266 results about "Secondary mirror" patented technology

The invention relates to the technical field of intelligent precision calibration of optical instruments, in particular to a primary and secondary mirror calibration method based on a neural network algorithm, which comprises the following steps: step 1, synchronously acquiring multi-physics field coupling data of primary and secondary mirrors; step 2, constructing a dual-mode neural network model, wherein the dual-mode neural network model comprises a first model and a second model; 3, kinematics feasibility verification and dynamic optimization are carried out on the initial prediction value, specifically, a Lie group space parameterization method is adopted to avoid a rotation freedom degree singular point, and a platform reachable working space is adjusted through Jacobian matrix verification; and 4, driving a secondary mirror adjustment platform based on the optimized adjustment parameters, and triggering online incremental learning of the neural network model according to the actual wavefront residual error. Through innovative application of the neural network algorithm, multiple technical problems of a traditional optical system calibration method in an extreme environment and a high-frequency dynamic condition are solved, and the calibration precision, the real-time performance and the efficiency are improved through self-learning and self-adaptive capabilities.

The invention discloses a primary and secondary mirror combined detection system and method for a beam shrinking system, and belongs to the technical field of optical detection.The method comprises the steps that a first micro-spherical mirror and a second micro-spherical mirror are arranged, reflection light spots are captured through an interferometer, the position offset is calculated, and a first control instruction for adjusting the pose of a secondary mirror is generated; a dual-band light source is integrated in a detection light path, wavefront data and alignment monitoring data are collected, and temperature drift is corrected to obtain effective combined wavefront; an error separation model is constructed based on the primary mirror compensator parameter and the Zernike aberration coefficient, and a primary mirror surface shape error component and a secondary mirror offset error component are decoupled and separated by using a preset aberration coupling coefficient; feeding the error component back to a polishing process and a displacement table for closed-loop iterative correction until the RMS value and the PV value of the effective combined wavefront meet a preset imaging quality index; through precise positioning, error correction and decoupling separation, the precision and efficiency of primary and secondary mirror combination detection are improved, and targeted correction is realized.

The invention relates to a three-waveband off-axis reflective optical system with view field switching and focusing functions. Belongs to the photoelectric technical field. Multi-band common-caliber imaging is realized by adopting an off-axis two-reflection-path form, imaging information can be continuously obtained day and night all day, laser emitting and receiving capabilities are considered, and the device has functions of positioning aiming, laser guiding and the like. Large and small field-of-view switching imaging is realized through switching-in and switching-out of the secondary mirror, and the system has the capability of carrying out rapid search in a large field-of-view range and carrying out accurate identification and tracking in a small field-of-view range; the auto-collimation focusing of the optical system is realized by switching the position of the focusing mirror and arranging the focusing system, the system is ensured to be clear in imaging under the use conditions of different atmospheric pressures, temperature changes and photographing distances, and the system is suitable for accurate aiming and detection of a target under various complex and severe working conditions. The total reflection optical system is free of chromatic aberration, free of blocking, compact in structure and high in system integration degree, and the requirement for functional diversification of a photoelectric system is met.

The invention relates to a common-aperture double-linear-array surveying and mapping camera optical system based on secondary mirror multiplexing, and belongs to the technical field of space remote sensing measurement. The optical system comprises two double-line-scan digital cameras which share the same aperture diaphragm and the same main reflector. According to the optical system, an integrated structure that the double-line-scan digital camera shares the primary mirror and a structure that the secondary mirror and the fourth mirror are coplanar and most of effective areas are overlapped are adopted at the same time, the double-line-scan digital camera is subjected to integrated structure design, the measurement precision regulation and control difficulty is reduced, and the surveying and mapping precision is improved; and a free-form surface is also introduced to realize coplanarity of the secondary mirror and the fourth mirror, so that two reflection areas of the coplanar reflector are overlapped, and the volume and the mass of the coplanar reflector are reduced. On the basis that three reflectors of the optical system are reduced, the focal plane is placed between the main reflector and the third reflector, light is overlapped on the premise that the image quality is not reduced, the size of the optical system is compressed, the space utilization rate of the system is improved, and the emission cost is reduced.

