Zonal Flows and Turbulence in Fluids and Plasmas
Jeffrey B. Parker

TL;DR
This paper investigates how turbulence transitions to zonal flows in fluids and plasmas, using the CE2 framework to analyze symmetry-breaking instabilities and pattern formation, revealing multiple stable flow wavelengths and jet merging dynamics.
Contribution
It extends the understanding of zonostrophic instability within the CE2 framework, linking it to pattern formation theory and analyzing the stability of zonal flow wavelengths.
Findings
Zonostrophic instability can be viewed as a pattern formation process.
Multiple zonal flow wavelengths are possible, with only a subset being stable.
Unstable wavelengths evolve through jet merging to reach stability.
Abstract
In geophysical and plasma contexts, zonal flows are well known to arise out of turbulence. We elucidate the transition from statistically homogeneous turbulence without zonal flows to statistically inhomogeneous turbulence with steady zonal flows. Starting from the Hasegawa--Mima equation, we employ both the quasilinear approximation and a statistical average, which retains a great deal of the qualitative behavior of the full system. Within the resulting framework known as CE2, we extend recent understanding of the symmetry-breaking `zonostrophic instability'. Zonostrophic instability can be understood in a very general way as the instability of some turbulent background spectrum to a zonally symmetric coherent mode. As a special case, the background spectrum can consist of only a single mode. We find that in this case the dispersion relation of zonostrophic instability from the CE2…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Magnetic confinement fusion research · Ionosphere and magnetosphere dynamics
