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Juno Jupiter image

Neil Bowles

Professor of Planetary Science

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Planetary atmosphere observation analysis
  • Planetary surfaces
  • Solar system
  • Space instrumentation
Neil.Bowles@physics.ox.ac.uk
Telephone: 01865 (2)72097
Atmospheric Physics Clarendon Laboratory, room 307
  • About
  • Publications

The Long wave (11–16 μm) spectrograph for the EChO M3 Mission Candidate study

Experimental Astronomy Springer Nature 40:2-3 (2015) 801-811

Authors:

NE Bowles, M Tecza, JK Barstow, JM Temple, PGJ Irwin, LN Fletcher, S Calcutt, J Hurley, M Ferlet, D Freeman

The transit spectra of Earth and Jupiter

Icarus Elsevier 242 (2014) 172-187

Authors:

PGJ Irwin, JK Barstow, NE Bowles, LN Fletcher, S Aigrain, J-M Lee

Modelling of an asteroid photoelectron sheath and implications for a sample return mission

Planetary and Space Science Elsevier 99 (2014) 103-111

Authors:

KL Aplin, AJ Macfaden, NE Bowles

Design and performance of the Exo-planet Characterisation Observatory (EChO) integrated payload

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 9143 (2014) 91432e-91432e-12

Authors:

Bruce Swinyard, Marcel Tessenyi, Giovanna Tinetti, Ingo Waldmann, Paul Eccleston, Marc Ferlet, Ranah Irshad, Tanya Lim, Kevin Middleton, Tom Bradshaw, Martin Crook, Tom Hunt, Berend Winter, Ian Bryson, Naidu Bezawada, William Taylor, Neil Bowles, Enzo Pascale, Gianluca Morgante, Emanuele Pace, Alberto Adriani, Jean-Michel Reess, Pierre Drossart, Vincent Coudé du Foresto, Marc Ollivier, Roland Ottensamer, Mirek Rataj, Gonzalo Ramos Zapata, Jan-Rutger Schrader, Avri Selig, Kate Isaak, Martin Linder, Ludovic Puig, Paul Hartogh, Christophe Lovis, Giusi Micela, Ignasi Ribas, Ignas Snellen, Jean-Phillippe Beaulieu

An innovative satellite mission concept to measure the effects of aerosols on clouds and climate

Bulletin of the American Meteorological Society 94:5 (2013) 685-694

Authors:

NO Rennó, E Williams, D Rosenfeld, DG Fischer, J Fischer, T Kremic, A Agr Awal, MO Andreae, R Bierbaum, R Blakeslee, A Boerner, N Bowles, H Christian, A Cox, J Dunion, A Horvath, X Huang, A Khain, S Kinne, MC Lemos, JE Penner, U Pöschl, J Quaas, E Seran, B Stevens, T Walati, T Wagner

Abstract:

The Clouds, Hazards, and Aerosols Survey for Earth Researchers (CHASER) satellite mission concept responds to the IPCC and Decadal Survey concerns by studying the activation of CCN and their interactions with clouds and storms. The CHASER satellite mission was developed to remotely sense quantities necessary for determining the interactions of aerosols with clouds and storms. CHASER will make the first global survey of Na, the activated CCN spectrum, and the vertical profiles of cloud properties directly affecting climate. CHASER will complement and transcend current National Aeronautics and Space Administration (NASA) Earth Science Missions studying aerosols, clouds, and thunderstorms. CHASER will determine vertical profiles of cloud parameters and lightning flashes pointing 30° off track toward sun-illuminated cloud surfaces, which minimizes shadowing. CHASER will use a high-heritage Cloud Profiler Suite (CPS) consisting of two instruments pointing 30° off nadir across track toward sun-illuminated surfaces on the east.

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