The building of planetary systems is controlled by the gas and dust dynamics of
protoplanetary disks. While the gas is simultaneously accreted onto the central star and …

The effect of large magnetic Prandtl number Pm (the ratio of viscosity to resistivity) on the
turbulent transport and energetics of the magnetorotational instability (MRI) is poorly …

The evolution of the magnetic field from the large-scale dynamo is considered a central
feature of the accretion disk around a black hole. The resulting low-frequency oscillations …

Abstract The Kelvin–Helmholtz instability (KHI) is a standard test of hydrodynamic and
magnetohydrodynamic (MHD) simulation codes and finds many applications in …

We investigate sustenance and dependence on magnetic Prandtl number (Pm) for
magnetorotational instability (MRI)-driven turbulence in Keplerian disks with zero net …

Context. Angular momentum transport in accretion discs is often believed to be due to
magnetohydrodynamic turbulence mediated by the magnetorotational instability (MRI) …

We use high-resolution direct numerical simulations to study the anisotropic contents of a
turbulent, statistically homogeneous flow with random transitions among multiple energy …

We revisit the linear magnetorotational instability (MRI) in a cylindrical model of an accretion
disc and uncover a number of attractive results overlooked in previous treatments. In …

The discovery of the first binary neutron star merger, GW170817, has spawned a plethora of
global numerical relativity simulations. These simulations are often ideal (with dissipation …

Active Modes and Dynamical Balances in MRI Turbulence of Keplerian Disks with a Net
Vertical Magnetic Field - IOPscience This site uses cookies. By continuing to use this site you …