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697 results about "Primary mirror" patented technology

A primary mirror (or primary) is the principal light-gathering surface (the objective) of a reflecting telescope.

Spectral imaging method and spectrum imaging instrument of snapshot-type high throughput

The invention relates to a spectral imaging method and a spectrum imaging instrument of a snapshot-type high throughput, which aim at realizing a picture-type photograph. The spectrum instrument comprises a linear gradient filter array and an optical-field imaging mechanism, and the optical-field imaging mechanism comprises a primary mirror, a micro lens array and a detector. The filter array is arranged on an aperture diaphragm between lenses of the primary mirror, the filter array consists of a plurality of filters which have identical width and are arranged at intervals, and the filter is a linear gradient filter band with continuous spectrum. The micro lens array is arranged on an imaging surface of a front-mounted optical imaging system, and the detector is arranged on a focus plane of the micro lens array. The spectrum imaging method is characterized in that light in different directions transmitted or reflected by a target is imaged on one micro lens after being modulated by the primary mirror and the filter array, the light is dispersed by the micro lens onto a picture element of the detector to form a subimage, and finally three-dimensional spectrum image data is obtained. The complete spectrum image information of the target can be obtained through the photograph in one step, and the spectral imaging method and the spectrum imaging instrument can be used for monitoring and tracking a rapid variable or movable target.
Owner:BEIHANG UNIV

Orthoptic synthetic aperture laser imaging radar

ActiveCN102435996AReduce the effects of phase interferenceBig optic toesElectromagnetic wave reradiationHigh resolution imagingRadar systems
The invention relates to an orthoptic synthetic aperture laser imaging radar. The orthoptic synthetic aperture laser imaging radar comprises a laser light source, a transmission polarization beam splitter, a horizontal polarization optical path beam deflector, a horizontal polarization optical path transform lens, a vertical polarization optical path beam deflector, a vertical polarization optical path transform lens, a transmission polarization beam combiner, a transmitter telescope ocular, a transmitter telescope primary lens, a receiver telescope, a receiving polarization beam splitter, a 2 * 490 DEG optical bridge, an inphase channel balanced detector, an inphase channel A / D (analogue / digital) converter, a 90 DEG of phase shift channel balanced detector, a 90 DEG of phase shift channel A / D (analogue / digital) converter, a pluralizing processor, a digital image processor and a control computer. The orthoptic synthetic aperture laser imaging radar automatically eliminates phase changes and interference of atmosphere, motion platforms, optical radar systems and speckles, has high resolution imaging in larger optical footprint and larger receiving aperture, does not need optical delay lines, does not need real-time beat frequency signal phase synchronization, does not have shadows during imaging, and can be used for various lasers with single-module and single-frequency properties.
Owner:SHANGHAI INST OF OPTICS & FINE MECHANICS CHINESE ACAD OF SCI

Low-cost refracting-reflecting athermalizing medium wave infrared lens

InactiveCN104035188AFew aspherical mirrorsEasy to detectMirrorsConvex sideLight beam
The invention provides a low-cost refracting-reflecting athermalizing medium wave infrared lens and aims at providing a low-cost refracting-reflecting optical lens which is small in aspherical mirror number, low in cost, made of a small amount of aspherical lenses and conventional silicon and germanium optical materials at a 3.7-4.8 [mu]m medium-wave infrared band and having the optical passive athermalizing performance. The technical scheme is that parallel light enters a main reflection spherical mirror (3) to form a converged light beam through a spherical cover (2) in an incidence mode, a convergence angle is decreased through a Mangin refracting-reflecting mirror (4), a primary mirror face (5) is formed by decreasing a part of aberration and increasing a part of balanced aberration and negative thermal difference of a lens to be arranged behind, the light beam is changed into divergent light, the divergent light enters a negative lens (6) made of an aspherical germanium material and a positive meniscus lens (7) made of a silicon material so as to reduce chromatic aberration and aberration, then converges through a positive convex lens (8) made of the silicon material, enters a detector window (9) and finally forms an image on a detector focal plane (11) through a cold light diaphragm (10), and the whole imaging process is finished.
Owner:SOUTH WEST INST OF TECHN PHYSICS

High dynamic imaging module based on DMD dynamic beam splitting

ActiveCN107343130AAchieve clear imagingGuaranteed full coverage of linear response dynamic rangeTelevision system detailsColor television detailsHigh-dynamic-range imagingMulti camera
The invention relates to a high dynamic imaging module based on DMD dynamic beam splitting. The module includes DMD-based high dynamic imaging module hardware, optical path control software, and image fusion software. A target light enters a main mirror, is reflected by a dynamic beam splitting device, and then passes through an adapter, a light intensity dynamic adjustable mechanism, and a position sensor, images are acquired by cameras, and then the light passes through a DMD spatial light modulator and is transmitted to a computer for parameter calculation compensation, and the high dynamic range images can be obtained; the adapter can realize the dynamic adjustment of the splitting ratio area to the camera target surfaces according to different imaging tasks; a main lens+adapter+multi-camera optical path structure is formed through the combination with an image fusion and enhancement processing algorithm, the dynamic range provided by the optical path structure can reach 136dB, the whole dynamic range of the system is greater than 150dB, so that the high dynamic range imaging of the target can be realized. the compact and small beam splitting structure can be realized by a DMD device, so that the whole and sub-area dynamic beam splitting can be realized. The technical problem of simultaneous high-quality imaging of the rocket and flame of a target range can be solved.
Owner:NAT UNIV OF DEFENSE TECH

