Exact planetary waves and jet streams
Nick Pizzo, Rick Salmon

TL;DR
This paper derives exact nonlinear planetary wave solutions on approximated rotating sphere surfaces, revealing their structure, mean flows, and stability, with implications for understanding jet streams and turbulence.
Contribution
It introduces exact nonlinear wave solutions in Lagrangian form on beta and gamma plane approximations, linking them to planetary jet streams and turbulence.
Findings
Wave solutions exhibit simple Lagrangian forms and non-trivial mean flows.
Some waves resemble polar jet streams and Ptolemaic vortex waves.
Numerical simulations show stable and turbulent flow regimes.
Abstract
We investigate exact nonlinear waves on surfaces locally approximating the rotating sphere for two-dimensional inviscid incompressible flow. Our first system corresponds to a beta-plane approximation at the equator and the second to a gamma approximation, with the latter describing flow near the poles. We find exact wave solutions in the Lagrangian reference frame that cannot be written down in closed form in the Eulerian reference frame. The wave particle trajectories, contours of potential vorticity and Lagrangian mean velocity take relatively simple forms. The waves possess a non-trivial Lagrangian mean flow that depends on the amplitude of the waves and on a particle label that characterizes values of constant potential vorticity. The mean flow arises due to potential vorticity conservation on fluid particles. Solutions over the entire space are generated by assuming that the flow…
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
TopicsSolar and Space Plasma Dynamics
