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Image of Jupiter's Great Red Spot from Voyager 1

Image of Jupiter's Great Red Spot, obtained during the fly-by of Jupiter by NASA's Voyager 1 spacecraft in 1979.

Credit: NASA/JPL

Prof. Peter Read

Emeritus/researcher

Research theme

  • Climate physics
  • Exoplanets and planetary physics

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Geophysical and Astrophysical Fluid Dynamics
  • Planetary Climate Dynamics
Peter.Read@physics.ox.ac.uk
Telephone: 01865 (2)72082
Atmospheric Physics Clarendon Laboratory, room 210
  • About
  • Publications

Turbulence, waves, and jets in a differentially heated rotating annulus experiment

PHYSICS OF FLUIDS 20:12 (2008) ARTN 126602

Authors:

RD Wordsworth, PL Read, YH Yamazaki

Direct Numerical Simulation of structural vacillation in the transition to geostrophic turbulence

(2007)

Authors:

Anthony Randriamampianina, Pierre Maubert, Wolf-Gerrit Fruh, Peter L Read

Dynamics of convectively driven banded jets in the laboratory

Journal of the Atmospheric Sciences 64:11 (2007) 4031-4052

Authors:

PL Read, J Sommeria, P D Williams, Y H Yamazaki

Dynamics of convectively driven banded jets in the laboratory

Journal of the Atmospheric Sciences 64:11 (2007) 4031-4052

Authors:

PL Read, YH Yamazaki, SR Lewis, PD Williams, R Wordsworth, K Miki-Yamazaki, J Sommeria, H Didelle

Abstract:

The banded organization of clouds and zonal winds in the atmospheres of the outer planets has long fascinated observers. Several recent studies in the theory and idealized modeling of geostrophic turbulence have suggested possible explanations for the emergence of such organized patterns, typically involving highly anisotropic exchanges of kinetic energy and vorticity within the dissipationless inertial ranges of turbulent flows dominated (at least at large scales) by ensembles of propagating Rossby waves. The results from an attempt to reproduce such conditions in the laboratory are presented here. Achievement of a distinct inertial range turns out to require an experiment on the largest feasible scale. Deep, rotating convection on small horizontal scales was induced by gently and continuously spraying dense, salty water onto the free surface of the 13-m-diameter cylindrical tank on the Coriolis platform in Grenoble, France. A "planetary vorticity gradient" or "Ξ² effect" was obtained by use of a conically sloping bottom and the whole tank rotated at angular speeds up to 0.15 rad s-1. Over a period of several hours, a highly barotropic, zonally banded large-scale flow pattern was seen to emerge with up to 5-6 narrow, alternating, zonally aligned jets across the tank, indicating the development of an anisotropic field of geostrophic turbulence. Using particle image velocimetry (PIV) techniques, zonal jets are shown to have arisen from nonlinear interactions between barotropic eddies on a scale comparable to either a Rhines or "frictional" wavelength, which scales roughly as (Ξ²/Urms) -1/2. This resulted in an anisotropic kinetic energy spectrum with a significantly steeper slope with wavenumber k for the zonal flow than for the nonzonal eddies, which largely follows the classical Kolmogorov k-5/3 inertial range. Potential vorticity fields show evidence of Rossby wave breaking and the presence of a "hyperstaircase" with radius, indicating instantaneous flows that are supercritical with respect to the Rayleigh-Kuo instability criterion and in a state of "barotropic adjustment." The implications of these results are discussed in light of zonal jets observed in planetary atmospheres and, most recently, in the terrestrial oceans. Β© 2007 American Meteorological Society.

Atmospheric and Oceanic Fluid Dynamics: Fundamentals and Large‐Scale Circulation Geoffrey K. Vallis. ISBN 0‐5218‐4969‐1. Cambridge University Press 2007. 770 pages.

Quarterly Journal of the Royal Meteorological Society Wiley 133:629 (2007) 2145-2146

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