Phase transitions and marginal ensemble equivalence for freely evolving flows on a rotating sphere

C Herbert1, B Dubrulle, P H Chavanis

  • 1Service de Physique de l'Etat Condensé, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Saclay, Gif-sur-Yvette, France. corentin.herbert@lsce.ipsl.fr

Summary

Planetary atmospheric circulation can be understood through statistical mechanics of turbulent flows. This study reveals phase transitions between zonal flow and dipole structures in a simplified atmospheric model.

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