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Two-dimensional numerical simulations have been performed to understand the effect of wall proximity on the vortex-induced vibrations (VIV) of an elastically mounted circular cylinder having two degrees of freedom for gap ratios g/D =…

Fluid Dynamics · Physics 2022-12-06 V Brahmini Priya P , Aditya Karthik , Vedanth N K , Supradeepan K , P S Gurugubelli

We report some qualitatively new features of emergence, competition and dynamical stabilization of dissipative rotating spiral waves (RSWs) in the cellular-automaton model of laser-like excitable media proposed in arXiv:cond-mat/0410460v2 ;…

Cellular Automata and Lattice Gases · Physics 2008-05-15 S. D. Makovetskiy , D. N. Makovetskii

The extreme infrared (IR) luminosity of local luminous and ultra-luminous IR galaxies (U/LIRGs; 11 < log LIR /Lsun < 12 and log LIR /Lsun > 12, respectively) is mainly powered by star-formation processes triggered by mergers or…

The present work investigates forced ignition and oscillating propagation of spray flame in a mixture of fine ethanol droplets and air. Eulerian-Eulerian method with two-way coupling is used and detailed chemical mechanism is considered.…

Fluid Dynamics · Physics 2022-02-16 Qiang Li , Huangwei Zhang

The paper presents a numerical investigation of the leading-edge vortices generated by rotating triangular wings at Reynolds number $Re=250$. A series of three-dimensional numerical simulations have been carried out using a Fourier…

Fluid Dynamics · Physics 2015-04-20 Dmitry Kolomenskiy , Yossef Elimelech , Kai Schneider

We study the effect of shear due to the large scale flow (LSF) on the heat flux in Rayleigh B'enard convection for a range of near-plate Rayleigh numbers $8\times 10^7 \leq Ra_w \leq 5\times 10^{14}$, by studying its effect on the local…

Fluid Dynamics · Physics 2024-09-04 Prafulla P. Shevkar , Baburaj A. Puthenveettil

The intracluster light (ICL) fraction, measured at certain specific wavelengths, has been shown to provide a good marker for determining the dynamical stage of galaxy clusters, i.e., merging versus relaxed, for small to intermediate…

Astrophysics of Galaxies · Physics 2023-08-09 Y. Jiménez-Teja , R. A. Dupke , P. A. A. Lopes , J. M. Vílchez

A linear analysis of the zombie vortex instability is performed in a stratified shearing sheet setting for three model barotropic shear flows. The linear analysis is done by utilizing a Green's function formulation to resolve the critical…

Fluid Dynamics · Physics 2016-10-26 Orkan M. Umurhan , Karim Shariff , Jeffrey N. Cuzzi

We report the physical origin of transient off-centre convective zones (oCZs) that arise in mass accreting stellar models. Using detailed MESA simulations of binary evolution, we find that these oCZs are not numerical artefacts but emerge…

Solar and Stellar Astrophysics · Physics 2025-09-17 A. Miszuda

We study the dynamics and properties of a turbulent flame, formed in the presence of subsonic, high-speed, homogeneous, isotropic Kolmogorov-type turbulence in an unconfined system. Direct numerical simulations are performed with…

High Energy Astrophysical Phenomena · Physics 2011-06-21 Alexei Y. Poludnenko , Elaine S. Oran

A novel jet-stirred combustion chamber is designed to study turbulent premixed flames. In the new approach, multiple impinging turbulent jets are used to stir the mixture. It is well known that pair of counterflowing turbulent jets produces…

Fluid Dynamics · Physics 2017-12-07 Abbasali A. Davani , Paul D. Ronney

A wall-resolved large-eddy simulation (LES) of the fluid flow around a 30P30N airfoil is conducted at a Reynolds number of Rec=750,000 and an angle of attack (AoA) of 9 degrees. The simulation results are validated against experimental data…

Fluid Dynamics · Physics 2024-11-11 Ricard Montalà , Benet Eiximeno , Arnau Miró , Oriol Lehmkuhl , Ivette Rodriguez

Monte Carlo simulations and finite-size scaling theory have been used to study the critical behavior of repulsive dimers on square lattices at 2/3 monolayer coverage. A "zig-zag" (ZZ) ordered phase, characterized by domains of parallel ZZ…

Statistical Mechanics · Physics 2008-04-09 F. Roma , J. L. Riccardo , A. J. Ramirez-Pastor

The problem of linear stability of confined V-flames with arbitrary gas expansion is addressed. Using the on-shell description of flame dynamics, a general equation governing propagation of disturbances of an anchored flame is obtained.…

Fluid Dynamics · Physics 2009-02-26 Hazem El-Rabii , Guy Joulin , Kirill A. Kazakov

This study investigates the dynamics of non-isothermal swirling jets undergoing vortex breakdown, with an emphasis on helical coherent structures. It is proposed that the dominant helical coherent structure can be suppressed by heating the…

Fluid Dynamics · Physics 2016-11-03 Lothar Rukes , Moritz Sieber , Oliver Paschereit , Kilian Oberleithner

With the ever faster cadence of untargeted surveys of the sky, the supernova (SN) community will capture in the coming years a growing number of shock breakouts in red-supergiant (RSG) stars. Expecting a high frequency of breakouts within…

Solar and Stellar Astrophysics · Physics 2026-03-18 Luc Dessart , W. V. Jacobson-Galan

Experimental and numerical study of the steady-state cyclonic vortex from isolated heat source in a rotating fluid layer is described. The structure of laboratory cyclonic vortex is similar to the typical structure of tropical cyclones from…

Fluid Dynamics · Physics 2017-05-03 A. Sukhanovskii , A. Evgrafova , E. Popova

The dimensionless kinetic energy dissipation rate C_epsilon is estimated from numerical simulations of statistically stationary isotropic box turbulence that is slightly compressible. The Taylor microscale Reynolds number Re_lambda range is…

We investigate the incompressible flow past a square cylinder immersed in the wake of an upstream nearby splitter plate separating two streams of different velocity. The bottom stream Reynolds number, based on the square side, $Re_B=56$ is…

Fluid Dynamics · Physics 2022-11-09 Reda El Mansy , Wasim Sarwar , Josep M Bergada , Fernando Mellibovsky

In confined rotating convection, a strong zonal flow can develop close to the side wall with a modal structure that precesses anti-cyclonically (counter to the applied rotation) along the side wall. It is surmised that this is a robust…

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