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To understand the self-sustenance of subcritical turbulence in spectrally stable shear flows, we performed direct numerical simulations of homogeneous shear turbulence for different aspect ratios of the flow domain and analyzed the…

流体动力学 · 物理学 2017-05-17 G. Mamatsashvili , G. Khujadze , G. Chagelishvili , S. Dong , J. Jiménez , H. Foysi

We investigate magnetohydrodynamic turbulence driven by the magnetorotational instability (MRI) in Keplerian disks with a nonzero net azimuthal magnetic field using shearing box simulations. As distinct from most previous studies, we…

地球与行星天体物理 · 物理学 2017-08-23 D. Gogichaishvili , G. Mamatsashvili , W. Horton , G. Chagelishvili , G. Bodo

We investigate magnetohydrodynamic (MHD) turbulence in plane shear flows with a streamwise background magnetic field in the super-Alfv\'enic regime. We show that the large-scale velocity shear suppresses turbulence imbalance, driving the…

空间物理 · 物理学 2026-02-17 M. Kavtaradze , G. Mamatsashvili , G. Chagelishvili , E. Uchava

Laminar shear flows can display large non-modal perturbation growth, often through the lift-up mechansm, and can undergo subcritical transition to turbulence. The process is three-dimensional. Two-dimensional (2D) spanwise-independent…

流体动力学 · 物理学 2024-05-01 Sharath Jose

Identifying generic physical mechanisms responsible for the generation of magnetic fields and turbulence in differentially rotating flows is fundamental to understand the dynamics of astrophysical objects such as accretion disks and stars.…

天体物理学 · 物理学 2009-11-13 F. Rincon , G. I. Ogilvie , M. R. E. Proctor , C. Cossu

We briefly review helicity dynamics, inverse and bi-directional cascades in fluid and magnetohydrodynamic (MHD) turbulence, with an emphasis on the latter. The energy of a turbulent system, an invariant in the non-dissipative case, is…

流体动力学 · 物理学 2019-03-13 A. Pouquet , D. Rosenberg , J. E. Stawarz , R. Marino

We present results from two-dimensional numerical simulations of a supersonic turbulent flow in the plane of the galactic disk, incorporating shear, thresholded and discrete star formation (SF), self-gravity, rotation and magnetic fields. A…

天体物理学 · 物理学 2009-10-28 T. Passot , E. Vazquez-Semadeni , A. Pouquet

Electron magnetohydrodynamic (EMHD) turbulence in two dimensions is studied via high-resolution numerical simulations with a normal diffusivity. The resulting energy spectra asymptotically approach a $k^{-5/2}$ law with increasing $R_B$,…

等离子体物理 · 物理学 2009-05-01 C. J. Wareing , R. Hollerbach

Special features of magnetohydrodynamic waves linear dynamics in smooth shear flows are studied. Quantitative asymptotic and numerical analysis are performed for wide range of system parameters when basic flow has constant shear of velocity…

天体物理学 · 物理学 2016-08-30 G. Gogoberidze , G. D. Chagelishvili , R. Z. Sagdeev , D. G. Lominadze

The emergence of turbulence in shear flows is a well-investigated field. Yet, one of major issues is the apparent contradiction between linear stability analysis quoting a flow to be stable and results from experiments and simulations…

高能天体物理现象 · 物理学 2018-09-28 Tanayveer Singh Bhatia , Banibrata Mukhopadhyay

The dynamics of spectral transport in two-dimensional turbulent convection of electrically conducting fluids is studied by means of direct numerical simulations (DNS) in the frame of the magnetohydrodynamic (MHD) Boussinesq approximation.…

太阳与恒星天体物理 · 物理学 2015-05-13 Dan Škandera , Wolf-Christian Müller

It is often asserted or implicitly assumed, without justification, that the results of two-dimensional investigations of plasma turbulence are applicable to the three-dimensional plasma environments of interest. A projection method is…

太阳与恒星天体物理 · 物理学 2019-02-20 Gregory G. Howes

We investigate sustenance and dependence on magnetic Prandtl number (${\rm Pm}$) for magnetorotational instability (MRI)-driven turbulence in astrophysical Keplerian disks with zero net magnetic flux using standard shearing box simulations.…

高能天体物理现象 · 物理学 2020-12-02 George Mamatsashvili , George Chagelishvili , Martin E. Pessah , Frank Stefani , Gianluigi Bodo

We present a set of three-dimensional (3D) direct numerical simulations of incompressible decaying magnetohydrodynamic turbulence in which we investigate the influence of an external uniform magnetic field B_0. A parametric study in terms…

流体动力学 · 物理学 2009-11-13 Barbara Bigot , Sebastien Galtier , Helene Politano

We analyze 3D numerical simulations of driven incompressible magnetohydrodynamic (MHD) turbulence in a periodic box threaded by a moderately strong external magnetic field. We sum over nonlinear interactions within Fourier wavebands and…

天体物理学 · 物理学 2011-05-10 Jungyeon Cho , Alex Lazarian , Ethan Vishniac

Linear transient growth analysis is commonly used to suggest the structure of disturbances which are particularly efficient in triggering transition to turbulence in shear flows. We demonstrate that the addition of nonlinearity to the…

流体动力学 · 物理学 2010-09-06 Chris C. T. Pringle , Rich R. Kerswell

This manuscript has been accepted for publication in Physical Review Fluids, see https://journals.aps.org/prfluids/accepted/d5074S28J6b11905012b7cb06505e8f2149dd5f20. This work investigates the mechanisms that underlie transitions to…

流体动力学 · 物理学 2020-12-24 Christopher J. Camobreco , Alban Pothérat , Gregory J. Sheard

The non-modal transient growth of perturbations in horizontal and inclined channel flows of two immiscible fluids is studied. 3D perturbations are examined in order to find the optimal perturbations that attain the maximum amplification of…

流体动力学 · 物理学 2018-10-31 Ilya Barmak , Alexander Gelfgat , Amos Ullmann , Neima Brauner

The fluid dynamics community has found success in explaining both the onset and coherent structure formation in wall-bounded turbulence through examining transient growth and pseudoresonance. Whether similar effects are important in plasmas…

等离子体物理 · 物理学 2024-11-01 Elias Pratschke

When magnetohydrodynamic turbulence evolves in the presence of a large-scale mean magnetic field, an anisotropy develops relative to that preferred direction. The well-known tendency is to develop stronger gradients perpendicular to the…

等离子体物理 · 物理学 2020-07-15 Rohit Chhiber , William H. Matthaeus , Sean Oughton , Tulasi N. Parashar
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