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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

HARMONI: a single-field wide-band integral-field spectrograph for the European ELT

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 7735 (2010) 77352i-77352i-11

Authors:

Niranjan Thatte, Mathias Tecza, Fraser Clarke, Roger L Davies, Alban Remillieux, Roland Bacon, David Lunney, Santiago Arribas, Evencio Mediavilla, Fernando Gago, Naidu Bezawada, Pierre Ferruit, Ana Fragoso, David Freeman, Javier Fuentes, Thierry Fusco, Angus Gallie, Adolfo Garcia, Timothy Goodsall, Felix Gracia, Aurelien Jarno, Johan Kosmalski, James Lynn, Stuart McLay, David Montgomery, Arlette Pecontal, Hermine Schnetler, Harry Smith, Dario Sosa, Giuseppina Battaglia, Neil Bowles, Luis Colina, Eric Emsellem, Ana Garcia-Perez, Szymon Gladysz, Isobel Hook, Patrick Irwin, Matt Jarvis, Robert Kennicutt, Andrew Levan, Andy Longmore, John Magorrian, Mark McCaughrean, Livia Origlia, Rafael Rebolo, Dimitra Rigopoulou, Sean Ryan, Mark Swinbank, Nial Tanvir, Eline Tolstoy, Aprajita Verma
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The future of planetary geophysics

Astronomy & Geophysics Oxford University Press (OUP) 51:2 (2010) 2.22-2.25

Authors:

Nick Teanby, Neil Bowles
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The lunar reconnaissance orbiter diviner lunar radiometer experiment

Space Science Reviews 150:1-4 (2010) 125-160

Authors:

DA Paige, MC Foote, BT Greenhagen, JT Schofield, S Calcutt, AR Vasavada, DJ Preston, FW Taylor, CC Allen, KJ Snook, BM Jakosky, BC Murray, LA Soderblom, B Jau, S Loring, J Bulharowski, NE Bowles, IR Thomas, MT Sullivan, C Avis, EM De Jong, W Hartford, DJ McCleese

Abstract:

The Diviner Lunar Radiometer Experiment on NASA's Lunar Reconnaissance Orbiter will be the first instrument to systematically map the global thermal state of the Moon and its diurnal and seasonal variability. Diviner will measure reflected solar and emitted infrared radiation in nine spectral channels with wavelengths ranging from 0.3 to 400 microns. The resulting measurements will enable characterization of the lunar thermal environment, mapping surface properties such as thermal inertia, rock abundance and silicate mineralogy, and determination of the locations and temperatures of volatile cold traps in the lunar polar regions. © The author(s) 2009.
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Global Silicate Mineralogy of the Moon from the Diviner Lunar Radiometer

SCIENCE 329:5998 (2010) 1507-1509

Authors:

Benjamin T Greenhagen, Paul G Lucey, Michael B Wyatt, Timothy D Glotch, Carlton C Allen, Jessica A Arnold, Joshua L Bandfield, Neil E Bowles, Kerri L Donaldson Hanna, Paul O Hayne, Eugenie Song, Ian R Thomas, David A Paige
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The Lunar Reconnaissance Orbiter Diviner Lunar Radiometer Experiment

SPACE SCIENCE REVIEWS 150:1-4 (2010) 125-160

Authors:

DA Paige, MC Foote, BT Greenhagen, JT Schofield, S Calcutt, AR Vasavada, DJ Preston, FW Taylor, CC Allen, KJ Snook, BM Jakosky, BC Murray, LA Soderblom, B Jau, S Loring, J Bulharowski, NE Bowles, IR Thomas, MT Sullivan, C Avis, EM De Jong, W Hartford, DJ McCleese
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