System and method for effecting high-power beam control with outgoing wavefront correction utilizing holographic sampling at primary mirror, phase conjugation, and adaptive optics in low power beam path

A beam control system and method. In an illustrative embodiment, the inventive system (500) provides a first beam of electromagnetic energy (503); samples the first beam (503) and provides a second beam (505) in response thereto; detects aberrations in the second beam (505); and corrects aberrations in the first beam (503) in response to the detected aberrations. In a specific implementation, the invention (500) includes a beam director telescope (510) having a primary mirror (516) on which a holographic optical element (518) is disposed. The holographic optical element (518) samples the output high-power beam and provides a sampled beam to a wavefront sensor (520). The wavefront sensor (520) provides signals to an adaptive optics processor (580). The adaptive optics processor (580) analyzes the sampled wavefront, detects aberrations therein and provides a correction signal to an optical phased array (550). A master oscillator (552) provides a reference beam, which reads the optical phased array (550) and is back reflected off a front surface of an aperture sharing element (540). The resulting beamfront is conjugated by a first phase conjugate mirror (546) and then again by a second phase conjugate mirror (556). The output of the second phase conjugate mirror (556) is amplified and reflected off the front surface of the aperture sharing element (540). The aperture sharing element (540) outputs the high power beam via the telescope (510) which is corrected for the optical distortions in the telescope and beam path.
Owner:RAYTHEON CO

Novel high resolution large visual field optical imaging system

ActiveCN103064171AAchieve super large field of viewHigh-resolutionOptical elementsAir monitoringImaging quality
A novel high resolution large visual field optical imaging system is composed of a share primary mirror, a microlens array and a detector array. The share primary mirror is in a holocentric spherical mirror structure, and the center of the share primary mirror is a spherical mirror. Two meniscus lenses are wrapped on two sides of the share primary mirror, and incident rays respectively pass through the share primary mirror and the microlens array, and finally reach the detector array for imaging. Through the computed imaging technology, image restoration is carried out on every sub-image (eliminating impact of spherical difference on image quality), and all sub-images are subjected to registration recombination to obtain a complete clear image. The novel high resolution large visual field optical imaging system is simple in structural type, and the visual field can reach 180 degrees in theory. The full visual field has a uniform resolution ratio, and combines with the computed image post processing technology, the systematic resolution ratio can be close to a diffraction limit in theory. The novel high resolution large visual field optical imaging system has the advantages of having an extra large visual field, a high resolution ratio, and the like, and particularly suitable for researching and finding of space targets in a wide range, air monitoring for a stratosphere, and the like.
Owner:BEIJING RES INST OF SPATIAL MECHANICAL & ELECTRICAL TECH

Foldable spectacle frame with engaging means for maintaining the spectacle frame in unfolded state while wearing

A foldable spectacle frame having two lens frames forming a plane, two temples which are foldable to a thin form in substantially the same plane as the lens frames without lapping over the lens frames. Each of the temples comprises an auxiliary temple member supported by a pivot provided at an outer portion of the lens frames and being movable about the pivot in an auxiliary plane of pivotal movement substantially orthogonal to the plane of the lens frames, and a main temple member pivoted to the auxiliary temple rotatably in a main plane of pivotal movement orthogonal to the auxiliary plane of pivotal movement of the auxiliary temple member. The spectacle frame further comprises a slide member slidably provided within the auxiliary temple and having a length permitting a base end thereof to project from the auxiliary temple member, and biasing means for biasing the slide member away from the pivot when folding the spectacle frame. The pivot includes engaging means for engaging the slide member with the pivot of the lens frames by cooperation of the slide member, the pivot, and the main temple member. The slide member will engage with the pivot when the main temple member is brought into an unfolded state, and will disengage from the pivot when the main temple member or the auxiliary temple member is folded.
Owner:HUANG DAVID

Direct wave face conversion scanner for direct sight synthetic aperture laser imaging radar emitting light beam

