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We study a two-dimensional isotropic rotating system and obtain both theoretically and numerically a $K^{-2}$ energy spectrum under the rapidly rotating condition ($Ro\ll 1$), which was initially obtained by Zeman (1994) and Zhou (1995). In…

流体动力学 · 物理学 2024-08-28 Peiyang Li , Jin-Han Xie

We investigate the statistics of rogue waves occurring in the inverse cascade of surface gravity wave turbulence. In such statistically homogeneous, stationary and isotropic wave fields, low-frequency waves are generated by nonlinear…

流体动力学 · 物理学 2022-06-15 Guillaume Michel , Félicien Bonnefoy , Guillaume Ducrozet , Eric Falcon

We present a perturbation theory for studying the instabilities of non-axisymmetric gaseous discs. We perturb the dynamical equations of self-gravitating fluids in the vicinity of a non-axisymmetric equilibrium, and expand the perturbed…

天体物理学 · 物理学 2009-11-11 Naser M. Asghari , Mir Abbas Jalali

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

Wave turbulence is the study of the long-time statistical behaviour of equations describing a set of weakly non-linear interacting waves. Such a theory, which has a natural asymptotic closure, allows us to probe the nature of turbulence…

流体动力学 · 物理学 2023-10-24 Sebastien Galtier

The mechanism describing the recently developed notion of kernel gravity waves (KGWs) is reviewed and such structures are employed to interpret the unstable dynamics of an example stratified plane parallel shear flow. This flow has constant…

地球物理 · 物理学 2007-11-30 O. M. Umurhan , E. Heifetz , N. Harnik , F. Lott

Quasigeostrophic turbulence on a beta-plane with a finite deformation radius is studied nu- merically, with particular emphasis on frequency and combined wavenumber-frequency do- main analyses. Under suitable conditions, simulations with…

大气与海洋物理 · 物理学 2016-04-08 D. L. Suhas , Jai Sukhatme

It is proposed that critical balance - a scale-by-scale balance between the linear propagation and nonlinear interaction time scales - can be used as a universal scaling conjecture for determining the spectra of strong turbulence in…

流体动力学 · 物理学 2011-07-26 S. V. Nazarenko , A. A. Schekochihin

We propose a phenomenological model for incompressible magnetohydrodynamic turbulence. We argue that nonlinear-wave interaction weakens as the energy cascade proceeds to small scales, however, the anisotropy of fluctuations along the…

天体物理学 · 物理学 2009-11-10 Stanislav Boldyrev

Anticyclonic vortices focus and trap near-inertial waves so that near-inertial energy levels are elevated within the vortex core. Some aspects of this process, including the nonlinear modification of the vortex by the wave, are explained by…

流体动力学 · 物理学 2021-07-14 Hossein A. Kafiabad , Jacques Vanneste , William R. Young

Nonlinear interaction and breaking of internal ocean waves are responsible for much of the interior ocean mixing, affecting ocean carbon storage and the global overturning circulation. These interactions may affect the observed Garrett-Munk…

混沌动力学 · 物理学 2025-12-16 Golan Bel , Eli Tziperman

In the presence of inertia-gravity waves, the geostrophic and hydrostatic balance that characterises the slow dynamics of rapidly rotating, strongly stratified flows holds in a time-averaged sense and applies to the Lagrangian-mean velocity…

大气与海洋物理 · 物理学 2021-01-27 Hossein A. Kafiabad , Jacques Vanneste , William R. Young

Decaying three-dimensional (3D) turbulence is studied via direct numerical simulations (DNS) for an isotropic non-rotating flow and for rotating flows with and without helicity. We analyze the cases of moderate Rossby number and large…

流体动力学 · 物理学 2015-05-14 T. Teitelbaum , P. D. Mininni

We study the oscillations and stability of self-gravitating cylindrically symmetric fluid systems and collisionless systems. This is done by studying small perturbations to the equilibrium system and finding the normal modes, using methods…

宇宙学与河外天体物理 · 物理学 2014-01-15 Patrick C. Breysse , Marc Kamionkowski , Andrew Benson

Cosmic ray (CR)-driven instabilities play a decisive role during particle acceleration at shocks and CR propagation in galaxies and galaxy clusters. These instabilities amplify magnetic fields and modulate CR transport so that the…

高能天体物理现象 · 物理学 2021-03-03 Mohamad Shalaby , Timon Thomas , Christoph Pfrommer

We consider a full set of harmonics for the Stokes wave in deep water in the absence of viscosity, and examine the role that higher harmonics play in modifying the classical Benjamin-Feir instability. Using a representation of the wave…

流体动力学 · 物理学 2017-04-26 Shahrdad G. Sajjadi , David L. Ross

Large amplitude water waves on deep water has long been known in the sea faring community, and the cause of great concern for, e.g., oil platform constructions. The concept of such freak waves is nowadays, thanks to satellite and radar…

混沌动力学 · 物理学 2015-05-13 A. Grönlund , B. Eliasson , M. Marklund

Holmboe (1962) postulated that resonant interaction between two or more progressive, linear interfacial waves produces exponentially growing instabilities in idealized (broken-line profiles), homogeneous or density stratified, inviscid…

流体动力学 · 物理学 2014-07-02 Anirban Guha , Gregory A. Lawrence

We study the longitudinal instabilities of two interpenetrating fluids interacting only through gravity. When one of the constituents is of relatively low density, it is possible to have a band of unstable wave numbers well separated from…

天体物理学 · 物理学 2013-03-06 A. R. R. Casti , P. J. Morrison , E. A. Spiegel

We study the tensorial modes of the two-fluid model, where one of this fluids has an equation of state $p = - \rho/3$ (variable cosmological constant, cosmic string fluid, texture) or $p = - \rho$ (cosmological constant), while the other…

广义相对论与量子宇宙学 · 物理学 2007-05-23 J. C. Fabris , S. V. B. Goncalves