Abstract

We present a new method for generating robust guesses for unstable periodic orbits (UPOs) by post-processing turbulent data using dynamic mode decomposition (DMD). The approach relies on the identification of near-neutral, repeated harmonics in the DMD eigenvalue spectrum from which both an estimate for the period of a nearby UPO and a guess for the velocity field can be constructed. In this way, the signature of a UPO can be identified in a short time series without the need for a near recurrence to occur, which is a considerable drawback to recurrent flow analysis, the current state-of-the-art. We first demonstrate the method by applying it to a known (simple) UPO and find that the period can be reliably extracted even for time windows of length one quarter of the full period. We then turn to a long turbulent trajectory, sliding an observation window through the time series and performing many DMD computations. Our approach yields many more converged periodic orbits (including multiple new solutions) than a standard recurrent flow analysis of the same data. Furthermore, it also yields converged UPOs at points where the recurrent flow analysis flagged a near recurrence but the Newton solver did not converge, suggesting that the new approach can be used alongside the old to generate improved initial guesses. Finally, we discuss some heuristics on what constitutes a "good" time window for the DMD to identify a UPO.

Highlights

  • Since the discovery of the first unstable periodic orbit (UPO) in a transiently turbulent flow by Kawahara & Kida (2001), there has been a surge in interest and a large number of other periodic solutions found both in this configuration (e.g. Viswanath 2007; Cvitanovic & Gibson 2010) and in other canonical turbulent flows (Chandler & Kerswell 2013; Willis, Cvitanovic & Avila 2013; Lucas, Caulfield & Kerswell 2017)

  • In this paper we introduce a new method based on dynamic mode decomposition (DMD) that goes some way to addressing these issues

  • While DMD on a trajectory shadowing the unstable periodic orbits (UPOs) for one cycle is unlikely to be able to identify the stability properties of the nearby structure, the results presented in Page & Kerswell (2019) indicate that the signature of the periodic orbit – its neutral harmonics – in the DMD results can remain even for relatively short time windows

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Summary

Introduction

Since the discovery of the first unstable periodic orbit (UPO) in a transiently turbulent flow by Kawahara & Kida (2001), there has been a surge in interest and a large number of other periodic solutions found both in this configuration (e.g. Viswanath 2007; Cvitanovic & Gibson 2010) and in other canonical turbulent flows (Chandler & Kerswell 2013; Willis, Cvitanovic & Avila 2013; Lucas, Caulfield & Kerswell 2017). Since the discovery of the first unstable periodic orbit (UPO) in a transiently turbulent flow by Kawahara & Kida (2001), there has been a surge in interest and a large number of other periodic solutions found both in this configuration Viswanath 2007; Cvitanovic & Gibson 2010) and in other canonical turbulent flows (Chandler & Kerswell 2013; Willis, Cvitanovic & Avila 2013; Lucas, Caulfield & Kerswell 2017). The discovery of a large number of UPOs supports a perspective of turbulence in which the flow is viewed as a trajectory in a very high-dimensional dynamical system, wandering between unstable exact coherent structures (Kerswell 2005; Kawahara, Uhlmann & van Veen 2012).

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