The invention discloses a non-diffraction laser communication terminal based on Bessel beams. The terminal comprises a beacon transmitting module, an optical antenna module, a beacon receiving module, a signal transmitting module, a signal receiving module and a light splitting module. The beacon transmitting module and the signal transmitting module respectively convert the Gaussian beam into a Bessel beam through an axicon, and the Bessel beam is output through a collimating lens; a primary mirror and a secondary mirror of the optical antenna module are mounted in an off-axis manner, so that light beams are shrunk and expanded; the light splitting module completes light path switching and light splitting through a fast reflecting mirror, a 1 / 4 wave plate, a dichroscope and a polarizing beam splitter; the beacon receiving module obtains beacon light position information through a CMOS detector, and the signal receiving module receives signal light through an APD detector. The non-diffraction characteristic of the Bessel beam is utilized, and the off-axis optical antenna and the polarization beam splitting design are combined, so that high-precision and low-loss laser communication is realized.

The present invention relates to a lidar system including: laser transmitter and receiver systems, the laser transmitter system including: a wavelength-tunable seed laser which emits pulses at selected wavelength points, and switches between wavelengths within a switching time of <200 ns; a fiber amplifier which amplifies the laser pulses up to 200 kW to a transmitter grating; and a transmitter telescope including primary and secondary mirrors. The laser beam is directed from the transmitter grating to the secondary then primary mirrors, and the first transmitter grating is imaged on the primary mirror to minimize laser beam wander thereon. The transmitter grating diffracts and steers the laser beam by wavelength to a surface, to an arbitrary subset of <2000 resolvable footprints along a cross-track direction at a beam pointing angle switching time of <200 ns, such that footprints illuminated by the laser beam on the surface are imaged in 3D.

The invention relates to a coaxial four-mirror optical system, which comprises a primary mirror, a secondary mirror, a third mirror, a fourth mirror and an annular diaphragm, all the mirrors and the annular diaphragm are coaxially arranged, both the secondary mirror and the third mirror are provided with light through holes, light is reflected by the primary mirror and then is reflected by the secondary mirror, the third mirror and the fourth mirror in sequence, and the light is reflected by the annular diaphragm. And finally converging and imaging. In the design, through application of the annular diaphragm, edge aberration is reduced, and stray light suppression capability is remarkably enhanced at the same time. The coaxial four-mirror optical system has the advantages of being compact in structure, high in imaging quality, wide in applicability and the like, and is suitable for being applied to multiple fields of aerospace, biomedicine, industrial detection and the like.

The invention discloses an infrared four-waveband composite annular aperture folded imaging optical system, belongs to the technical field of optical catadioptric optical paths, and aims to solve the problem that 1550nm / 1064nm dual-laser and medium-wave / long-wave infrared four-waveband composite detection is difficult to realize at the same time in the conventional annular aperture imaging technology. The system comprises a primary mirror, a secondary mirror, a 1064nm laser spot correction mirror, a 1550nm laser spot correction mirror, a 1064nm laser spectroscope, a 1550nm laser spectroscope, a broadband infrared detector, a 1550nm laser detector and a 1064nm laser detector. And high-performance common-aperture composite detection of 1064nm / 1550nm dual laser and medium-wave / long-wave infrared four wavebands is realized through a multi-stage light splitting mechanism. The limitation that a traditional annular aperture system is single in wave band is broken through, and the all-weather sensing and target recognition capability of the system in a complex environment is remarkably improved.

The invention relates to a packaging structure of a micro display chip and a display device, and the packaging structure comprises a substrate, the surface of which comprises a display area and a non-display area; the electrode pads are located in the non-display area; and a plurality of through hole plugs located in the substrate, wherein one end of each through hole plug is electrically connected with the electrode pad. In AR near-to-eye display application, the light absorption structure can effectively absorb stray light returned from components such as an optical waveguide and the like, secondary specular reflection of the metal electrode pad on the non-display area is avoided, ghosting is prevented from being formed, and the imaging contrast ratio and the picture purity are remarkably improved. The light absorption structure is integrated in the packaging structure, and a stray light feedback path is cut off through a physical means on the premise that normal light emitting of a display area and electrical connection of an electrode pad are not affected, so that the optical performance of the micro-projection ray machine is improved, the final display effect is guaranteed, and the display effect is improved. Therefore, the technical problem of image quality degradation caused by high reflectivity of the non-display area is effectively solved.

