Optical sheet module and backlight unit having same
US-2020041715-A1 · Feb 6, 2020 · US
US11280615B2 · US · B2
| Field | Value |
|---|---|
| Publication number | US-11280615-B2 |
| Application number | US-201816018846-A |
| Country | US |
| Kind code | B2 |
| Filing date | Jun 26, 2018 |
| Priority date | Jun 26, 2017 |
| Publication date | Mar 22, 2022 |
| Grant date | Mar 22, 2022 |
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A wide field-of-view celestial sighting system and method are provided. The method includes orienting an imaging optic to collect light from at least one light source, such as at least one celestial body, the imaging optic being secured to a platform. The method further includes selectively collecting light from the at least one celestial body through a selective light collector secured to the platform and positioned in an imaging surface, such as an imaging plane, of the imaging optic. The method further includes combining forward scattered light from the at least one celestial body to provide a combined forward scattered light, and detecting a light intensity of the combined forward scattered light. Systems for performing the method are provided.
Opening claim text (preview).
What is claimed is: 1. A method for determining a position of a star tracker sensing light from a plurality of celestial bodies, wherein the light passes through, and is scattered by, atmospheric clouds between the celestial bodies and the star tracker, the method comprising: disposing a light sensor in the star tracker; disposing a lens, in the star tracker, between the celestial bodies and the light sensor; disposing a mask between the lens and the light sensor, wherein the mask is configured to define a pattern of light-passing apertures there through, the pattern matching positions of the celestial bodies; admitting light through the lens from a cloudy sky having a plurality of celestial bodies whose light passes through, and is scattered by, atmospheric clouds between the celestial bodies and the lens; orienting the mask so as to maximize intensity of the light from the celestial bodies passing through the apertures and impinging on the light sensor; and automatically calculating a navigational parameter, based on orientation of the mask. 2. The method according to claim 1 , further comprising oscillating the mask. 3. The method according to claim 1 , further comprising: disposing a plurality of optical fibers between the mask and the light sensor; and conducting the light, via the plurality of optical fibers, to the light sensor. 4. The method according to claim 1 , wherein disposing the mask comprises disposing a mask comprising a plurality of holes defining the light-passing apertures. 5. The method according to claim 1 , wherein disposing the mask comprises disposing a liquid crystal display (LCD). 6. A star tracker for determining a navigational parameter by sensing light from a plurality of celestial light sources in the sky, the star tracker comprising: a lens configured to focus, onto an imaging surface, light emitted by a plurality of celestial light sources in the sky and subsequently forward scattered by atmospheric clouds disposed between the plurality of celestial light sources and the lens, the lens being configured to form an image of the plurality of celestial light sources on the imaging surface; a selective light collector disposed in the imaging surface and configured to define a pattern of apertures, wherein the pattern matches positions of a selected set of the celestial light sources in the sky, each aperture being configured to: allow forward-scattered light from a respective one of the selected set of celestial light sources to pass through the selective light collector; and at least partially block other scattered light; a detector comprising a plurality of photo-sensitive pixels arranged in an array, each pixel being configured to receive, from the selective light collector, forward-scattered light from a respective different portion of the sky of a plurality of portions of the sky; and a processor coupled to the detector and configured to: receive a light intensity signal from the detector; monitor the plurality of portions of the sky to thereby track a plurality of celestial bodies; orient the selective light collector in response to intensity of light sensed by the detector; and determine a navigational parameter based at least in part on orientation of the selective light collector. 7. The star tracker according to claim 6 , wherein the selective light collector comprises a mask. 8. The star tracker according to claim 6 , wherein the selective light collector comprises a liquid crystal display (LCD). 9. The star tracker according to claim 6 , wherein the selective light collector comprises a plurality of optical fibers.
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