The ORA occultation radiometer on EURECA. Instrument description and preliminary results

ADV SPACE RES 16:8 (1995) 33-36

Authors:

E ARIJS, D NEVEJANS, D FUSSEN, P FREDERICK, E VANRANSBEECK, FW TAYLOR, SB CALCUTT, ST WERRETT, CL HEPPLEWHITE, TM PRITCHARD, I BURCHELL, CD RODGERS

Abstract:

A short description is given of the Occultation Radiometer which has been flown recently on the EURECA carrier. A brief outline of the scientific rationale, instrument characteristics and status of the data reduction is presented.

VESAT: The Venus Environmental Satellite Discovery mission

Acta Astronautica Elsevier 35 (1995) 417-426

Authors:

KH Baines, RW Carlson, D Crisp, JT Schofield, B Bézard, C de Bergh, P Drossart, WA Delamere, B Fegley, WH Smith, SJ Limaye, CT Russell, G Schubert, S Calcutt, FW Taylor

VIRTIS, visible InfraRed thermal imaging spectrometer for the ROSETTA mission

(1995) 1604-1606

Authors:

A CORADINI, F CAPACCIONI, MT CAPRIA, P CERRONI, MC DESANCTIS, G MAGNI, R BONSIGNORI, F REININGER, T ENCRENAZ, P DROSSART, A SEMERY, G ARNOLD, H MICHAELIS, FW TAYLOR, SB CALCUTT, TJ VELLACOTT, P VENTERS, REJ WATKINS

The deep atmosphere of Venus

PHILOS T ROY SOC A 349:1690 (1994) 273-283

Authors:

SB CALCUTT, FW TAYLOR

Abstract:

Venus as a planet resembles the Earth, but has a much hotter and denser atmosphere due to an extreme case of the greenhouse effect, caused by compositional differences and tile thick cloud cover. Studies of the lower atmosphere are inhibited by the cloud opacity, which makes remote measurements at most frequencies short. of the radio range quite difficult. Progress in understanding of the com position and thermal structure below the clouds has been made by the Pioneer and Venera entry probes of the 1970s, and more recently with results from the Galileo fly-by in 1990. The latter exploited the newly discovered near-infrared 'windows' to achieve measurements of carbon monoxide and water vapour abundances in the deep atmosphere, and provided the first detailed view of the global cloud structure. The morphology and spatial variations seen in the main mass of clouds are remarkable, and suggest a powerful and diverse meteorology dominated by convection. Carbon monoxide is significantly more abundant at high northern latitudes than at low latitudes in either hemisphere.

Characterization of the thermodynamic behaviour of pressure modulated cells for remote sensing of the atmosphere of Mars

Journal of Quantitative Spectroscopy and Radiative Transfer 52:1 (1994) 1-20

Authors:

PGJ Irwin, SB Calcutt, FW Taylor

Abstract:

A radiometric experiment was conducted to investigate the thermodynamic behaviour of the H2O and CO2 pressure modulated cells of the Pressure Modulator Infrared Radiometer (PMIRR) which flew on "Mars Observer" in 1992. The wave forms and phases of the transmission, emission, pressure and piston position cycles, together with the mean absorption were, for the first time, all measured during the same experiment. The measured transmission and emission cycles were used to calculate the phase and amplitude of the temperature cycles and were found to be super-adiabatic for both cells, in reasonable agreement with a thermal diffusion model. Anomalies were seen in the H2O modulator driving frequency, as has been observed by other authors, but none were evident in the measured cell wave forms suggesting that the water vapour behaves as an ideal gas in the cell. © 1994.