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Non-normal transient growth of disturbances is considered as an essential prerequisite for subcritical transition in shear flows, i.e. transition to turbulence despite linear stability of the laminar flow. In this work we present numerical…

流体动力学 · 物理学 2014-03-06 Simon Maretzke , Björn Hof , Marc Avila

Attempts to understand the dynamics of warped astrophysical discs have garnered significant attention, largely motivated by the growing catalogue of observed distorted systems. Previous studies have shown that the evolution of the warp is…

太阳与恒星天体物理 · 物理学 2023-01-25 Callum W. Fairbairn , Gordon I. Ogilvie

Differential rotation is known to suppress linear instabilities in fusion plasmas. However, even in the absence of growing eigenmodes, subcritical fluctuations that grow transiently can lead to sustained turbulence. Here transient growth of…

等离子体物理 · 物理学 2015-08-26 A. A. Schekochihin , E. G. Highcock , S. C. Cowley

Bearing in mind the application to core-collapse supernovae, we study nonlinear properties of the magneto-rotational instability (MRI) by means of three- dimensional simulations in the framework of a local shearing box approximation. By…

太阳与恒星天体物理 · 物理学 2015-06-11 Y. Masada , T. Takiwaki , K. Kotake , T. Sano

The effects that energetic trapped ions have on linear resistive magnetohydrodynamic (MHD) instabilities are studied in a reduced model that captures the essential physics driving or damping the modes through variations in the magnetic…

等离子体物理 · 物理学 2017-06-28 Michael R. Halfmoon , Dylan P. Brennan

Geodesic acoustic mode (GAM) is analyzed by using modified gyro-kinetic (MGK) equation applicable to low-frequency microinstabilities in a rotating axisymmetric plasma. Dispersion relation of GAM in the presence of arbitrary Mach number is…

等离子体物理 · 物理学 2015-01-19 Haijun Ren , Jintao Cao

A linearly unstable, sinusoidal $E \times B$ shear flow is examined in the gyrokinetic framework in both the linear and nonlinear regimes. In the linear regime, it is shown that the eigenmode spectrum is nearly identical to hydrodynamic…

等离子体物理 · 物理学 2019-03-27 A. E. Fraser , M. J. Pueschel , P. W. Terry , E. G. Zweibel

Global time-dependent simulations provide a means to investigate time-dependent dynamic evolution in accretion disks. This paper seeks to extend previous local simulations by beginning a systematic effort to develop fully global…

天体物理学 · 物理学 2009-10-31 John F. Hawley

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

The toroidal geometry of tokamaks and stellarators is known to play a crucial role in the linear physics of zonal flows, leading to e.g. the Rosenbluth-Hinton residual and geodesic acoustic modes. However, descriptions of the nonlinear…

等离子体物理 · 物理学 2026-03-11 Richard Nies , Felix Parra

A nonmodal kinetic theory of the stability of the two-dimensional compressed-sheared mesoscale plasma flows, generated by the radially inhomogeneous electrostatic ion cyclotron parametric microturbulence in the pedestal plasma with a…

等离子体物理 · 物理学 2023-05-24 V. S. Mikhailenko , V. V. Mikhailenko , Hae June Lee

This paper uses the gyro-moment (GM) approach as a multi-fidelity tool to explore the effect of triangularity on tokamak edge turbulence. Considering experimental data from an L-mode DIII-D discharge, we conduct gyrokinetic (GK) simulations…

等离子体物理 · 物理学 2024-07-19 A. C. D. Hoffmann , P. Ricci

We present a study of the linear properties of ion temperature gradient (ITG) modes with collisions modelled by the linearized gyrokinetic (GK) Coulomb collision operator (Frei et al. 2021) in the local limit. The study is based on a…

等离子体物理 · 物理学 2022-06-01 B. J. Frei , A. C. R. Hoffmann , P. Ricci

The magnetorotational instability (MRI) is the leading candidate for driving turbulence, angular momentum transport, and accretion in astrophysical disks. I consider the linear theory of the MRI in a thin, equatorial disk in the Kerr…

天体物理学 · 物理学 2009-11-10 Charles F. Gammie

(Abridged) We analyse the stability and evolution of power-law accretion disc models. These have midplane densities that follow radial power-laws, and have either temperature or entropy distributions that are power-law functions of…

地球与行星天体物理 · 物理学 2015-06-11 Richard P. Nelson , Oliver Gressel , Orkan M. Umurhan

In this work, we compare gyrokinetic simulations in stellarators using different computational domains, namely, flux tube, full-flux-surface, and radially global domains. Two problems are studied: the linear relaxation of zonal flows and…

The nonlinear evolution and the saturation mechanism of the magnetorotational instability (MRI) are investigated using three-dimensional resistive MHD simulations. A local shearing box is used for our numerical analysis and the simulations…

天体物理学 · 物理学 2009-11-07 Takayoshi Sano , Shu-ichiro Inutsuka

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

A new mechanism for toroidal momentum transport in a tokamak is investigated using the gyro-kinetic model. First, an analytic model is developed through the use of the ballooning transform. The terms that generate the momentum transport are…

A linear gyrokinetic eigenvalue code is developed to study the stability of toroidal Alfv\'en eigenmode (TAE) in general axisymmetric toroidal geometry, with the self-consistent treatment of energetic particle drive and core plasma Landau…

等离子体物理 · 物理学 2025-08-21 Guangyu Wei , Fulvio Zonca , Matteo Valerio Falessi , Zhiyong Qiu