Physics
Scientist
Department of Earth and Ocean Sciences, University of Liverpool, 4 Brownlow Street, Liverpool, L69 3GP United Kingdom r.t.
Department of Geology and Geophysics, University of Edinburgh, Edinburgh, UK
GeoForschungsZentrum Potsdam, Telegrafenberg, D-14473 Potsdam, Germany Université d'Avignon et des Pays de Vaucluse, La Grande Combe, F-84400 Rustrel, France
Department of Earth and Ocean Sciences, University of Liverpool, Liverpool, UK
Department of Earth Sciences, The Jane Herdman Laboratories, The University of Liverpool, 4 Brownlow Street, L69 3GP, Liverpool, UK
Department of Earth and Ocean Sciences, University of Liverpool, UK
GeoForschungsZentrum Potsdam, Telegrafenberg, D-14473 Potsdam, Germany of Liverpool, Department of Earth and Ocean Sciences, Liverpool, UK
GeoForschungsZentrum Potsdam, Telegrafenberg, D-14473 Potsdam, Germany
Department of Earth and Ocean Sciences, University of Liverpool, 4 Brownlow Street, Liverpool L69 36P, UK.
University of Liverpool, Geomagnetism Laboratory, Department of Earth and Ocean Sciences, University of Liverpool, Liverpool, L69 7ZE, United Kingdom
University of Liverpool, Department of Earth and Ocean Sciences 4 Brownlow Street, Liverpool, L69 3GP, United Kingdom
School of Environmental Sciences, University of Liverpool, Liverpool L69 3GP, UK
School of Environmental Sciences, University of Liverpool, L69 3GP, UK.
Department of Earth and Ocean Sciences, University of Liverpool, 4 Brownlow St., Liverpool, L69 3GP, England
Department of Earth and Ocean Sciences, University of Liverpool, Liverpool, United Kingdom of Earth and Ocean Sciences, University of Liverpool, UK.
Department of Earth and Ocean Sciences, Geomagnetism Laboratory, Oliver Lodge Building, Oxford Street, University of Liverpool, Liverpool L69 7Z
A comparison of Cluster magnetic data with the Tsyganenko 2001 model
An explanation for the shape of Earth's gravity spectrum based on viscous mantle flow models
Baroclinic instability in the interiors of the giant planets: A cooling history of Uranus?
Baroclinic Instability in the Interiors of the Giant Planets: A Mechanism for Depleting the Internal Energy of Uranus
Book review
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