S
Stanley W. H. Cowley
Researcher at University of Leicester
Publications - 505
Citations - 24768
Stanley W. H. Cowley is an academic researcher from University of Leicester. The author has contributed to research in topics: Magnetosphere & Solar wind. The author has an hindex of 83, co-authored 504 publications receiving 23457 citations. Previous affiliations of Stanley W. H. Cowley include European Space Research and Technology Centre & Imperial College London.
Papers
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Observations at the magnetopause and in the auroral ionosphere of momentum transfer from the solar wind
TL;DR: In this article, it was shown that there is very little convection "flywheel" effect in the dayside polar ionosphere and that only newly-opened flux tubes impart significant momentum to the ionosphere, in a relatively narrow region immediately poleward of the cusp.
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Rosetta and Mars Express observations of the influence of high solar wind pressure on the Martian plasma environment
Niklas J. T. Edberg,Niklas J. T. Edberg,U. Auster,S. Barabash,A. Bößwetter,David Brain,James L. Burch,Chris Carr,Stanley W. H. Cowley,Emanuele Cupido,Firdevs Duru,Anders Eriksson,Markus Fränz,Karl-Heinz Glassmeier,Karl-Heinz Glassmeier,Raymond Goldstein,Mark Lester,Rickard Lundin,Ronan Modolo,Hans Nilsson,Ingo Richter,M. Samara,Jean-Gabriel Trotignon +22 more
TL;DR: In this article, the authors report on new simultaneous in-situ observations at Mars from Rosetta and Mars Express (MEX) on how the Martian plasma environment is affected by high pressure solar wind.
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Cassini nightside observations of the oscillatory motion of Saturn's northern auroral oval
Emma J. Bunce,Denis Grodent,S. L. Jinks,David Andrews,Sarah V. Badman,Andrew J. Coates,Andrew J. Coates,Stanley W. H. Cowley,Michele K. Dougherty,William S. Kurth,D. G. Mitchell,G. Provan +11 more
TL;DR: In this paper, the motion of the auroral oval evident from the UVIS images requires a careful interpretation of the associated latitudinally "oscillating" magnetic field and auroral field-aligned current signatures, whereas previous interpretations have assumed a static current system.
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Response of Uranus' auroras to solar wind compressions at equinox
TL;DR: The work in this article was stimulated by observations made by the NASA/ESA Hubble Space Telescope (GO Program 12601) and was supported by STFC grants ST/H002480/1 and ST/K001000/1.
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Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field model
TL;DR: In this article, the field-aligned mapping of Saturn's auroras into the magnetosphere was determined by combining UV images of the southern dayside oval obtained by the Hubble Space Telescope (HST) with a global model of the magnetospheric magnetic field.