Super- and sub-rotating equatorial jets: Newtonian cooling versus Rayleigh friction
Emma S. Warneford, Paul J. Dellar

TL;DR
This paper investigates why different damping mechanisms in shallow water models lead to either super-rotating or sub-rotating equatorial jets, explaining the phenomenon through Rossby wave decay effects within quasigeostrophic theory.
Contribution
It provides a theoretical mechanism based on Rossby wave decay to explain the formation of super- and sub-rotating equatorial jets under different damping conditions.
Findings
Newtonian cooling induces eastward equatorial flow.
Rayleigh friction induces westward equatorial flow.
The mechanism is consistent with quasigeostrophic theory and Rossby wave dynamics.
Abstract
Numerical simulations of the shallow water equations on rotating spheres produce mixtures of robust vortices and alternating zonal jets, as seen in the atmospheres of the gas giant planets. However, simulations that include Rayleigh friction invariably produce a sub-rotating (retrograde) equatorial jet for Jovian parameter regimes, whilst observations of Jupiter show a super-rotating (prograde) equatorial jet that has persisted over several decades. Super-rotating equatorial jets have recently been obtained in shallow water simulations that include a Newtonian relaxation of perturbations to the layer thickness to model radiative cooling to space, and in simulations of the thermal shallow water equations that include a similar relaxation term in their temperature equation. Simulations of global quasigeostrophic forms of these different models produce equatorial jets in the same…
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Taxonomy
TopicsAstro and Planetary Science · Geophysics and Gravity Measurements · Geology and Paleoclimatology Research
