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...
Príomhchruthaitheoirí: | Latter, H, Lesaffre, P, Balbus, S |
---|---|
Formáid: | Journal article |
Teanga: | English |
Foilsithe / Cruthaithe: |
2009
|
Míreanna comhchosúla
Míreanna comhchosúla
-
A comparison of local simulations and reduced models of MRI-induced turbulence
de réir: Lesaffre, P, et al.
Foilsithe / Cruthaithe: (2009) -
The effects of Prandtl number on black hole accretion flows
de réir: Balbus, S, et al.
Foilsithe / Cruthaithe: (2008) -
Exact shearing box solutions of magnetohydrodynamic flows with resistivity, viscosity and cooling
de réir: Lesaffre, P, et al.
Foilsithe / Cruthaithe: (2007) -
Inertial waves near corotation in three-dimensional hydrodynamical discs
de réir: Latter, H, et al.
Foilsithe / Cruthaithe: (2009) -
The tachocline and differential rotation in the Sun
de réir: Balbus, S, et al.
Foilsithe / Cruthaithe: (2010)