Radiometer for the measurement of water vapor in the upper atmosphere from space.
Appl Opt 32:33 (1993) 6764-6776
Abstract:
We describe the design, the development, and the calibration of a radiometer to measure water vapor abundance in the middle atmosphere, using the solar occultation technique from an orbiting platform. The use of gas cells containing water vapor and carbon dioxide leads to a relatively simple, but sensitive, design. This radiometer is shown to be capable of detecting water vapor in the mesosphere, where, because of dissociation by the Sun, the amounts are very small, of the order of 1 part per 10(6) or less. A flight version of the instrument will be launched in 1992 on board the European Retrievable Carrier space platform, and the data will be employed for a better understanding of the Earth's water budget.Investigation of dielectric spaced resonant mesh filter designs for PMIRR
Infrared Physics 34:6 (1993) 549-563
Abstract:
The fabrication of the filters for the two longest wave channels of the Pressure Modulator Infra-red Radiometer (PMIRR), launched in September 1992 on Mars Observer, was not possible using conventional multilayer dielectric techniques. Thus the extension of far-infrared/microwave mesh filter designs was investigated using a new dielectric spacing material. Test filters were designed and fabricated and, using their measured transmission spectra, a new model of the behaviour of resonant meshes in both air and dielectrics was developed. The low transmission of these filters in the end made them unsuitable for PMIRR but the model provides a useful design tool for future dielectric spaced filters providing a new, less absorbing dielectric can be found. © 1993.EARTH GLOBAL MOSAIC OBSERVATIONS WITH NIMS-GALILEO
PLANETARY AND SPACE SCIENCE 41:7 (1993) 551-561
LATITUDINAL DISTRIBUTION OF CARBON-MONOXIDE IN THE DEEP ATMOSPHERE OF VENUS
PLANETARY AND SPACE SCIENCE 41:7 (1993) 487-494
SEARCH FOR SPATIAL VARIATIONS OF THE H2O ABUNDANCE IN THE LOWER ATMOSPHERE OF VENUS FROM NIMS-GALILEO
PLANETARY AND SPACE SCIENCE 41:7 (1993) 495-504