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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

From mixing to geostrophy: geostrophic turbulence in atmospheres, oceans, and the laboratory

Chapter in Marine Turbulence, Cambridge Univ Pr (2005) 52

Abstract:

This 2005 book gives a comprehensive overview of measurement techniques and theories for marine turbulence and mixing processes.

Hadley circulation and Kelvin wave-induced equatorial jets in the atmospheres of Jupiter and Saturn

Planetary and Space Science 53 (2005) 508-525

Authors:

Y Yamazaki, P.L. Read, D.R. Skeet

The atmospheric circulation and dust activity in different orbital epochs on Mars

Icarus 174 (2005) 135-160

Authors:

PL Read, C E Newman, S R Lewis

Temperatures, Winds, and Composition in the Saturnian System

Science 307 (2005) 1247-1251

Authors:

FM Flasar, PGJ Irwin, SB Calcutt, R Achterberg, FW Taylor

A simplified model of the Martian atmosphere - Part 2: A POD-Galerkin analysis

Nonlinear Processes in Geophysics 12:5 (2005) 625-642

Authors:

SG Whitehouse, SR Lewis, IM Moroz, PL Read

Abstract:

In Part I of this study Whitehouse et al. (2005) performed a diagnostic analysis of a simplied model of the Martian atmosphere, in which topography was absent and in which heating was modelled as Newtonian relaxation towards a zonally symmetric equilibrium temperature field. There we derived a reduced-order approximation to the vertical and the horizonal structure of the baroclinically unstable Martian atmosphere, retaining only the barotropic mode and the leading order baroclinic modes. Our objectives in Part II of the study are to incorporate these approximations into a Proper Orthogonal Decomposition-Galerkin expansion of the spherical quasi-geostrophic model in order to derive hierarchies of nonlinear ordinary differential equations for the time-varying coefficients of the spatial structures. Two different vertical truncations are considered, as well as three different norms and 3 different Galerkin truncations. We investigate each in turn, using tools from bifurcation theory, to determine which of the systems most closely resembles the data for which the original diagnostics were performed. 漏 2005 Author(s). This work is licensed under a Creative Commons License.

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