On the local topology evolution of a high-symmetry flow
From MaRDI portal
Publication:4423932
DOI10.1063/1.868487zbMath1023.76574OpenAlexW2045188236MaRDI QIDQ4423932
Richard B. Pelz, Oluş N. Boratav
Publication date: 18 November 2003
Published in: Physics of Fluids (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1063/1.868487
Related Items
Evidence for the development of singularities in Euler flow, The three-dimensional Euler equations: Where do we stand?, Influence of flow topology and dilatation on scalar mixing in compressible turbulence, Self-similar collapse of 2D and 3D vortex filament models, Structures and structure functions in the inertial range of turbulence, Dynamics of the velocity gradient tensor invariants in isotropic turbulence, A vortex interaction mechanism for generating energy and enstrophy fluctuations in high-symmetric turbulence, Self-similar collapse of a 3D straight vortex filament model
Cites Work
- Tracing complex singularities with spectral methods
- Remarks on the breakdown of smooth solutions for the 3-D Euler equations
- Remarks on a paper by J. T. Beale, T. Kato, and A. Majda (Remarks on the breakdown of smooth solutions for the 3-dimensional Euler equations)
- A model of vortex reconnection
- Collapsing solutions to the 3-D Euler equations
- The kinematics of stretching and alignment of material elements in general flow fields
- Exact solution of a restricted Euler equation for the velocity gradient tensor
- Reconnection in orthogonally interacting vortex tubes: Direct numerical simulations and quantifications
- Dynamical aspects of vortex reconnection of perturbed anti-parallel vortex tubes
- Evidence for a singularity of the three-dimensional, incompressible Euler equations
- On the behavior of velocity gradient tensor invariants in direct numerical simulations of turbulence
- Development of enstrophy and spectra in numerical turbulence
- Eigenvalue problems in three-dimensional Euler flows
- Locally isotropic pressure Hessian in a high-symmetry flow
- A study of the fine-scale motions of incompressible time-developing mixing layers
- Direct numerical simulation of transition to turbulence from a high-symmetry initial condition