A design method of an off-axis three-mirror free-form surface imaging system comprises the following steps: according to design values of performance parameters and structure parameters of an optical system, establishing an optical system initial structure consisting of a primary reflector, a secondary reflector and a third reflector as an initial state of iterative calculation of the optical system initial structure; the radiuses, the eccentricity and the inclination of the primary mirror, the secondary mirror and the third mirror are updated in sequence; the initial structure of the optical system meeting the threshold requirement is obtained by judging the evaluation function value MF of the initial structure of the optical system; and by taking the minimum wavefront difference of the optical system as an optimization target, optimizing the obtained initial structure of the optical system by using a damping least square method, and outputting a design result of the optimized optical system. According to the method, the process of repeated iteration adjustment according to the actual engineering space requirement in the conventional design method can be reduced, and the free-form surface off-axis three-mirror optical system meeting the actual engineering space requirement can be conveniently obtained.

To provide a compact, high-performance catadioptric optical system. [Solution] The optical system comprises, in order of light passage from the object side, a primary mirror section consisting of an aspherical concave mirror with its concave surface facing the object side, a secondary mirror section arranged on the object side of the primary mirror section and consisting of an aspherical convex mirror with its convex surface facing the image side, and a refractive system arranged on the image side of the secondary mirror section, the refractive system comprising a front group with positive refractive power and a rear group with negative refractive power separated by a maximum air gap, the refractive system comprising at least five lenses, where PG is the Petzval sum of the refractive system obtained by normalizing the focal length of each surface by the focal length of the entire system, and PM is the Petzval sum of the reflective system obtained by normalizing the focal length of each surface by the focal length of the entire system, 0.6<|PG / PM|<1.2…(1) If the refractive power of the refractive system is φG and the refractive power of the entire system is φ0, then 0.05<|φG / φ0|<1.5…(2) 7 <PM<20…(3) It is characterized by satisfying the conditions (1), (2), and (3).

The invention relates to the field of electronic detectors, and discloses a reflective ultrafast scintillation vacuum ultraviolet light imaging detection system and a method thereof.The reflective ultrafast scintillation vacuum ultraviolet light imaging detection system comprises a light path system, a detection and recording component and a structure supporting component, and the light path system is in reflective light path configuration and comprises a primary mirror, a secondary mirror, a correction lens, an integrated filter and a vacuum ultraviolet scintillator; and the vacuum ultraviolet scintillator is made of a PEA2PbBr4 crystal or a BA2PbBr4 crystal. According to the invention, by constructing reflective optical path configuration, the capability of the device in vacuum ultraviolet (VUV) scintillation imaging is successfully shown. The invention not only provides a new solution for reducing the influence of the self-absorption effect in the perovskite scintillator, but also establishes a bridge between the perovskite scintillator and the perovskite scintillator actually applied to ultrafast VUV detection, and opens up a new way for the application of the perovskite material in the field of VUV imaging.

The application provides a dual-wavelength coaxial aiming system capable of automatic collimation, which is used for attitude adjustment and target positioning aiming of a picosecond terminal optical path cone target of inertial confinement fusion (ICF). The system comprises automatic collimation optical paths and aiming optical paths of different working wavelengths; the automatic collimation optical paths comprise a light source, a light splitting prism, a secondary mirror, a reflecting mirror and a CCD detector; the aiming optical paths are composed of a primary mirror, a secondary mirror, a lens group, a light splitting prism and a CCD detector group, and each optical element is coaxial; the system multiplexes the secondary mirror, and realizes automatic collimation and positioning aiming through different wavelength transmission and reflection respectively; the system adopts combination of flint and crown glasses to correct chromatic aberration of different wavelengths; the image planes of the dual-wavelength optical paths are located at the same position; and the system adopts a coaxial two-mirror structure, and is compact in structure and small in size.

