MRI channel flows and their parasites
Local simulations of the magnetorotational instability (MRI) in accretion discs can exhibit recurrent coherent structures called channel flows. The formation and destruction of these structures may play a role in the development and saturation of MRI-induced turbulence, and consequently help us unde...
Hauptverfasser: | Latter, H, Lesaffre, P, Balbus, S |
---|---|
Format: | Journal article |
Sprache: | English |
Veröffentlicht: |
2009
|
Ähnliche Einträge
Ähnliche Einträge
-
A comparison of local simulations and reduced models of MRI-induced turbulence
von: Lesaffre, P, et al.
Veröffentlicht: (2009) -
The effects of Prandtl number on black hole accretion flows
von: Balbus, S, et al.
Veröffentlicht: (2008) -
Exact shearing box solutions of magnetohydrodynamic flows with resistivity, viscosity and cooling
von: Lesaffre, P, et al.
Veröffentlicht: (2007) -
Inertial waves near corotation in three-dimensional hydrodynamical discs
von: Latter, H, et al.
Veröffentlicht: (2009) -
The tachocline and differential rotation in the Sun
von: Balbus, S, et al.
Veröffentlicht: (2010)