Integrated on-chip wireless optical communication terminal
US-2023085936-A1 · Mar 23, 2023 · US
US12526046B2 · US · B2
| Field | Value |
|---|---|
| Publication number | US-12526046-B2 |
| Application number | US-202318191244-A |
| Country | US |
| Kind code | B2 |
| Filing date | Mar 28, 2023 |
| Priority date | Mar 28, 2023 |
| Publication date | Jan 13, 2026 |
| Grant date | Jan 13, 2026 |
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Embodiments of the present invention include free-space optical communication systems and methods employing homodyne encoding on the receiver sides of the terminals that are configured to mitigate optical degradation due to atmospheric turbulence.
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What is claimed is: 1 . A method for homodyne aperture reconstruction of a spatially encoded optical source light signal corrupted by atmospheric turbulence sent from a remote optical source, the method comprising: providing a system for the homodyne aperture reconstruction of the source light signal; physically separating the source light signal to generate laterally separated light in a non-redundant array; collimating the laterally separated light to obtain laterally separated collimated light; focusing the laterally separated collimated light; capturing a time sample of the laterally separated collimated light; extracting spatially separated beat terms from the time sample; determining phase errors in the time sample of the spatially separated beat terms to obtain phase corrected optical data; determining jitter correction in the phase corrected optical data to obtain jitter corrected optical data; deconvolving the jitter corrected data using estimated power and noise spectra to obtain deconvolved optical data; and recombining the deconvolved optical data to obtain a corrected light signal. 2 . The method according to claim 1 , wherein the system comprises: a multi-aperture primary beam separating interferometer; a multi-aperture secondary beam collimating interferometer spaced apart from the primary beam separating interferometer; and a sensor for capturing optical image data time samples. 3 . The method according to claim 2 , wherein the physically separating the source light signal further comprises passing the source light signal through the multi-aperture primary beam separating interferometer to generate the laterally separated light. 4 . The method according to claim 2 , wherein the collimating the laterally separated light further comprises passing the laterally separated light through the secondary multi-aperture beam collimating interferometer to obtain the laterally separated collimated light. 5 . The method according to claim 2 , wherein the focusing the laterally separated collimated light further comprises focusing the laterally separated collimated light onto the sensor. 6 . The method according to claim 2 , wherein the capturing the time sample further comprises capturing the time sample with the sensor. 7 . The method according to claim 2 , further comprising calibrating the system for homodyne aperture reconstruction. 8 . The method according to claim 7 , wherein the calibrating further comprises: creating an initial calibration dataset; and computing initial offset shifts to obtain baseline spatial shifts. 9 . The method according to claim 2 , wherein the multi-aperture primary beam separating interferometer and the multi-aperture secondary beam collimating interferometer comprise a matched pair of three-aperture interferometer assemblies. 10 . The method according to claim 1 , wherein the determining phase errors, further comprises: solving for any phase errors in the time sample of the spatially separated beat terms by forcing computed overlapped regions to be in phase; and spatially placing frequency information back into correct locations as defined prior to separation. 11 . A non-transitory computer readable media storing computer readable software instructions that when executed by a processor causes the processor implementing the method for homodyne aperture reconstruction of a spatially encoded optical source light signal corrupted by atmospheric turbulence sent from a remote optical source recited in claim 1 . 12 . The method according to claim 1 , wherein the spatially encoded optical source light signal comprises multiple spatially encoded optical source light signals within a viewing field. 13 . The system according to claim 12 , wherein the data acquisition module further comprises a sensor array. 14 . A system for homodyne aperture reconstruction of a spatially encoded optical source light signal corrupted by atmospheric turbulence sent from a remote optical source comprising: an input optical setup module configured to receive the corrupted light signal and present a focused, laterally separated, corrupted light signal; a data acquisition module configured to capture at least one time sample of the focused, laterally separated, corrupted light signal; and an image processing module configured to correct phase errors and jitter in the at least one time sample and generate corrected image data, the image processing module further comprising: a spatially separated beat terms extractor; a phase error corrector; a jitter corrector; a deconvolver; and a recombiner. 15 . The system according to claim 14 , wherein the spatially encoded optical source light signal comprises multiple spatially encoded optical source light signals within a viewing field. 16 . The system according to claim 14 , wherein the input optical setup further comprises: a primary aperture interferometer, the primary aperture interferometer configured to receive the corrupted light signal and laterally separate the corrupted light signal; a secondary aperture interferometer including three secondary apertures in communication with the primary aperture interferometer and configured to collimate the laterally separated, corrupted light signal; and focusing optics in communication with the secondary aperture interferometer and configured to focus the collimated laterally separated, corrupted light signal. 17 . The system according to claim 16 , wherein the primary aperture interferometer further includes three primary apertures, wherein each of the three primary apertures further comprise: a diameter, d 1 , of about 12.7 mm; and center-to-center spacing, s 1 , of about 13.7 mm, relative to one another. 18 . The system according to claim 17 , wherein the secondary aperture interferometer includes three secondary apertures, wherein each of the three secondary apertures further comprise: a diameter, d 2 , of about 25.4 mm; and center-to-center spacing, s 2 , of about 44.0 mm, relative to one another. 19 . The system according to claim 18 , wherein the primary apertures and the secondary apertures are matched and separated by a distance, s 3 , of about 50 mm. 20 . The system according to claim 18 , wherein the primary apertures and the secondary apertures each further comprise: a blazed diffraction grating with 300 lines per mm; a blaze angle of about 11.25°; a diffraction efficiency of about 60%; a center wavelength of about 670 nm; and a blaze arrow direction toward beamline's center. 21 . The data acquisition module, according to claim 14 , wherein the data acquisition module comprises a visible-band camera. 22 . An optical communications system including a plurality of optical transceivers in communication with each other, each transceiver comprising: a transmitter; and a system for homodyne aperture reconstruction, the system further comprising: a receiver adapted for receiving a spatially encoded optical source light signal corrupted by atmospheric turbulence; a processor in communication with the receiver; and a memory in communication with the processor configured to store a computer program adapted for implementing a method for homodyne aperture reconstruction of a spatially encoded optical source light signal corrupted by atmospheric turbulence sent from a remote optical source; and wherein the method further comprises: providing a system for the homodyne aperture
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