The invention provides a hyperspectral imaging system. The hyperspectral imaging system comprises a telescope group, a collimator objective, a prism, a volume holographic diffraction grating, an imaging objective and an imaging sensor which are arranged in sequence, the telescope group is composed of a primary reflector, a secondary reflector, a third reflector, a plane reflector and an entrance slit; the primary reflector, the secondary reflector and the third reflector form an off-axis three-reflector structure; the plane reflector is used for folding a light path; the collimating objective lens, the prism, the volume holographic diffraction grating, the imaging objective lens and the imaging sensor form an imaging spectrometer, and an entrance slit is used as object space input; the formed off-axis three-mirror and folded light path and an imaging spectrometer are in coaxial butt joint by taking an entrance slit as a node, and are used for joint correction and splicing to form a hyperspectral imaging system. According to the optical path architecture, optimal matching of the unobstructed total reflection front end and the transmission type rear end is realized, and the detection sensitivity of crop weak spectrum signals is greatly improved while a better modulation transfer function of a full view field is ensured.

The invention relates to the technical field of reflective optics, in particular to an off-axis three-mirror optical system with double folding mirrors, which comprises a primary mirror adopting a concave reflecting mirror and a secondary mirror adopting a convex reflecting mirror, an intermediate image is formed on an output light path of the secondary mirror, and a first folding mirror is arranged at the position of the intermediate image; the first folding mirror folds the light beam from one side of the incident light beam of the primary mirror to the other side, so that the third mirror receives the light beam; the third mirror of the concave reflecting mirror is matched with the primary mirror and the secondary mirror to correct aberration, and a final imaging light beam is generated; a second folding mirror located on an output light path of the third mirror reflects the light beam again, so that the focal plane is close to and higher than the primary mirror; the focal plane is located in an envelope space of the primary mirror and the third mirror; the diaphragm is arranged in an off-axis mode, and the off-axis amount of the diaphragm is 0.3-0.6 times of the diameter of the aperture. According to the invention, the compactness of the off-axis three-mirror optical system is improved through double-folding front and back split arrangement; through focal plane position optimization, the optimized focal plane is higher than the primary mirror.

This invention provides an optical system and method for free-space quantum key distribution. The optical telescope employs a transmission-type telescope and a simplified rear optical path terminal, effectively avoiding secondary mirror obstruction and vignetting. The optical telescope system has a smaller axial dimension and is lighter than a Cassette-type reflecting telescope of the same aperture, making it more suitable for large-scale use in short-range free-space quantum communication. It can be carried and deployed by a single person and has all-day quantum key distribution capabilities. Furthermore, the transmitting and receiving telescopes are interchangeable, meaning the system can function as both a transmitter and a receiver, extending quantum communication coverage to areas inaccessible by fiber optics and satellites, and enabling rapid deployment in various emergency and unforeseen circumstances.

The invention discloses a high-precision control method for optical parameters of an off-axis spliced sub-lens of a primary lens of a large astronomical telescope, and belongs to the field of advanced optical manufacturing and detection. According to the method, precise adjustment of a detection light path is achieved through different diffraction function areas of computer generated holography (CGH), and high-precision control over the curvature radius and the off-axis amount of an off-axis sub-mirror is achieved by combining distance measurement of a laser tracker and angle measurement of a theodolite. The method specifically comprises three stages of inspection light path coarse adjustment, fine adjustment and light path parameter measurement and processing, optical element space attitude adjustment is guided through a diffraction reference point of the CGH, and finally off-axis sub-mirror surface shape and optical parameter information are obtained. According to the invention, the problem of installation and adjustment precision in the detection of the large off-axis aspheric reflector can be effectively solved, and reliable technical support is provided for the manufacturing of the primary mirror and the spliced secondary mirror of the astronomical telescope.

The invention relates to an ultra-large field-of-view dual-waveband aperture multiplexing type optical remote sensing camera, and belongs to the technical field of optical remote sensing. The optical remote sensing camera comprises a visible light optical system and an infrared optical system which share a primary mirror and a secondary mirror. The visible light optical system comprises a primary mirror, a secondary mirror, a visible light third mirror, a reflex mirror and a visible light focal plane in the light path direction; the infrared optical system comprises a primary mirror, a secondary mirror, an infrared third mirror and an infrared focal plane in the light path direction. According to the ultra-large field-of-view dual-waveband aperture multiplexing type optical remote sensing camera, all-weather ground investigation and surveying and mapping can be realized; primary mirrors and secondary mirrors of the visible light optical system and the infrared light optical system can be reused, the focal lengths of the two systems are different, the view fields of the visible light optical system and the infrared light optical system can be 20 degrees or above, and the ultrahigh energy utilization rate of the system is guaranteed through the total reflection mode. The camera is especially suitable for being used as a high-resolution camera of a wide-area detection, small-size and multi-spectrum integrated micro-nano satellite.

