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- W2048180873 abstract "Using the data from Veneras 4–8 and Mariners 5 and 10 related to the composition and structure of the atmosphere of Venus, the three scans obtained with the microwave radiometer on Mariner 2 at a wavelength of 1.9 cm have been reanalyzed. In the previous analysis of the microwave data, both the percentage of Co 2 and the surface pressures were considerably lower than the in situ measurements and the assumed longitudinal temperature gradient was much larger than indicated by more recent measurements. Using these more recent data, it has not been possible to match the measured scan ratios with or without any spherically symmetric distribution of microwave cloud absorber. The scan ratios, therefore, require the existence of different average values of microwave cloud opacity for each scan. In addition, the anomalous temperature drop observed in the south polar region of the terminator scan has been found to require a very opaque microwave cloud in the local zenith angle range of 40°–70°. This type of distribution is consistent with the trend seen in the Mariner 2 infrared terminator scan suggesting some degree of coupling between the infrared and microwave clouds. It is suggested that some of the variability seen in the earth-based interferometer data may be a result of changes in the distribution of the microwave clouds over the disc of the planet." @default.
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- W2048180873 title "Evidence for the nonuniform distribution of microwave attentuating clouds in the atmosphere of Venus: Mariner 2" @default.
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