Statistics – Methodology
Scientist
Statistics
Methodology
Scientist
Department of Physics, Oxford University, Oxford, UK
Atmospheric, Oceanic and Planetary Physics, Oxford University, Clarendon Laboratory, Parks Road, Oxford, OX13PU
Atmospheric, Oceanic, and Planetary Physics, Department of Physics, Clarendon Laboratory, University of Oxford, Oxford, UK
Southwest Research Institute
Southwest Research Inst
Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, University of Oxford, United Kingdom
Atmospheric, Oceanic, and Planetary Physics, Clarendon Laboratory, University of Oxford, Oxford, UK
Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302, USA
Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Parks Road, Oxford, Oxon, OX1 3PU, UK
Atmospheric, Oceanic, and Planetary Physics, University of Oxford, Clarendon Laboratory, Parks Rd, Oxford, OX1 3PU, UK
Department of Space Studies, Southwest Research Institute, Boulder, CO 80302, USA
Oxford Univ., United Kingdom
Southwest Research Institute, San Antonio, TX, USA
Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Parks Road, Oxford, Oxf OX1 3PU, United Kingdom
Southwest Research Institute, Boulder, CO, USA
University of Oxford, United Kingdom
Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Oxford, UK
Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, Department of Physics, University of Oxford, Oxford, UK
Department of Space Studies, Southwest Research Institute, 1050 Walnut St., Suite 300, Boulder, CO 80302, USA
Clarendon Laboratory, Department of Atmospheric, Oceanic and Planetary Physics, University of Oxford, Oxford, UK
A correlated-k model of radiative transfer in the near-infrared windows of Venus
A dynamic upper atmosphere of Venus as revealed by VIRTIS on Venus Express
An approach to study the cosmic ray 'knee' composition from underground multimuon events at a shallower depth.
Analysis of thermal emission from the nightside of Venus at 1.51 and 1.55 μm
Composition of the Venusian atmosphere after Venus Express
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