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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

Generation of inertia-gravity waves by a time-dependent baroclinic wave in the laboratory

PHYSICS AND CHEMISTRY OF THE EARTH PART B-HYDROLOGY OCEANS AND ATMOSPHERE 24:5 (1999) 455-460

Authors:

AF Lovegrove, PL Read, CJ Richards
More details from the publisher

Improved general circulation models of the Martian atmosphere from the surface to above 80 km

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS 104:E10 (1999) 24155-24175

Authors:

F Forget, F Hourdin, R Fournier, C Hourdin, O Talagrand, M Collins, SR Lewis, PL Read, JP Huot
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The effect of sloping boundaries on baroclinic instability in two related internally heated, rotating fluid systems

PHYSICS AND CHEMISTRY OF THE EARTH PART B-HYDROLOGY OCEANS AND ATMOSPHERE 24:5 (1999) 481-486

Authors:

ME Bastin, PL Read
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Investigation of Saturn's atmosphere by Cassini

PLANET SPACE SCI 46:9-10 (1998) 1315-1324

Authors:

FW Taylor, SB Calcutt, PGJ Irwin, CA Nixon, PL Read, PJC Smith, TJ Vellacott

Abstract:

This paper considers the rationale for the exploration of Saturn's atmosphere by the Cassini mission, taking account of the key scientific questions posed by the earlier investigation by Voyager, and the capabilities of the instrumentation making up the Cassini payload. While by no means all objectives can be addressed by this particular configuration, in particular without a Saturn entry probe, if everything goes according to plan important progress should be possible on a number of key objectives. (C) 1998 Elsevier Science Ltd. All rights reserved.
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A comparison of empirical orthogonal decomposition methods in baroclinic flows

Dynamics of Atmospheres and Oceans 27:1-4 (1998) 649-660

Authors:

AV Stephen, IM Moroz, PL Read, WG Früh

Abstract:

The relative merits of three contrasting empirical orthogonal decomposition methods in common use (namely, Proper Orthogonal Decomposition, Biorthogonal Decomposition and Multivariate Singular Systems Analysis) are considered as applied to baroclinic flow data. The regimes analysed are a steady, drifting wave, a modulated amplitude vacillating wave flow and a neighbouring multi-mode state which exhibits intermittency. The results are used to make a qualitative comparison of the methods in terms of convergence properties, variance capture and eigenfunction structure. The feasibility of using the resulting empirical orthogonal functions to transform partial differential equations to ordinary differential equations by Galerkin projection is mentioned. © 1997 Elsevier Science B.V.
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