The utility model discloses a multi-terminal Newton reflection telescope system, which comprises a telescope body, an adjusting assembly and an optical assembly, an optical channel coaxial with the telescope body is arranged in the telescope body, and a plurality of mounting seats used for mounting photographic terminals are arranged on the circumferential side wall of the telescope body. The mounting base is provided with a connecting channel used for guiding light in the light channel to the photographing terminal, the adjusting assembly is arranged in the light channel and comprises a support, a base, a first adjusting mechanism and a second adjusting mechanism, the base is arranged on the support, the second adjusting mechanism is arranged on the base, and the support is connected with the lens body through the first adjusting mechanism; the first adjusting mechanism is used for adjusting the position of the support, the optical assembly comprises an auxiliary mirror, the auxiliary mirror is connected with a second adjusting mechanism, and the second adjusting mechanism is used for adjusting the position of the auxiliary mirror so that light reflected by the auxiliary mirror can be projected to the connecting channel of any mounting base. The system can be provided with a plurality of photographing terminals at the same time, the photographing requirement is met, and the application range of the Newton reflection telescope is widened.

The invention discloses a high-performance ultraviolet visible light hyperspectral imaging system and an adjustment method thereof, and belongs to the technical field of spectral imaging, in the system, a front mirror assembly comprises a front primary mirror assembly, a front secondary mirror assembly, a front three-mirror assembly and a folding-axis mirror assembly; light enters through the incidence assembly, is reflected by the primary mirror assembly, the front secondary mirror assembly, the front three-mirror assembly and the folding-axis mirror assembly in sequence, enters the optical slit, and then enters the grating through the optical filter, the prism, the first rear mirror, the second rear mirror and the third rear mirror in sequence. And after being dispersed and reflected by the grating, the light sequentially passes through the rear mirror 3, the rear mirror 2 and the rear mirror 1, enters the prism, and reaches an imaging image surface after being reflected by the prism. According to the invention, high-reflectivity detection of an ultraviolet band can be realized, high-resolution detection of an ultraviolet visible spectrum of 280-1000 nm can be realized, and the highest spectral resolution of 0.5 nm can be realized; the imaging quality is close to the diffraction limit, plug and play is achieved, and the light and small layout has engineering applicability.

An optical assembly includes a primary mirror, a secondary mirror, and an optical steering system configured to support and position the primary mirror and the secondary mirror. The optical steering system includes a base and a yoke rotatably coupled to the base. The yoke is configured to support the primary mirror to rotate the primary mirror about a first axis and to support a secondary mirror to rotate the secondary mirror about a second axis. The yoke further is configured to rotate the primary and secondary mirror about a third axis. The secondary mirror is configured to move from a stowed position in which the optical assembly is positioned to receive an image from a field of view to a deployed position in which the optical assembly is positioned to receive an image from a field of regard.

The invention discloses a compact, large-aperture and variable-focal-length collimator system, which comprises a Cassegrain reflector group, a correction lens group and a thermal compensation piece, the Cassegrain reflector group and the correction lens group are in optical conjugate design; the thermal compensation part is arranged in the Cassegrain reflector group so as to compensate the thermal expansion effect of the Cassegrain reflector group; the correction lens group is located on one side, close to the focal plane, of the Cassegrain reflector group, and the correction lens group is detachably connected with the Cassegrain reflector group; the Cassegrain reflector group comprises a primary mirror and a secondary mirror which are coaxially arranged; the correction lens group is used for collimating the short-focal-length parallel light beams output by the Cassegrain reflector group into long-focal-length parallel light beams; the correction lens group comprises one or more optical lenses, and the correction lens group is configured to be assembled with optical lenses with different focal powers and different numbers so as to realize focal length switching of the collimator system. Therefore, not only is the light beam collimation precision ensured, but also the collimator system is compact in structure and can quickly change the focal length.

