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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

A calibrated, non-invasive method for measuring the internal interface height field at high resolution in the rotating, two-layer annulus

GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS 98:6 (2004) 453-471

Authors:

PD Williams, PL Read, TWN Haine
More details from the publisher

An intense stratospheric jet on Jupiter

Nature 427 (2004) 132-135

Authors:

SB Calcutt, Achtergerg, Flasar, Kunde
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Estimation of dynamical invariants without embedding by recurrence plots

CHAOS 14:2 (2004) 234-243

Authors:

M Thiel, MC Romano, PL Read, J Kurths
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Nonconservation of Ertel potential vorticity in hydrogen atmospheres

JOURNAL OF THE ATMOSPHERIC SCIENCES 61:15 (2004) 1953-1965

Authors:

PJ Gierasch, BJ Conrath, PL Read
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Predicting weather conditions and climate for Mars expeditions

SCI TECH 107 (2004) 3-21

Authors:

PL Read, SR Lewis, SJ Bingham, CE Newman

Abstract:

Weather and climatic conditions are among the most important factors to be taken into account when planning expeditions to remote and challenging locations on Earth. This is likely to be equally the case for expedition planners on Mars, where conditions (in terms of extremes of temperature, etc.) can be at least as daunting as back on Earth. With the success of recent unmanned missions to Mars, such as NASA's Mars Pathfinder, Mars Global Surveyor and Mars Odyssey, there is now a great deal of information available on the range of environmental conditions on Mars, from the tropics to the CO2 ice-covered polar caps. This has been further supplemented by the development of advanced numerical models of the Martian atmosphere, allowing detailed and accurate simulations and predictions of the weather and climate across the planet. This report discusses the main weather and climate variables which future Martian human expedition planners will need to take into account. The range of conditions likely to be encountered at a variety of typical locations on Mars is then considered, with reference to predictions from the ESA Mars Climate Database.
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