Near-Infrared Spectroscopy and Spectral Mapping of Jupiter and the Galilean Satellites: Results from Galileo's Initial Orbit
Science American Association for the Advancement of Science (AAAS) 274:5286 (1996) 385-388
Calculated k distribution coefficients for hydrogen- And self-broadened methane in the range 2000-9500 cm-1 from exponential sum fitting to band-modelled spectra
Journal of Geophysical Research: Planets 101:E11 (1996) 26137-26154
Abstract:
The spectral band data derived by Strong et al. [1993] for laboratory-measured transmission spectra of hydrogen-broadened methane at 10 cm-1 resolution have been fitted with k coefficients over a wide range of pressures and temperatures representing those likely to be encountered in the atmosphere of Jupiter. The mean fitting error is found to be only 2.0脳10-3 in transmission. These data are essential for the scattering calculations likely to be necessary for analysis of the data from the Near Infrared Mapping Spectrometer aboard the NASA Galileo spacecraft. The new data have significant advantages over those previously derived by Baines et al. [1993] in that they cover a wider spectral range, are applicable to longer paths, and also apply to the hydrogen-broadened case, which is the dominant broadening mechanism in this atmosphere. A similar table has also been calculated for the self-broadening case for comparison. Copyright 1996 by the American Geophysical Union.Remote sounding of the Martian atmosphere in the context of the InterMarsNet mission: General circulation and meteorology
Planetary and Space Science 44:11 SPEC. ISS. (1996) 1347-1360
Abstract:
A concept has been developed for a remote sensing experiment to investigate the physics of the Martian atmosphere from a spin-stabilized orbiter, like that planned for the InterMarsNet mission. Using coincident infrared and microwave channels and limb-to-limb scanning, it can map the planet much more extensively than previously in temperature, atmospheric dust loading, and humidity. When combined with one or more surface stations measuring the same variables, the sounder experiment can contribute to major progress in understanding the general circulation and dust and water cycles of the atmosphere of Mars, and the characterization of medium-scale meteorological systems. Copyright 漏 1996 Elsevier Science Ltd.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
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. 漏 1994.Investigation of dielectric spaced resonant mesh filter designs for PMIRR
Infrared Physics 34:6 (1993) 549-563