Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Atmospheric Physics Laboratory, Department of Physics and Astronomy, University College London, London, UK
A.P.L., University College London
Department of Physics and Astronomy, University College London, London, United Kingdom; College, London
Atmospheric Physics Laboratory, University College London, 67-73 Riding House Street London W1P 7PP, UK of Physics and Astronomy, University College London, London, of Physics and Astronomy, University College London, London, United Kingdom of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom Physics Laboratory, University College London London W1P 7PP, UK
Atmospheric Physics Laboratory, University College, London, UK
Department of Physics and Astronomy, University College London
Department of Physics and Astronomy, University College London, WC1E 6BT, UK
Atmospheric Physics Laboratory, University College London 67-73 Riding House Street, W1P 7PP, London, UK
Atmospheric Physics Laboratory, University COllege London, 67-73 Riding House Street, London, W1P 7PP United Kingdom of Physics and Astronomy, University College London, London WC1E 6BT, UK Physics Laboratory, Department of Physics and Astronomy, University College, London, UK
Atmospheric Physics Laboratory, University College London, 67-73 Riding House Street, London W1P 7PP, UK
Atmospheric Physics Laboratory, University College London, 67-73 Riding House Street, London, W1W 7EJ United Kingdom College London, Atmospheric Physics Laboratory, 67-73 Riding House Street, London, W1W 7EJ United Kingdom
Atmospheric Physics Laboratory, Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom. s.
Department of Physics and Astronomy, University College
3D Simulations of the Upper Atmosphere and Ionosphere of HD17156b
A fast computation of the secondary ion production in the ionosphere of Mars
A global circulation model of Saturn's thermosphere
A stability limit for the atmospheres of giant extrasolar planets
A study into the effect of the diurnal tide on the structure of the background mesosphere and thermosphere using the new coupled middle atmosphere and thermosphere (CMAT) general circulation model
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