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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

Storm-clouds brooding on towering heights

Nature Springer Nature 475:7354 (2011) 44-45
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Thermal structure and dynamics of Saturn's northern springtime disturbance.

Science 332:6036 (2011) 1413-1417

Authors:

Leigh N Fletcher, Brigette E Hesman, Patrick GJ Irwin, Kevin H Baines, Thomas W Momary, Agustin Sanchez-Lavega, F Michael Flasar, Peter L Read, Glenn S Orton, Amy Simon-Miller, Ricardo Hueso, Gordon L Bjoraker, Andrei Mamoutkine, Teresa del Rio-Gaztelurrutia, Jose M Gomez, Bonnie Buratti, Roger N Clark, Philip D Nicholson, Christophe Sotin

Abstract:

Saturn's slow seasonal evolution was disrupted in 2010-2011 by the eruption of a bright storm in its northern spring hemisphere. Thermal infrared spectroscopy showed that within a month, the resulting planetary-scale disturbance had generated intense perturbations of atmospheric temperatures, winds, and composition between 20° and 50°N over an entire hemisphere (140,000 kilometers). The tropospheric storm cell produced effects that penetrated hundreds of kilometers into Saturn's stratosphere (to the 1-millibar region). Stratospheric subsidence at the edges of the disturbance produced "beacons" of infrared emission and longitudinal temperature contrasts of 16 kelvin. The disturbance substantially altered atmospheric circulation, transporting material vertically over great distances, modifying stratospheric zonal jets, exciting wave activity and turbulence, and generating a new cold anticyclonic oval in the center of the disturbance at 41°N.
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Introduction

Chapter in , Informa UK Limited 105:2-3 (2011) 113-116

Authors:

John Brindley, Peter Read, John Gibbon, Andrew Soward
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A laboratory study of global-scale wave interactions in baroclinic flow with topography I: multiple flow regimes

GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS 105:2-3 (2011) PII 934802668

Authors:

PL Read, SH Risch
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Corrigendum to "Breeding and predictability in the baroclinic rotating annulus using a perfect model" published in Nonlin. Processes Geophys., 15, 469–487, 2008

Nonlin. Proc. Geophys. Copernicus Publications 18 (2011) 359-359

Authors:

RMB Young, PL Read

Abstract:

No abstract.
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