Vortex crystals at Jupiter’s poles: Emergence controlled by initial small-scale turbulence

At the poles of Jupiter, cyclonic vortices are clustered together in patterns made up of equilateral triangles called vortex crystals. Such patterns are seen in laboratory flows but never before in a planetary atmosphere, where the planet’s rotation and gravity add new physics. Siegelman (2022b) used a one-layer quasi-geostrophic (QG) model with an infinite radius of deformation to study the emergence of vortex crystals from small-scale turbulence, and Li (2020) showed that shielding of the vortices is important for the stability of the vortex crystals. Here we use the shallow water (SW) equations at the pole of a rotating planet to study the emergence and evolution of vortices starting from an initial random pattern of small-scale turbulence. The flow is in a single layer with a free surface whose slope produces the horizontal pressure gradient force. With the planet’s radius and rotation used to define the units, only three input parameters are needed to define the system: the mean kinetic energy of the initial turbulence, the horizontal scale of the initial turbulence, and the radius of deformation of the undisturbed fluid layer. We identified a non-dimensional number, Δ h / h , which is related to the relative layer thickness variation of the initial turbulence and determines whether the vortex crystal or chaotic patterns emerge: Small Δ h / h values lead to vortex crystals, and large Δ h / h values lead to chaotic patterns. The value Δ h / h is related to the radius of deformation as L d − 2 . This means that a large polar radius of deformation is positively correlated to the emergence of vortex crystals, and this implies either a polar atmosphere enriched with water or deeper roots for the vortices than previously estimated. • The study investigates the formation of vortex crystals from initial turbulence. • We identify the perturbation of layer thickness as a critical parameter. • A large polar radius of deformation is necessary for vortex crystal. • Stable vortex crystals rely on shielding mechanisms.

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Publication Details

Journal
Icarus
Published
2024-12-18
DOI
https://doi.org/10.1016/j.icarus.2024.116438
Citations
3
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
0.99

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article

Vortex crystals at Jupiter’s poles: Emergence controlled by initial small-scale turbulence

Sihe Chen, Cheng Li, Andrew P. Ingersoll
3 citations
Icarus
Astro and Planetary Science
0.99
article

Vortex crystals at Jupiter’s poles: Emergence controlled by initial small-scale turbulence

Sihe Chen, Cheng Li, Andrew P. Ingersoll
article en
3 citations

Abstract

At the poles of Jupiter, cyclonic vortices are clustered together in patterns made up of equilateral triangles called vortex crystals. Such patterns are seen in laboratory flows but never before in a planetary atmosphere, where the planet’s rotation and gravity add new physics. Siegelman (2022b) used a one-layer quasi-geostrophic (QG) model with an infinite radius of deformation to study the emergence of vortex crystals from small-scale turbulence, and Li (2020) showed that shielding of the vortices is important for the stability of the vortex crystals. Here we use the shallow water (SW) equations at the pole of a rotating planet to study the emergence and evolution of vortices starting from an initial random pattern of small-scale turbulence. The flow is in a single layer with a free surface whose slope produces the horizontal pressure gradient force. With the planet’s radius and rotation used to define the units, only three input parameters are needed to define the system: the mean kinetic energy of the initial turbulence, the horizontal scale of the initial turbulence, and the radius of deformation of the undisturbed fluid layer. We identified a non-dimensional number, Δ h / h , which is related to the relative layer thickness variation of the initial turbulence and determines whether the vortex crystal or chaotic patterns emerge: Small Δ h / h values lead to vortex crystals, and large Δ h / h values lead to chaotic patterns. The value Δ h / h is related to the radius of deformation as L d − 2 . This means that a large polar radius of deformation is positively correlated to the emergence of vortex crystals, and this implies either a polar atmosphere enriched with water or deeper roots for the vortices than previously estimated. • The study investigates the formation of vortex crystals from initial turbulence. • We identify the perturbation of layer thickness as a critical parameter. • A large polar radius of deformation is necessary for vortex crystal. • Stable vortex crystals rely on shielding mechanisms.

IcarusVol. 429
California Institute of Technology (US), University of Michigan (US)
National Aeronautics and Space Administration, California Institute of Technology, Southwest Research Institute, Marshall Space Flight Center
Climate action
Openalex Percentile: Top 22%
Astro and Planetary Science
0.99
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