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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

Baroclinic waves in an air-filled thermally driven rotating annulus.

Phys Rev E Stat Nonlin Soft Matter Phys 75:2 Pt 2 (2007) 026301

Authors:

AA Castrejón-Pita, PL Read

Abstract:

In this study an experimental investigation of baroclinic waves in air in a differentially heated rotating annulus is presented. Air has a Prandtl number of 0.707, which falls within a previously unexplored region of parameter space for baroclinic instability. The flow regimes encountered include steady waves, periodic amplitude vacillations, modulated amplitude vacillations, and either monochromatic or mixed wave number weak waves, the latter being characterized by having amplitudes less than 5% of the applied temperature contrast. The distribution of these flow regimes in parameter space are presented in a regime diagram. It was found that the progression of transitions between different regimes is, as predicted by recent numerical modeling results, in the opposite sense to that usually found in experiments with high Prandtl number liquids. No hysteresis in the flow type, with respect to variations in the rotation rate, was found in this investigation.
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DNS of Structural Vacillation in the transition to geostrophic turbulence

Advances in Turbulence XI - Proceedings of the 11th EUROMECH European Turbulence Conference (2007) 432-434

Authors:

WG Früh, P Maubert, PL Read, A Randriamampianina

Abstract:

The onset of small-scale fluctuations around a steady convection pattern in a rotating baroclinic annulus filled with air is investigated using Direct Numerical Simulations (DNS). In previous laboratory experiments of baroclinic waves, such fluctuations have been associated with Structural Vacillation which is regarded as the first step in the transition to fully-developed geostrophic turbulence. Here we present an analysis which focusses on the small-scale features.
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Editorial

Quarterly Journal of the Royal Meteorological Society Wiley 133:622 (2007) 1-1

Authors:

Peter L Read, Ian Roulstone
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Assimilation of thermal emission spectrometer atmospheric data during the Mars Global Surveyor aerobraking period

ICARUS 192:2 (2007) 327-347

Authors:

Stephen R Lewis, Peter L Read, Barney J Conrath, John C Pearl, Michael D Smith
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Dynamics of convectively driven banded jets in the laboratory

JOURNAL OF THE ATMOSPHERIC SCIENCES 64:11 (2007) 4031-4052

Authors:

Peter L Read, Yasuhiro H Yamazaki, Stephen R Lewis, Paul D Williams, Robin Wordsworth, Kuniko Miki-Yamazaki
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