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Juno Jupiter image

Simon Calcutt

Emeritus

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Planetary atmosphere observation analysis
  • Solar system
  • Space instrumentation
  • Planetary surfaces
simon.calcutt@physics.ox.ac.uk
Telephone: 01865 (2)72916
Atmospheric Physics Clarendon Laboratory, room 308
  • About
  • Publications

The Hera Saturn entry probe mission

PLANETARY AND SPACE SCIENCE 130 (2016) 80-103

Authors:

O Mousis, DH Atkinson, T Spilker, E Venkatapathy, J Poncy, R Frampton, A Coustenis, K Reh, J-P Lebreton, LN Fletcher, R Hueso, MJ Amato, A Colaprete, F Ferri, D Stam, P Wurz, S Atreya, S Aslam, DJ Banfield, S Calcutt, G Fischer, A Holland, C Keller, E Kessler, M Leese, P Levacher, A Morse, O Munoz, J-B Renard, S Sheridan, F-X Schmider, F Snik, JH Waite, M Bird, T Cavalie, M Deleuil, J Fortney, D Gautier, T Guillot, JI Lunine, B Marty, C Nixon, GS Orton, A Sanchez-Lavega
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Dual-telescope multi-channel thermal-infrared radiometer for outer planet fly-by missions

Acta Astronautica Elsevier 128 (2016) 628-639

Authors:

Shahid Aslam, Michael Amato, Neil Bowles, Simon Calcutt, Tilak Hewagama, Joseph Howard, Carly Howett, Wen-Ting Hsieh, Terry Hurford, Jane Hurley, Patrick Irwin, Donald E Jennings, Ernst Kessler, Brook Lakew, Mark Loeffler, Michael Mellon, Anthony Nicoletti, Conor A Nixon, Nathaniel Putzig, Gerard Quilligan, Julie Rathbun, Marcia Segura, John Spencer, Joseph Spitale, Garrett West

Abstract:

The design of a versatile dual-telescope thermal-infrared radiometer spanning the spectral wavelength range 8–200 µm, in five spectral pass bands, for outer planet fly-by missions is described. The dual-telescope design switches between a narrow-field-of-view and a wide-field-of-view to provide optimal spatial resolution images within a range of spacecraft encounters to the target. The switchable dual-field-of-view system uses an optical configuration based on the axial rotation of a source-select mirror along the optical axis. The optical design, spectral performance, radiometric accuracy, and retrieval estimates of the instrument are discussed. This is followed by an assessment of the surface coverage performance at various spatial resolutions by using the planned NASA Europa Mission 13-F7 fly-by trajectories as a case study.
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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
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On the detectability of trace chemical species in the martian atmosphere using gas correlation filter radiometry

Icarus Elsevier 260 (2015) 103-127

Authors:

JA Sinclair, PGJ Irwin, SB Calcutt, EL Wilson
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EVOLUTION OF THE FAR-INFRARED CLOUD AT TITAN’S SOUTH POLE

The Astrophysical Journal Letters American Astronomical Society 804:2 (2015) l34

Authors:

Donald E Jennings, RK Achterberg, V Cottini, CM Anderson, FM Flasar, CA Nixon, GL Bjoraker, VG Kunde, RC Carlson, E Guandique, MS Kaelberer, JS Tingley, SA Albright, ME Segura, R de Kok, A Coustenis, S Vinatier, G Bampasidis, NA Teanby, S Calcutt
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