Simon Calcutt: Publications

The atmosphere of Mars

JBIS - Journal of the British Interplanetary Society 52:5-6 (1999) 209-216

Authors:

PGJ Irwin, SB Calcutt, FW Taylor, DJ McCleese

Abstract:

Mars, one of the most Earth-like of the planets, is today a cold, dry and barren world. However, there is good evidence that it may have been much warmer and wetter in the past and perhaps even 91̽��ed life. The public interest aroused by these findings and by recent studies of 'SNC' meteorites, believed to have come from Mars, with their claims of the evidence of ancient Martian life, has focused attention on the ambitious programme of Mars Exploration currently being undertaken by NASA and ESA and has provided additional impetus. Improved measurements of the conditions on Mars' surface and in its atmosphere are central to both agencies' plans, and current atmospheric missions are reviewed in this paper together with possible future designs.

Jovian atmospheric studies with the Galileo near infrared mapping spectrometer: An update

Advances in Space Research Elsevier 23:9 (1999) 1623-1632

Authors:

PGJ Irwin, FW Taylor, RW Carlson, KH Baines, A Weir, P Cameron-Smith, S Calcutt, T Encrenaz, P Drossart, M Roos-Serote, E Lellouch

Network science landers for Mars

Advances in Space Research Elsevier 23:11 (1999) 1915-1924

Authors:

A-M Harri, O Marsal, P Lognonne, GW Leppelmeier, T Spohn, K-H Glassmeier, F Angrilli, WB Banerdt, JP Barriot, J-L Bertaux, JJ Berthelier, S Calcutt, JC Cerisier, D Crisp, V Dehant, D Giardini, R Jaumann, Y Langevin, M Menvielle, G Musmann, JP Pommereau, S Di Pippo, D Guerrier, K Kumpulainen, S Larsen, A Mocquet, J Polkko, J Runavot, W Schumacher, T Siili, J Simola, JE Tillman, NetLander Team

Band parameters and k coefficients for self-broadened ammonia in the range 4000-11000 cm^-1

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER 62:2 (1999) 193-204

Authors:

PGJ Irwin, SB Calcutt, K Sihra, FW Taylor, AL Weir, J Ballard, WB Johnston

Analysis of Jupiter north equatorial belt hot spots in the 4–5 μm range from Galileo/near‐infrared mapping spectrometer observations: Measurements of cloud opacity, water, and ammonia

Journal of Geophysical Research American Geophysical Union (AGU) 103:E10 (1998) 23023-23041

Authors:

M Roos‐Serote, P Drossart, T Encrenaz, E Lellouch, RW Carlson, KH Baines, L Kamp, R Mehlman, GS Orton, S Calcutt, P Irwin, F Taylor, A Weir

91̽��

Simon Calcutt

Sub department

The atmosphere of Mars

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Abstract:

Jovian atmospheric studies with the Galileo near infrared mapping spectrometer: An update

Authors:

Network science landers for Mars

Authors:

Band parameters and k coefficients for self-broadened ammonia in the range 4000-11000 cm^-1

Authors:

Analysis of Jupiter north equatorial belt hot spots in the 4–5 μm range from Galileo/near‐infrared mapping spectrometer observations: Measurements of cloud opacity, water, and ammonia

Authors:

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Simon Calcutt

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The atmosphere of Mars

Authors:

Abstract:

Jovian atmospheric studies with the Galileo near infrared mapping spectrometer: An update

Authors:

Network science landers for Mars

Authors:

Band parameters and k coefficients for self-broadened ammonia in the range 4000-11000 cm-1

Authors:

Analysis of Jupiter north equatorial belt hot spots in the 4–5 μm range from Galileo/near‐infrared mapping spectrometer observations: Measurements of cloud opacity, water, and ammonia

Authors:

Band parameters and k coefficients for self-broadened ammonia in the range 4000-11000 cm^-1