most citedOn the viability of the shearing box approximation for numerical studies of MHD turbulence in accretion disks

56 citations

5 papers

astro-ph20082 cited

Linear dynamics of weakly viscous accretion disks: A disk analog of Tollmien-Schlichting waves

O. M. Umurhan, G. Shaviv

This paper discusses new perspectives and approaches to the problem of disk dynamics where, in this study, we focus on the effects of viscous instabilities influenced by boundary e…

astro-ph200814 cited

A shallow-water theory for annular sections of Keplerian Disks

O. M. Umurhan

A scaling argument is presented that leads to a shallow water theory of non-axisymmetric disturbances in annular sections of thin Keplerian disks. To develop a theoretical construc…

astro-ph200756 cited

On the viability of the shearing box approximation for numerical studies of MHD turbulence in accretion disks

O. Regev, O. M. Umurhan

Most of our knowledge on the nonlinear development of the magneto-rotational instability (MRI) relies on the results of numerical simulations employing the shearing box (SB) approx…

astro-ph20073 cited

Hydrodynamic response of rotationally supported flows in the Small Shearing Box model

A. Sternberg, O. M. Umurhan, Y. Gil +1

The hydrodynamic response of the inviscid small shearing box model of a midplane section of a rotationally supported astrophysical disk is examined. An energy functional

astro-ph200724 cited

On the nonlinear saturation of the magnetorotational instability near threshold in a thin-gap Taylor-Couette setup

O. M. Umurhan, O. Regev, K. Menou

We study the saturation near threshold of the axisymmetric magnetorotational instability (MRI) of a viscous, resistive, incompressible fluid in a thin-gap Taylor-Couette configurat…