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  • 1
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    In:  CASI
    Publication Date: 2019-07-12
    Description: A technique for measuring optical beam shear is based on collecting light from the four quadrants of the beam and comparing the optical power collected from each quadrant with that from the other three quadrants. As used here, "shear" signifies lateral displacement of a beam of light from a nominal optical axis. A sensor for implementing this technique consists of a modified focusing lens and a quad-cell photodetector, both centered on the nominal optical axis. The modification of the lens consists in cutting the lens into four sectors (corresponding to the four quadrants) by sawing along two orthogonal diameters, then reassembling the lens following either of two approaches described next. In one approach, the lens is reassembled by gluing the sectors back together. In the simplest variant of this approach, the kerf of the saw matches the spacing of the photodetector cells, so that the focus of each sector crosses the axis of symmetry to fall on the opposite photodetector cell (see figure). In another variant of this approach, the lens sectors are spaced apart to make their individual foci to fall on separate photodetector cells, without crossing the optical axis. In the case of a sufficiently wide beam, the modified lens could be replaced with four independent lenses placed in a square array, each focusing onto an independent photodetector
    Keywords: Technology Utilization and Surface Transportation
    Type: NPO-41746 , NASA Tech Briefs, January 2007; 8-9
    Format: application/pdf
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  • 2
    Publication Date: 2019-07-13
    Description: The TPF Interferometer (TPF-I) concept is being studied at the Jet Propulsion Laboratory and the TPF-I Planet Detection Testbed has been developed to simulate the detection process for an earthlike planet orbiting a star within about 15 pc. The testbed combines four beams of infrared light simulating the operation of a dual chopped Bracewell interferometer observing a star and a faint planet. This paper describes the results obtained this year including nulling of the starlight on four input beams at contrast ratios up to 250,000 to 1, and detection of faint planet signals at contrast ratios with the star of 2 million to 1.
    Keywords: Astronomy
    Type: SPIE Astronomical Telescopes and Instrumentation; May 24, 2006 - May 30, 2006; Orlando, FL; United States
    Format: text
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  • 3
    Publication Date: 2019-07-13
    Description: While the overall architecture of an Entry Descent and Landing (EDL) system may vary depending on specific mission requirementsw, measurements of the rate vector with respect to the surface is a primary requirement for the Terminal Descent Control (TDC) phase of any controlled lander.
    Keywords: Lunar and Planetary Science and Exploration
    Type: Coherent Laser Radar Conference; Oct 16, 2005 - Oct 21, 2005; Kamakura; Japan
    Format: text
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