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相关论文: Magnetorotational instability in electrically driv…

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The dynamo instability is investigated in the limit of infinite magnetic Prandtl number. In this limit the fluid is assumed to be very viscous so that the inertial terms can be neglected and the flow is slaved to the forcing. The forcing…

流体动力学 · 物理学 2015-05-20 Alexandros Alexakis

The paper deals with a theoretical investigation of the peristaltic transport of a physiological fluid in a porous asymmetric channel under the action of a magnetic field. The stream function, pressure gradient and axial velocity are…

流体动力学 · 物理学 2010-06-04 J. C. Misra , S. Maiti , G. C. Shit

According to Rayleigh's criterion, rotating flows are linearly stable when their specific angular momentum increases radially outward. The celebrated magnetorotational instability opens a way to destabilize those flows, as long as the…

流体动力学 · 物理学 2015-11-23 Frank Stefani , Oleg N. Kirillov

We describe an instability of viscoelastic Couette-Taylor flow that is directly analogous to the magnetorotational instability (MRI) in astrophysical magnetohydrodynamics, with polymer molecules playing the role of magnetic field lines. By…

天体物理学 · 物理学 2009-06-23 Gordon I. Ogilvie , Adrian T. Potter

The linear stability of MHD Taylor-Couette flow of infinite vertical extension is considered for liquid sodium with its small magnetic Prandtl number Pm of order of 10^-5 and an uniform axial magnetic field. The sign of the constant a in…

天体物理学 · 物理学 2016-08-16 G. Rüdiger , M. Schultz , D. Shalybkov

We study the instability of a B\'enard layer subject to a vertical uniform magnetic field, in which the fluid obeys the Maxwell-Cattaneo (MC) heat flux-temperature relation. We extend the work of Bissell (Proc. R. Soc. A, 472: 20160649,…

流体动力学 · 物理学 2020-10-15 I. A. Eltayeb , D. W. Hughes , M. R. E. Proctor

Decades ago S. Lundquist, S. Chandrasekhar, P.H. Roberts and R. J.~Tayler first posed questions about the stability of Taylor-Couette flows of conducting material under the influence of large-scale magnetic fields. These and many new…

等离子体物理 · 物理学 2018-05-23 Günther Rüdiger , Marcus Gellert , Rainer Hollerbach , Manfred Schultz , Frank Stefani

The paper presents 3D numerical results for the laminar liquid metal flow in a rectangular duct compared with experimental results. It is shown that the magnetic interaction parameter $N$ is the main parameter governing the flow provided…

流体动力学 · 物理学 2009-01-06 E. V. Votyakov , E. Zienicke

The magnetorotational instability (MRI) in cylindrical Taylor-Couette flow with external helical magnetic field is simulated for infinite and finite aspect ratios. We solve the MHD equations in their small Prandtl number limit and confirm…

天体物理学 · 物理学 2008-11-26 Jacek Szklarski , Günther Rüdiger

We study the magnetorotational instability in cylindrical Taylor-Couette flow, with the (vertically unbounded) cylinders taken to be perfect conductors, and with externally imposed spiral magnetic fields. The azimuthal component of this…

天体物理学 · 物理学 2009-11-11 G. Ruediger , R. Hollerbach , M. Schultz , D. A. Shalybkov

The instability of a supercritical Taylor-Couette flow of a conducting fluid with resting outer cylinder under the influence of a uniform axial electric current is investigated for magnetic Prandtl number Pm=1. In the linear theory the…

流体动力学 · 物理学 2015-01-16 M. Gellert , G. Rüdiger

We consider a 2D incompressible and electrically conducting fluid in the domain $\mathbb{T}\times\mathbb{R}$. The aim is to quantify stability properties of the Couette flow $(y,0)$ with a constant homogenous magnetic field $(\beta,0)$ when…

偏微分方程分析 · 数学 2023-08-25 Michele Dolce

To find out whether toroidal field can stably exist in galaxies the current-driven instability of toroidal magnetic fields is considered under the influence of an axial magnetic field component and under the influence of both rigid and…

星系天体物理 · 物理学 2015-05-19 G. Ruediger , M. Schultz , D. Elstner

Flow-induced instabilities are relevant for the storage and dynamics of magnetic fields in stellar convection zones and possibly also in other astrophysical contexts. We continue the study started in the first paper of this series by…

天体物理学 · 物理学 2009-11-13 V. Holzwarth , D. Schmitt , M. Schuessler

The flow of an electrically conducting fluid driven by a traveling magnetic field imposed at the endcaps of a cylindrical annulus is numerically studied. At sufficiently large magnetic Reynolds number, the system undergoes a transition from…

流体动力学 · 物理学 2018-06-27 Sandeep R. Kanuganti , Stephan Fauve , Christophe Gissinger

We study the linear stability of weakly magnetized differentially rotating plasmas in both collisionless kinetic theory and Braginskii's theory of collisional, magnetized plasmas. We focus on the very weakly magnetized limit that is…

星系天体物理 · 物理学 2015-06-23 Eliot Quataert , Tobias Heinemann , Anatoly Spitkovsky

We report on a numerical study of axisymmetric flow of liquid metal in a circular duct with rectangular cross-section. The flow is forced through the combination of an axial magnetic field and a radial current. Sweeping a wide range of…

流体动力学 · 物理学 2020-04-08 A. Poyé , O. Agullo , N. Plihon , W. J. T. Bos , V. Desangles , G. Bousselin

We reveal and investigate a new type of linear axisymmetric helical magnetorotational instability which is capable of destabilizing viscous and resistive rotational flows with radially increasing angular velocity, or positive shear. This…

流体动力学 · 物理学 2019-10-23 G. Mamatsashvili , F. Stefani , R. Hollerbach , G. Rüdiger

The linear stability of MHD Taylor-Couette flows in axially unbounded cylinders is considered, for magnetic Prandtl number unity. Magnetic fields varying from purely axial to purely azimuthal are imposed, with a general helical field…

太阳与恒星天体物理 · 物理学 2015-05-14 G. Ruediger , M. Gellert , M. Schultz , R. Hollerbach

The magnetorotational instability (MRI) is considered to be one of the most powerful sources of turbulence in hydrodynamically stable quasi-Keplerian flows, such as those governing accretion disk flows. Although the linear stability of…

流体动力学 · 物理学 2017-11-21 A. Guseva , R. Hollerbach , A. P. Willis , M. Avila