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We outline a novel linear instability that may arise in the dead-zones of protostellar disks, and possibly the fluid interiors of planets and protoplanets. In essence it is an axisymmetric buoyancy instability, but one that would not be…

地球与行星天体物理 · 物理学 2015-05-18 Henrik N. Latter , Julius F. Bonart , Steven A. Balbus

We present here a study of selection of rhombic patterns close to a bicritical point at the onset of primary surface instability in viscous fluids under two-frequency vertical vibration. Rhombic patterns appear to be natural at the primary…

流体动力学 · 物理学 2020-08-18 Krishna Kumar , Supriyo Paul , Dharmesh Jain

In a composite fluid system of two gravitationally coupled barotropic scale-free discs bearing a rotation curve $v\propto r^{-\beta}$ and a power-law surface mass density $\Sigma_0\propto r^{-\alpha}$ with $\alpha=1+2\beta$, we construct…

天体物理学 · 物理学 2009-11-10 Yue Shen , Yu-Qing Lou

In this paper, we derive consistent shallow water equations for bi-layer flows of Newtonian fluids flowing down a ramp. We carry out a complete spectral analysis of steady flows in the low frequency regime and show the occurence of…

流体动力学 · 物理学 2011-04-28 Marc Boutounet , Pascal Noble , Jean-Paul Vila

Vertical oscillation of a fluid interface above a critical amplitude excites the Faraday instability, typically manifesting itself as a standing wave pattern. Fundamentally, the phenomenon is an example of parametric resonance. At high…

流体动力学 · 物理学 2013-10-10 William Batson , Farzam Zoueshtiagh , Ranga Narayanan

The local axisymmetric stability of hydrodynamical and magnetized, nearly-Keplerian gaseous accretion disks around non-rotating black holes is examined in the vicinity of the classical marginally-stable orbit (at radii ~ R_ms). An…

天体物理学 · 物理学 2011-05-10 Kristen Menou

Rotating spiral waves organize spatial patterns in chemical, physical and biological excitable systems. Factors affecting their dynamics such as spatiotemporal drift are of great interest for par- ticular applications. Here, we propose a…

数学物理 · 物理学 2014-08-20 Hans Dierckx , Evelien Brisard , Henri Verschelde , Alexander Panfilov

We have recently shown that spiral density waves propagating in accretion disks can undergo a parametric instability by resonantly coupling with and transferring energy into pairs of inertial waves (or inertial-gravity waves when buoyancy…

地球与行星天体物理 · 物理学 2016-12-21 Jaehan Bae , Richard P. Nelson , Lee Hartmann

We develop a theory of three-dimensional slow Rossby waves in rotating spherical density stratified convection. The Rossby waves with frequencies which are much smaller than the rotating frequency, are excited by a non-axisymmetric…

流体动力学 · 物理学 2017-09-20 T. Elperin , N. Kleeorin , I. Rogachevskii

This article deals with rotating magnetohydrodynamic flows of a thin stratified layer of astrophysical plasma in a gravitational field with a free-surface in a vertical external magnetic field. Magnetohydrodynamic equations are obtained in…

等离子体物理 · 物理学 2019-07-02 Maria Fedotova , Dmitry Klimachkov , Arakel Petrosyan

The vertical shear instability (VSI) is a hydrodynamical instability likely to produce turbulence in the dead zones of protoplanetary disks. Various aspects of this instability remain to be understood, including the disk regions where it…

地球与行星天体物理 · 物理学 2024-02-19 Julio David Melon Fuksman , Mario Flock , Hubert Klahr

The stability of density-stratified viscous Taylor-Couette flows is considered using the Boussinesq approximation but without any use of the short-wave approximation. The flows which are unstable after the Rayleigh criterion (\hat \mu<\hat…

天体物理学 · 物理学 2009-11-10 D. Shalybkov , G. Ruediger

The problem for two-dimensional steady water waves with vorticity is considered. Using methods of spatial dynamics, we reduce the problem to a finite dimensional Hamiltonian system. As an application, we prove the existence of non-symmetric…

数学物理 · 物理学 2019-03-18 Evgeniy Lokharu , Vladimir Kozlov

In this paper we present the global baroclinic instability as a source for vigorous turbulence leading to angular momentum transport in Keplerian accretion disks. We show by analytical considerations and three-dimensional radiation hydro…

天体物理学 · 物理学 2009-11-07 Hubert Klahr , Peter Bodenheimer

The Global Magnetorotational Instability (MRI) is investigated for a configuration in which the rotation frequency changes only in a narrow transition region. If the vertical wavelength of the unstable mode is of the same order or smaller…

天体物理仪器与方法 · 物理学 2011-02-11 J. Pino , S. M. Mahajan

We present results from full general relativistic three-dimensional hydrodynamics simulations of stellar core collapse of a 70 M$_\odot$ star with spectral neutrino transport. To investigate the impact of rotation on non-axisymmetric…

高能天体物理现象 · 物理学 2021-02-03 Shota Shibagaki , Takami Kuroda , Kei Kotake , Tomoya Takiwaki

The collisional drift wave instability in a straight magnetic field configuration is studied within a full-F gyro-fluid model, which relaxes the Oberbeck-Boussinesq (OB) approximation. Accordingly, we focus our study on steep background…

等离子体物理 · 物理学 2019-05-22 Markus Held , Matthias Wiesenberger , Alexander Kendl

Internal waves with frequency larger than twice the local minimum allowable wave frequency can be susceptible to parametric subharmonic instability (PSI). This instability draws energy from the wave and provides a mechanism for generating…

流体动力学 · 物理学 2026-05-28 Logan Knudsen , Jacob Wenegrat , James Hilditch , Leif Thomas

Results from the laboratory experiments on the evolution of vortices (eddies) generated in a rotating tank with topographic beta-effect are presented. The surface elevation and velocity fields are measured by the Altimetric Imaging…

大气与海洋物理 · 物理学 2015-07-06 Yang Zhang , Y. D. Afanasyev

An analytical approach is carried out that provides an inviscid stability criterion for the strato-rotational instability (in short SRI) occurring in a Taylor-Couette system. The control parameters of the problem are the rotation ratio…

流体动力学 · 物理学 2008-11-20 Christiane Normand