This invention belongs to the field of target detection technology, and particularly relates to a miniaturized three-mode composite detection optical system. Target light rays are transmitted through a radome and then incident on a primary mirror. The primary mirror reflects the target light rays onto a secondary mirror. A dichroic film is coated on the surface of the secondary mirror closest to the primary mirror, separating the target light rays into laser and infrared rays. The laser light rays sequentially pass through the optical surface of the secondary mirror closest to the radome, a first lens, a second lens, and a filter to reach the photosensitive surface of a laser four-quadrant detector. The infrared light rays sequentially pass through a first infrared lens, a second infrared lens, and a third infrared lens to reach an infrared detector. Millimeter-wave signals emitted by a millimeter-wave waveguide slotted array radar are radiated to the target sequentially through the primary mirror and the radome. The echo signals reflected by the target are transmitted through the radome and the primary mirror sequentially before reaching the millimeter-wave waveguide slotted array radar. This invention can reduce the system length and volume, and expand the rotation angle of the servo frame within a limited space.

The invention discloses a primary and secondary mirror support machining device and a primary and secondary mirror support machining method, and the primary and secondary mirror support machining device comprises a bottom plate, a supporting cylinder, a plurality of arc-shaped fixing seats, a sensor mounting seat and a display device. On one hand, the outer side surface of the arc-shaped elastic sheet is fixedly connected with the metal induction block, and the metal induction block fills a pit formed by the outer side surface of the arc-shaped elastic sheet and the radial through hole, so that when the inner side surface of the arc-shaped elastic sheet is machined by a cutter, a second bolt on the sensor mounting seat can apply an abutting force to the metal induction block; the arc-shaped elastic piece can be prevented from being elastically bent and deformed in the radial direction under the acting force of a cutter, and therefore the inner side face of the arc-shaped elastic piece can be precisely subjected to finish machining. And on the other hand, in the finish machining process of the arc-shaped elastic piece, an operator can adjust machining parameters in real time according to the machining deformation amount of the arc-shaped elastic piece, and therefore the machining deformation of the arc-shaped elastic piece is within a proper range.

The invention discloses a remote high-depth-of-field LIBS self-focusing detection device for a lunar soil environment, and the device comprises a variable-curvature primary mirror which is provided with a central light through hole, and one side of the variable-curvature primary mirror is sequentially provided with a beam expanding assembly, a low-pass dichroscope, a focusing system, and a spectrometer; the multi-secondary-mirror zooming structure is arranged on the other side of the curvature-variable primary mirror; wherein the low-pass dichroscope corresponds to the transmitting end of the pulse laser; the variable-curvature primary mirror comprises a plurality of reflectors which are sequentially stacked from left to right, wherein the curvatures of the reflectors are sequentially increased. The multi-mirror zoom structure comprises a guide rail capable of rotating and axially moving; and the plurality of secondary mirrors with different curvature radiuses are sequentially arranged on the guide rail through the electronic clutch, and the secondary mirrors can diverge and reflect the light beams. According to the invention, the super-large depth of field with the axial depth of 1.5 cm is constructed by using the variable-curvature primary mirror, and the large-range coverage of the full life cycle area of the expanded plasma is realized.

The invention discloses a high-stability damping vibration attenuation secondary mirror three-period minimum curved surface dot matrix supporting structure which comprises a secondary mirror supporting frame, three-period minimum curved surface dot matrix supporting arms and a supporting seat. A microcrystal secondary mirror is arranged in the secondary mirror supporting frame; one ends of n groups of three-period minimal curved surface dot matrix supporting arms are fixedly connected to the outer side of the secondary mirror supporting frame, the other ends are mounted on the lens barrel platform through supporting seats, and n is greater than or equal to 3; each group of three-period minimal curved surface dot matrix supporting arms are tangentially arranged along the circumference of the secondary mirror supporting frame, and the connection positions of the n groups of three-period minimal curved surface dot matrix supporting arms and the secondary mirror supporting frame are uniformly distributed along the circumference of the secondary mirror supporting frame; the three-period minimal curved surface dot matrix supporting arm is of an array structure composed of Gyandroid basic units. The structure provided by the invention can be widely applied to a high-resolution space camera secondary mirror with ultra-light weight, high surface shape precision and high stability requirements and a support thereof, and has a wide application prospect.