The principle of a direct wave face conversion scanner for a direct sight synthetic aperture laser imaging radar emitting light beam is that a Mach-Zehnder polarized interferometer is adopted to divide an incident light beam into two cross-polarization separated space channels, each of the channel is internally provided with a track-along cylindrical mirror needed by phase quadratic term traversing and a track-crossing cylindrical mirror needed by phase line modulating, the track-crossing cylindrical mirror is provided with a scanning driver, and wave face conversion is performed on the light beam by combining the cylindrical mirrors of the two channels to generate two coaxial cross-polarization scanning emitting wave faces which are imaged to a target face by an emitting optical main mirror. The direct wave face conversion scanner for the direct sight synthetic aperture laser imaging radar emitting light beam has the advantages of simple and reliable structure, small size, small transmission loss, vibration resistance, realizing precise phase quadratic term by adopting a high-precision non-spherical optical element, and capability of changing the work mode and the running performance parameters of a radar by adopting the cylindrical mirrors with different focal lengths and different scanning directions without changing the whole structure.
Owner:SHANGHAI INST OF OPTICS & FINE MECHANICS CHINESE ACAD OF SCI

Telescopic truss type binary optical space camera and on-orbit work method thereof

The invention provides a telescopic truss type binary optical space camera and an on-orbit work method thereof and belongs to the field of spaceflight space repeatable unfolding. The telescopic truss type binary optical space camera aims to solve the problems that an existing space foldable and spreadable framework type supporting arm is complicated in structure, heavy and difficult to repeatedly fold and unfold. A partitioned type spreadable optical main lens of the telescopic truss type binary optical space camera is installed on a supporting arm through three ball hinges. The supporting arm comprises multiple framework type foldable units. The on-orbit work method comprises the steps that during launching, the supporting arm and the partitioned type spreadable optical main lens are in a folded mode, and the optical camera is in a launch closed mode; after injection, the supporting arm is switched to a unfolding mode and is unfolded; after the supporting arm is unfolded appropriately, the space camera is switched to an on-orbit operation mode, and the partitioned type spreadable optical main lens is unfolded; when the space camera is switched to an on-orbit closed mode, the supporting arm is folded, and the partitioned type spreadable optical main lens is unfolded. The telescopic truss type binary optical space camera is a large-caliber space camera.
Owner:HARBIN INST OF TECH

Large-caliber aspheric surface primary mirror detection device and method

The invention relates to a large-caliber aspheric surface primary mirror detection device and method. The device includes a point light source, a baffle, a measuring scale, a CCD (charge coupled detector) and a thin wire. According to the method, a spherical wave emitted by the point light source passes through an annular seam in the baffle and irradiates the mirror surface of a to-be-detected aspheric surface primary mirror; then the spherical wave is reflected by the mirror surface; the position of the baffle is adjusted, so that the light reflected by the mirror surface of the to-be-detected aspheric surface primary mirror can pass through the annular seam in the baffle; a circle of bright ray is formed at the point light source; the thin wire is used for cutting at the point light source; observing from the back of the thin wire, a user can see that the bright ray disappears; the CCD positioned behind the point light source is used for shooting and recording images of the bright ray; the radius of the annulus of the bright ray and the distance from the light point source to the to-be-detected aspheric surface primary mirror are measured. The position of the point light source or the baffle is adjusted, and the radius of the annulus of the bright ray and the distance from the light point source to the to-be-detected aspheric surface primary mirror are measured, so that the radius of curvature of a vertex of the to-be-detected aspheric surface primary mirror, a secondary constant and a surface shape are figured out according to the aspheric surface primary mirror surface shape formula.
Owner:INST OF OPTICS & ELECTRONICS - CHINESE ACAD OF SCI

Method for assembling convex grating imaging spectrometer

InactiveCN102141439ATroubleshoot assembly methodsHigh implementabilitySpectrum investigationTelephoto lensGrating
The invention discloses a method for assembling a convex grating imaging spectrometer, and the method provided by the invention belongs to the field of optical instruments, and is used for solving the problems that the existing convex grating concentric beam-splitting system is difficult to install and adjust, so that the concentric accuracy of the system is low and the practical applicability of the system is poor. The method disclosed by the invention comprises the following steps: configuring an interferometer and a standard compensating mirror; arranging a primary mirror and a triangular mirror of a convex grating beam splitting system in front of the interferometer, adjusting the positions of the primary mirror and the triangular mirror, so that an interference fringe occurs to the interferometer; arranging a mercury lamp in front of a slit, arranging a grating between the primary mirror and the triangular mirror, arranging a reading microscope at the image surface of the convex grating beam splitting system, and then adjusting the grating, so that the reading microscope can read out the zero-level and minus-one-level spectrums of the mercury lamp; and arranging a detector and a telephoto lens, and then adjusting the detector and the telephoto lens, so that the detector can accept an ideal spectral image of a detected target. In the method disclosed by the invention, because the assembling of the grating and the detector are realized by using a spectrogram direct-reading method, the method is strong in practicability and high in accuracy.
Owner:CHANGCHUN INST OF OPTICS FINE MECHANICS & PHYSICS CHINESE ACAD OF SCI
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