Variational methods for finding periodic orbits in the incompressible Navier-Stokes equations
arXiv:2108.12219 · doi:10.1017/jfm.2022.299
Abstract
Unstable periodic orbits are believed to underpin the dynamics of turbulence, but by their nature are hard to find computationally. We present a family of methods to converge such unstable periodic orbits for the incompressible Navier-Stokes equations, based on variations of an integral objective functional, and using traditional gradient-based optimisation strategies. Different approaches for handling the incompressibility condition are considered. The variational methods are applied to the specific case of periodic, two-dimensional Kolmogorov flow and compared against existing Newton iteration-based shooting methods. While computationally slow, our methods converge from very inaccurate initial guesses.
References in corpus (4)
- Unstable recurrent patterns in Kuramoto-Sivashinsky dynamics
- Recurrent flow analysis in spatiotemporally chaotic 2-dimensional Kolmogorov flow
- Capturing Turbulent Dynamics and Statistics in Experiments with Unstable Periodic Orbits
- Adjoint-based variational method for constructing periodic orbits of high-dimensional chaotic systems
Cited by in corpus (10)
- Exact coherent structures in two-dimensional turbulence identified with convolutional autoencoders
- A chaotic lattice field theory in one dimension
- Predicting chaotic statistics with unstable invariant tori
- Multi-scale invariant solutions in plane Couette flow: a reduced-order model approach
- Dynamics of a Data-Driven Low-Dimensional Model of Turbulent Minimal Pipe Flow
- Ghost states underlying spatial and temporal patterns: how non-existing invariant solutions control nonlinear dynamics
- Data-driven guessing and gluing of unstable periodic orbits
- Stabilising nonlinear travelling waves in pipe flow using time-delayed feedback
- Three-dimensional gravity-capillary standing waves: computation, resonance and instability
- On nonlinear transitions, minimal seeds and exact solutions for the geodynamo