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Galileo Probe Nephelometer experiment
Authors:B Ragent  C A Privette  P Avrin  J G Waring  C E Carlston  T C D Knight  J P Martin
Institution:(1) San Jose State University Foundation, 95192-0139 San Jose, CA, USA;(2) NASA Ames Research Center, 94035 Moffett Field, CA, USA;(3) Martin Marietta Astronautics Group, 80201 Denver, CO, USA
Abstract:The objective of the Nephelometer Experient aboard the Probe of the Galileo mission is to explore the vertical structure and microphysical properties of the clouds and hazes in the atmosphere of Jupiter along the descent trajectory of the Probe (nominally from 0.1 to > 10 bars). The measurements, to be obtained at least every kilometer of the Probe descent, will provide the bases for inferences of mean particle sizes, particle number densities (and hence, opacities, mass densities, and columnar mass loading) and, for non-highly absorbing particles, for distinguishing between solid and liquid particles. These quantities, especially the location of the cloud bases, together with other quantities derived from this and other experiments aboard the Probe, will not only yield strong evidence for the composition of the particles, but, using thermochemical models, for species abundances as well. The measurements in the upper troposphere will provide lsquoground truthrsquo data for correlation with remote sensing instruments aboard the Galileo Orbiter vehicle. The instrument is carefully designed and calibrated to measure the light scattering properties of the particulate clouds and hazes at scattering angles of 5.8°, 16°, 40°, 70°, and 178°. The measurement sensitivity and accuracy is such that useful estimates of mean particle radii in the range from about 0.2 to 20 mgr can be inferred. The instrument will detect the presence of typical cloud particles with radii of about 1.0 mgr, or larger, at concentrations of less than 1 cm3.Deceased.
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