An Evaluation of the TOPSAR Topographic SAR Interferometer Performance
Evaluation based on standard TOPSAR product with 10m pixel spacing.
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Evaluation based on standard TOPSAR product with 10m pixel spacing.
Existing and new mode shape expansion methods are presented within the framework of least squares minimization techniques with quadratic inequality constraints.
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Reliable prediction of stellar diameters, particularly angular diameters, is a useful and necessary tool for the increasing number of milliarcsecond resolution studies being carried out in the astronomical community.
If the dust content of nearby solar system is comparable to, or larger than, that of our own zodiacal disk, the thermal emission from exozodiacal disks will significantly outshine planetary companions to nearby stars.
Future NASA missions in astrophysics, Earth observation, and solar system exploration that require optical communication optical and infrared imaging, or high precision astrometric measurements impose very stringent demands for the dimensional stability issues included: the cassini Imaging Science Subsystem (ISS) and the Space Infrared Telescope (SIRTF). Longer range mission plans call for even more stringent dimensional stability. JPL has identified twenty-six proposed missions with critical dimensional stability requirements.
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A corner cube (CC) articulation model has been developed to evaluate the SIM internal metrology (IntMet) optical delay bias (with the accuracy of picometer) due to the component imperfections, such as vertex offset, reflection coating index error, dihedral error, and surface figure error at each facet. This physics-based and MATLAB-implemented geometric optics model provides useful guidance on the flight system design, integration, and characterization. The first portion of this paper covers the CC model details. Then several feature of the model, such as metrology beam footprint visualization, roofline straddling/crossing analysis, and application to drive the sub-system design and the error budget flow-down, are demonstrated in the second part.
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