Statistics – Methodology
Scientist
Statistics
Methodology
Scientist
Department of Physics, Oxford University, Oxford, UK
Department of Physics, Oxford University, Oxford OX1 3PU, UK
Atmospheric Physics, Oxford University, Oxford, United Kingdom;
AOPP, Oxford University
Atmospheric, Oceanic and Planetary Physics, Oxford University, Clarendon Laboratory, Parks Road, Oxford, OX13PU
Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, University of Oxford, Parks Road, Oxford, UK
University of Oxford, United Kingdom
Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, University of Oxford, United Kingdom
Oxford University, UK
Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Parks Road, Oxford, Oxf OX1 3PU, United Kingdom
Department of Atmospheric, Oceanic and Planetary Physics, Oxford University, Parks Road, Oxford, OX1 3PU United Kingdom
Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Oxford, UK
Atmospheric, Oceanic, and Planetary Physics, Clarendon Laboratory, University of Oxford, Oxford, UK
Atmospheric, Oceanic and Planetary Physics, University of Oxford, U.K.
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
Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, University of Oxford, UK
Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, Department of Physics, University of Oxford, Oxford, UK
Clarendon Laboratory, Department of Atmospheric, Oceanic and Planetary Physics, University of Oxford, Oxford, UK
Department of Physics, University of Oxford, Clarendon Laboratory, Parks Road, Oxford, UK
A correlated-k model of radiative transfer in the near-infrared windows of Venus
A new Wind Sensor for the Beagle 2 Mars Lander
A new Wind Sensor for the Beagle 2 Mars Lander
A wind tunnel for the calibration of Mars wind sensors
Analysis of thermal emission from the nightside of Venus at 1.51 and 1.55 μm
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