Magnetorotational instability in liquid metal Couette flow

被引:64
作者
Noguchi, K
Pariev, VI
Colgate, SA
Beckley, HF
Nordhaus, J
机构
[1] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[2] New Mexico Inst Min & Technol, Dept Phys, Socorro, NM 87801 USA
[3] Univ Rochester, Dept Phys & Astron, Rochester, NY 14627 USA
[4] PN Lebedev Phys Inst, Moscow 117924, Russia
关键词
accretion; accretion disks; instabilities; MHD; plasmas;
D O I
10.1086/341502
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Despite the importance of the magnetorotational instability (MRI) as a fundamental mechanism for angular momentum transport in magnetized accretion disks, it has yet to be demonstrated in the laboratory. A liquid sodium ! dynamo experiment at the New Mexico Institute of Mining and Technology provides an ideal environment to study the MRI in a rotating metal annulus ( Couette flow). A local stability analysis is performed as a function of shear, magnetic field strength, magnetic Reynolds number, and turbulent Prandtl number. The latter takes into account the minimum turbulence induced by the formation of an Ekman layer against the rigidly rotating end walls of a cylindrical vessel. Stability conditions are presented, and unstable conditions for the sodium experiment are compared with another proposed MRI experiment with liquid gallium. Because of the relatively large magnetic Reynolds number achievable in the sodium experiment, it should be possible to observe the excitation of the MRI for a wide range of wavenumbers and to further observe the transition to the turbulent state.
引用
收藏
页码:1151 / 1162
页数:12
相关论文
共 50 条
[41]   3D NUMERICAL STUDY OF MAGNETOHYDRODYNAMIC INSTABILITY IN LIQUID METAL TAYLOR-COUETTE FLOW [J].
Merah, A. ;
Mokhtari, F. ;
Bouabdallah, A. ;
Adnane, M. .
TOPICAL PROBLEMS OF FLUID MECHANICS 2015, 2015, :145-150
[42]   ROLE OF THE HALL EFFECT ON THE MAGNETOROTATIONAL INSTABILITY [J].
Bejarano, Cecilia ;
Gomez, Daniel .
INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2010, 19 (06) :695-700
[43]   Quasi-global galactic magnetorotational instability with Braginskii viscosity [J].
Rosin, M. S. ;
Mestel, A. J. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 425 (01) :74-86
[44]   Radiative heat conduction and the magnetorotational instability [J].
Araya-Góchez, RA ;
Vishniac, ET .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2004, 355 (02) :345-351
[45]   The effect of resistivity on the nonlinear stage of the magnetorotational instability in accretion disks [J].
Fleming, TP ;
Stone, JIM ;
Hawley, JF .
ASTROPHYSICAL JOURNAL, 2000, 530 (01) :464-477
[46]   Nonlinear evolution of the magnetorotational instability in ion-neutral disks [J].
Hawley, JF ;
Stone, JM .
ASTROPHYSICAL JOURNAL, 1998, 501 (02) :758-771
[47]   Saturation and thermalization of the magnetorotational instability: Recurrent channel flows and reconnections [J].
Sano, T ;
Inutsuka, S .
ASTROPHYSICAL JOURNAL, 2001, 561 (02) :L179-L182
[49]   Magnetorotational instability in diamagnetic, misaligned protostellar discs [J].
Devlen, Ebru ;
Ulubay, Ayse ;
Pekunlu, E. Rennan .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2020, 491 (04) :5481-5488
[50]   AXISYMMETRIC MAGNETOROTATIONAL INSTABILITY IN VISCOUS ACCRETION DISKS [J].
Masada, Youhei ;
Sano, Takayoshi .
ASTROPHYSICAL JOURNAL, 2008, 689 (02) :1234-1243