The invention relates to a secondary mirror, in particular to a secondary mirror with a high-stability supporting structure. The technical problem that an existing secondary mirror supporting structure is difficult to achieve ideal balance among multiple targets such as high rigidity, low thermal deformation, minimum blocking and light weight is mainly solved. The secondary mirror comprises a secondary mirror supporting shaft, a secondary mirror body, a secondary mirror supporting plate, a secondary mirror supporting frame and a secondary mirror light shield. The secondary mirror body is firstly adhered and fixed on the secondary mirror supporting shaft through adhesive glue, then fixed on the secondary mirror supporting plate through the secondary mirror supporting shaft, fastened by the secondary mirror pressing ring and then fixed on the secondary mirror supporting frame through the secondary mirror supporting plate; and the secondary mirror light shield and the thermal control baffle plate are fixed on the secondary mirror support frame. The secondary mirror provided by the invention has good mechanical and thermal stability and stray light inhibition capability, and can realize ideal balance among multiple targets such as high rigidity, low thermal deformation, minimum blocking and light weight.

The invention relates to a three-mirror anastigmat telescope, comprising at least a primary mirror (1), a secondary mirror (2) positioned in front of the primary mirror (1) such that the primary and secondary mirrors have optical surfaces (1.1, 2.1) opposite one another, a tertiary mirror (3) having an optical surface (3.1) opposite the optical surface (2.1) of the secondary mirror (2), and a first optronic sensor (10) positioned opposite the tertiary mirror (3). The telescope comprises a second optronic sensor (20) positioned behind the secondary mirror (2) and the optical surface of the secondary mirror (2.1) has a dichroic treatment (2') intended to separate an incident luminous flux reflected by the primary mirror (1) into a first luminous flux reflected towards the first optronic sensor (10) via the tertiary mirror (3) and a second luminous flux transmitted to the second optronic sensor (20), the first luminous flux and the second luminous flux being in different spectral bands and the secondary mirror (2) being transparent to the spectral band of the second luminous flux.

This invention relates to the field of optical imaging technology, specifically providing an optical radar co-aperture off-axis imaging system, comprising: an off-axis mirror assembly, a frequency-splitting device, a radar transceiver system, and an optical imaging system. The frequency-splitting device is disposed in the rear optical path of the secondary mirror and is used to reflect light waves and transmit microwaves. The frequency-splitting device includes a frequency-selective surface, which comprises an FSS pattern layer and a bias line layer. The FSS pattern layer includes periodically arranged FSS units. Nonlinear capacitors are electrically connected to the FSS units. The bias line layer applies a voltage to the nonlinear capacitors according to the received microwave band. By changing the voltage applied to the nonlinear capacitors, the resonant frequency of the FSS units is tuned, thereby changing the microwave passband frequency of the frequency-splitting device. This invention not only achieves a reflective wave-transmitting microwave design but also solves the problem that transmitting only a single band of microwaves in microwave-transmitting and light-reflecting methods is difficult to adapt to different task requirements.

The invention discloses an aviation surveying and mapping lens optical system and a lens, particularly discloses a long-focal-length passive athermalization aviation surveying and mapping lens optical system and a lens, and solves the problems that an existing aviation surveying and mapping lens cannot meet the requirements of long-distance and high-precision surveying and mapping and cannot have long focal length, miniaturization and wide temperature adaptability at the same time. The lens optical system comprises a primary lens, a diaphragm, a secondary lens and an aberration correction lens group, the diaphragm is arranged on a reflection light path of the primary mirror; the secondary mirror is arranged on one side, deviating from the primary mirror, of the diaphragm; the aberration correction lens group is arranged in the central through hole of the primary lens; light in a target area enters the primary mirror, passes through the diaphragm to enter the secondary mirror after being reflected by the primary mirror, reversely passes through the diaphragm to enter the aberration correction mirror group after being reflected by the secondary mirror, and then is imaged; the curvature radiuses of the vertexes of the reflecting surfaces of the primary mirror and the secondary mirror are respectively-400mm to-360mm and-220mm to-180mm; the axial interval between the primary mirror and the secondary mirror is-140 mm to-120 mm.