice of transport coefficients (viscosity and resistivity) on M...
International audienceMagnetohydrodynamic turbulence driven by the magnetorotational instability can...
International audienceMagnetohydrodynamic turbulence driven by the magnetorotational instability can...
Global three-dimensional magnetohydrodynamic (MHD) simulations of turbulent accretion disks are pres...
Aims.We study the properties of MHD turbulence driven by the magnetorotational instability (MRI) in ...
The saturation level of the magnetorotational instability (MRI) is investigated using three-dimensio...
We present a numerical study of turbulence and dynamo action in stratified shearing boxes with both ...
The magneto-rotational instability (MRI) is one of the most important processes in sufficiently ioni...
Context. MHD turbulence is known to exist in shearing boxes with either zero or nonzero net magnetic...
We study the saturation near threshold of the axisymmetric magnetorotational instability (MRI) of a ...
Aims. This letter investigates the transport properties of MHD turbulence induced by the magnetorot...
Context. Strongly stratified hydromagnetic turbulence has previously been found to produce magnetic ...
We investigate magnetohydrodynamic turbulence driven by the magnetorotational instability (MRI) in K...