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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

Mars Environment and Magnetic Orbiter Scientific and Measurement Objectives

Astrobiology Mary Ann Liebert 9:1 (2009) 71-89

Authors:

F Leblanc, B Langlais, T Fouchet, S Barabash, D Breuer, E Chassefire, A Coates, V Dehant, F Forget, H Lammer, S Lewis, M Lopez-Valverde, M Mandea, M Menvielle, A Pais, M Paetzold, P Read, C Sotin, P Tarits, S Vennerstrom
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Synchronization of modulated traveling baroclinic waves in a periodically forced, rotating fluid annulus.

Phys Rev E Stat Nonlin Soft Matter Phys 79:1 Pt 2 (2009) 015202

Authors:

FJR Eccles, PL Read, AA Castrejón-Pita, TWN Haine

Abstract:

Frequency entrainment and nonlinear synchronization are commonly observed between simple oscillatory systems, but their occurrence and behavior in continuum fluid systems are much less well understood. Motivated by possible applications to geophysical fluid systems, such as in atmospheric circulation and climate dynamics, we have carried out an experimental study of the interaction of fully developed baroclinic instability in a differentially heated, rotating fluid annulus with an externally imposed periodic modulation of the thermal boundary conditions. In quasiperiodic and chaotic amplitude-modulated traveling wave regimes, the results demonstrate a strong interaction between the natural periodic modulation of the wave amplitude and the externally imposed forcing. This leads to partial or complete phase synchronization. Synchronization effects were observed even with very weak amplitudes of forcing, and were found with both 1:1 and 1:2 frequency ratios between forcing and natural oscillations.
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FLUID DYNAMICS Rotating convection on the edge

NATURE 457:7227 (2009) 270-271
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QUAGMIRE v1.3: a quasi-geostrophic model for investigating rotating fluids experiments

GEOSCIENTIFIC MODEL DEVELOPMENT 2:1 (2009) 13-32

Authors:

PD Williams, TWN Haine, PL Read, SR Lewis, YH Yamazaki
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Saturn's Exploration Beyond Cassini-Huygens

Chapter in Saturn from Cassini-Huygens, Springer Nature (2009) 745-761

Authors:

Tristan Guillot, Sushil Atreya, Sébastien Charnoz, Michele K Dougherty, Peter Read
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