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相关论文: A Well-Posed Kelvin-Helmholtz Instability Test and…

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Using data obtained by the high resolution CRisp Imaging SpectroPolarimeter instrument on the Swedish 1-m Solar Telescope, we investigate the dynamics and stability of quiet-Sun chromospheric jets observed at disk center. Small-scale…

太阳与恒星天体物理 · 物理学 2016-10-26 D. Kuridze , T. V. Zaqarashvili , V. Henriques , M. Mathioudakis , F. P. Keenan , A. Hanslmeier

We investigate the conditions under which the magnetohydrodynamic (MHD) modes in a cylindrical magnetic flux tube moving along its axis become unstable against the Kelvin--Helmholtz (KH) instability. We \textbf{use} the dispersion relations…

太阳与恒星天体物理 · 物理学 2018-01-24 I. Zhelyazkov , Z. Dimitrov

Many dynamic pipe flow simulator tools are capable of predicting the onset of hydrodynamic flow instability through detailed simulation. These instabilities provide a natural mechanism for flow regime transition. The quality and reliability…

流体动力学 · 物理学 2018-11-29 Andreas Holm Akselsen

In this paper we discuss the treatment of discontinuities in Smoothed Particle Hydrodynamics (SPH) simulations. In particular we discuss the difference between integral and differential representations of the fluid equations in an SPH…

天体物理学 · 物理学 2008-11-26 Daniel J. Price

The linear MHD Kelvin-Helmholtz instability (KHI) in an anisotropic plasma concerning the direction of an external magnetic field is examined in detail. For this purpose, the MHD equations are used to describe the motion of plasma as a…

太阳与恒星天体物理 · 物理学 2022-04-12 N. S. Dzhalilov , R. Ismayilli

The Kelvin-Helmholtz instability has been proposed as a mechanism to extract energy from magnetohydrodynamic (MHD) kink waves in flux tubes, and to drive dissipation of this wave energy through turbulence. It is therefore a potentially…

太阳与恒星天体物理 · 物理学 2018-10-17 Andrew Hillier , Adrian Barker , Iñigo Arregui , Henrik Latter

We present here a survey of recent results concerning the mathematical analysis of instabilities of the interface between two incompressible, non viscous, fluids of constant density and vorticity concentrated on the interface. This…

偏微分方程分析 · 数学 2010-05-31 Claude Bardos , David Lannes

The Kelvin-Helmholtz instability is well-known in classical hydrodynamics, where it explains the sudden emergence of interfacial surface waves as a function of the velocity of flow parallel to the interface. It can be carried over to the…

超导电性 · 物理学 2019-02-13 V. B. Eltsov , A. Gordeev , M. Krusius

Two-dimensional Kelvin-Helmholtz instability problems are popular examples for assessing discretizations for incompressible flows at high Reynolds number. Unfortunately, the results in the literature differ considerably. This paper presents…

We investigate the Kelvin-Helmholtz instability of stratified jets. The internal component (core) is made of a relativistic gas moving with a relativistic bulk speed. The second component (sheath or envelope) flows between the core and…

天体物理学 · 物理学 2007-05-23 M. Hanasz , H. Sol

A relative motion of the normal and superfluid components of Helium II results in Kelvin-Helmholtz instability (KHI) at their common free surface. We found the exact solutions for the nonlinear stage of the development of that instability.…

流体动力学 · 物理学 2018-05-23 Pavel M. Lushnikov , Nikolay M. Zubarev

We model an imaged Kelvin-Helmholtz (KH) instability on a coronal mass ejecta (CME) in the lower corona by investigating conditions under which kink ($m = 1$) and $m = -3$ magnetohydrodynamic (MHD) modes in an uniformly twisted flux tube…

太阳与恒星天体物理 · 物理学 2015-01-28 I. Zhelyazkov , T. V. Zaqarashvili , R. Chandra

Paraxial propagation of a quasi-monochromatic light wave with two circular polarizations in a defocusing Kerr medium with anomalous dispersion inside a waveguide of annular cross-section was considered. In the phase-separated mode, the…

光学 · 物理学 2024-11-18 Victor P. Ruban

We investigate the Kelvin-Helmholtz instability occuring at the interface of a shear flow configuration in 2D compressible magnetohydrodynamics (MHD). The linear growth and the subsequent non-linear saturation of the instability are studied…

天体物理学 · 物理学 2009-10-31 R. Keppens , G. Toth , R. H. J. Westermann , J. P. Goedbloed

We investigate conditions under which kink magnetohydrodynamic waves propagating along photospheric uniformly twisted flux tubes with axial mass flows become unstable as a consequence of the Kelvin-Helmholtz instability. We employed the…

太阳与恒星天体物理 · 物理学 2015-06-11 I. Zhelyazkov , T. V. Zaqarashvili

We study here the arising of Kelvin--Helmholtz Instability (KHI) in one fast jet of 2014 April 16 observed by the Atmospheric Imaging Assembly (AIA) on board Solar Dynamics Observatory (SDO) in different UV and EUV wavelengths. The…

太阳与恒星天体物理 · 物理学 2018-05-16 M. Bogdanova , I. Zhelyazkov , R. Joshi , R. Chandra

Recent observations support the propagation of a number of magnetohydrodynamic (MHD) modes which, under some conditions, can become unstable and the developing instability is the Kelvin--Helmholtz instability (KHI). In its nonlinear stage…

太阳与恒星天体物理 · 物理学 2019-05-28 Ivan Zhelyazkov , Ramesh Chandra , Reetika Joshi

We consider the stability of clouds surrounded by a hotter confining medium with respect to which they are in motion, against Kelvin-Helmholtz instabilities (KHI). In the presence of cooling, sound waves are damped by dissipation. Whenever…

天体物理学 · 物理学 2009-10-30 Mario Vietri , Andrea Ferrara , Francesco Miniati

We present the results of simulations of the development of the Kelvin-Helmholtz (KH) instability in a cooled, slab symmetric system. The parameters were chosen to approximate the physical conditions typically found in jets from young…

天体物理学 · 物理学 2007-05-23 T. P. Downes , T. P. Ray

We derive here a new stability criterion for two-fluid interfaces. This criterion ensures the existence of "stable" local solutions that do no break down too fast due to Kelvin-Helmholtz instabilities. It can be seen both as a two-fluid…

偏微分方程分析 · 数学 2010-05-31 David Lannes