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We study the local stability of stratified, differentially-rotating fluids to axisymmetric perturbations in the presence of a weak magnetic field and of finite resistivity, viscosity and heat conductivity. This is a generalization of the…

天体物理学 · 物理学 2009-11-10 Kristen Menou , Steven A. Balbus , Henk C. Spruit

Global axisymmetric stability of viscous, resistive, magnetized Couette flow is re-examined, with the emphasis on flows that would be hydrodynamically stable according to Rayleigh's criterion: opposing gradients of angular velocity and…

天体物理学 · 物理学 2009-11-06 Jeremy Goodman , Hantao Ji

Aims. We investigate the impact of ambipolar diffusion on the development of the Rayleigh-Taylor instability (RTI) with an oblique magnetic field in the incompressible limit. Methods. We developed a general bi-fluid framework comprising…

星系天体物理 · 物理学 2025-06-25 E. Callies , V. Guillet , A. Marcowith , Z. Meliani , P. Lesaffre

We consider the effect of toroidal magnetic fields on hydrodynamically stable Taylor-Couette differential rotation flows. For current-free magnetic fields a nonaxisymmetric m=1 magnetorotational instability arises when the magnetic Reynolds…

天体物理学 · 物理学 2008-11-26 G. Ruediger , R. Hollerbach , M. Schultz , D. Elstner

We perform a local stability analysis of rotational flows in the presence of a constant vertical magnetic field and an azimuthal magnetic field with a general radial dependence. Employing the short-wavelength approximation we develop a…

流体动力学 · 物理学 2014-11-14 Oleg N. Kirillov , Frank Stefani , Yasuhide Fukumoto

The interaction of differential rotation and toroidal fields that are current-free in the gap between two corotating axially unbounded cylinders is considered. It is shown that nonaxisymmetric perturbations are unstable if the rotation rate…

太阳与恒星天体物理 · 物理学 2015-06-15 G. Ruediger , M. Gellert , M. Schultz , R. Hollerbach , F. Stefani

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

We study magnetic Taylor-Couette flow in a system having nondimensional radii $r_i=1$ and $r_o=2$, and periodic in the axial direction with wavelengths $h\ge100$. The rotation ratio of the inner and outer cylinders is adjusted to be…

流体动力学 · 物理学 2017-06-07 Rainer Hollerbach , Nigel Sibanda , Eun-jin Kim

The magnetohydrodynamic stability of axially unbounded cylindrical flows is considered which contain a toroidal magnetic background field with the same radial profile as the linear azimuthal velocity. Chandrasekhar (1956) has shown for…

星系天体物理 · 物理学 2015-09-30 Guenther Ruediger , Manfred Schultz , Frank Stefani , Michael Mond

The stability of dissipative Taylor-Couette flows with an axial stable density stratification and a prescribed azimuthal magnetic field is considered. Global nonaxisymmetric solutions of the linearized MHD equations with toroidal magnetic…

天体物理学 · 物理学 2009-11-13 G. Ruediger , D. A. Shalybkov

It is demonstrated that the azimuthal magnetorotational instability (AMRI) also works with radially increasing rotation rates contrary to the standard magnetorotational instability for axial fields which requires negative shear. The…

流体动力学 · 物理学 2017-12-14 Guenther Rüdiger , Manfred Schultz , Marcus Gellert , Frank Stefani

This paper presents the analysis of axisymmetric helical magnetorotational instability (HMRI) in the inviscid limit, which is relevant for astrophysical conditions. The inductionless approximation defined by zero magnetic Prandtl number is…

流体动力学 · 物理学 2011-12-20 Jānis Priede

We consider a differentially rotating flow of an incompressible electrically conducting and viscous fluid subject to an external axial magnetic field and to an azimuthal magnetic field that is allowed to be generated by a combination of an…

流体动力学 · 物理学 2021-11-01 Rong Zou , Joris Labarbe , Yasuhide Fukumoto , Oleg N. Kirillov

The magnetorotational instability (MRI) is thought to be a powerful source of turbulence and momentum transport in astrophysical accretion discs, but obtaining observational evidence of its operation is challenging. Recently, laboratory…

流体动力学 · 物理学 2015-09-15 A. Guseva , A. P. Willis , R. Hollerbach , M. Avila

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

The possibility that the magnetic shear-flow instability (MRI, Balbus-Hawley instability) might give rise to turbulence in a cylindric Couette flow is investigated through numerical simulations. The study is linear and the fluid flow is…

天体物理学 · 物理学 2009-11-06 G. Rüdiger , Y. Zhang

We investigate the linear stability of a sinusoidal shear flow with an initially uniform streamwise magnetic field in the framework of incompressible magnetohydrodynamics (MHD) with finite resistivity and viscosity. This flow is known to be…

流体动力学 · 物理学 2022-10-19 Adrian E. Fraser , Imogen G. Cresswell , Pascale Garaud

This paper presents numerical linear stability analysis of a cylindrical Taylor-Couette flow of liquid metal carrying axial electric current in a generally helical external magnetic field. Axially symmetric disturbances are considered in…

流体动力学 · 物理学 2015-03-30 Jānis Priede

The magnetorotational instability (MRI) of differential rotation under the simultaneous presence of axial and azimuthal components of the (current-free) magnetic field is considered. For rotation with uniform specific angular momentum the…

天体物理学 · 物理学 2009-11-13 Guenther Ruediger , Manfred Schultz

A `flutter machine' is introduced for the investigation of a singular interface between the classical and reversible Hopf bifurcations that is theoretically predicted to be generic in nonconservative reversible systems with vanishing…

经典物理 · 物理学 2018-02-28 Davide Bigoni , Oleg N. Kirillov , Diego Misseroni , Giovanni Noselli , Mirko Tommasini
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