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FIGURE 6.28 Predictive monitoring system would concentrate on the few sensor outputs that are most important at the moment.
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state of the system, and perhaps some future scheduled events. The outputs of the causal simulator would include a set of predicted events and a graph of causal dependency among events. The sensor planner would use the causal dependency graph generated by the causal simulator to determine which few of all the predicted events are important enough that they should be verified. In many cases, the most important events would be taken to be those that either caused, or are caused by, the greatest number of other events. This notion of causal importance would serve as the basis for the election of those sensors, the outputs of which should be used to verify the expected behavior of the system. The sensor interpreter would compare the actual outputs of the selected sensors with the values of those outputs predicted by the causal simulator. Alarms would be raised where the discrepancies between predicted and actual values were significant.
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Reflective Strip Imaging Camera Sensor Measuring a 180 -Wide Angle
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A proposed camera sensor would image a thin striplike portion of a field of view 180 wide. For example, it could be oriented to look at the horizon in an easterly direction from north to south or it could be rotated about a horizontal north/south axis to make a pushbroom scan of the entire sky proceeding from the easterly toward the westerly half of the horizon. Potential uses for the camera sensor include surveillance of clouds, coarse mapping of terrain, measurements of
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FIGURE 6.29 A thin segment of a hemispherical concave re ector would form an image from a 180 strip eld of view onto optical bers.
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the bidirectional reflectance distribution functions of aerosols, imaging spectrometry, oceanography, and exploration of the planets. The imaging optics would be a segment of concave hemispherical reflecting surfaces placed slightly off center (Fig. 6.29). Like other reflecting optics, it would be achromatic. The unique optical configuration would practically eliminate geometric distortion of the image. The optical structure could be fabricated and athermalized fairly easily in that it could be machined out of one or a few pieces of metal, and the spherical reflecting surface could be finished by diamond turning. In comparison, a camera sensor with a fish-eye lens, which provides a nearly hemispherical field of view, exhibits distortion, chromatism, and poor athermalization. The image would be formed on a thin semicircular strip at half the radius of the sphere. A coherent bundle of optical fibers would collect the light from this strip and transfer the image to a linear or rectangular array of photodetectors or to the entrance slit of an image spectrograph. Provided that the input ends of the fibers were properly aimed, the cones of acceptance of the fibers would act as aperture stops. Typically, the resulting width of the effective aperture of the camera sensor would be about onethird the focal length (f/3).
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The camera sensor would operate at wavelengths from 500 to 1100 nm. The angular resolution would be about 0.5 . In the case of an effective aperture of f/3, the camera would provide an unvignetted view over the middle 161 of the strip, with up to 50 percent vignetting in the outermost 9.5 on each end. The decentration of the spherical reflecting surface is necessary to make room for the optical fibers and the structure that would support them. On the other hand, the decentration distance must not exceed the amount beyond which the coma that results from decentration would become unacceptably large. In the case of an effective aperture of f/3, the coma would be only slightly in excess of the spherical aberration if the decentration were limited to about f/6. This would be enough to accommodate the fibers and supporting structure.
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