CN102749184A - Large-field-of-view stray light PST (particle swarm optimization) testing method and device - Google Patents

Large-field-of-view stray light PST (particle swarm optimization) testing method and device Download PDF

Info

Publication number
CN102749184A
CN102749184A CN2012102329160A CN201210232916A CN102749184A CN 102749184 A CN102749184 A CN 102749184A CN 2012102329160 A CN2012102329160 A CN 2012102329160A CN 201210232916 A CN201210232916 A CN 201210232916A CN 102749184 A CN102749184 A CN 102749184A
Authority
CN
China
Prior art keywords
light
stray light
pst
field
optical system
Prior art date
Legal status (The legal status is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the status listed.)
Granted
Application number
CN2012102329160A
Other languages
Chinese (zh)
Other versions
CN102749184B (en
Inventor
徐亮
赵建科
周艳
刘峰
张周峰
胡丹丹
张洁
Current Assignee (The listed assignees may be inaccurate. Google has not performed a legal analysis and makes no representation or warranty as to the accuracy of the list.)
XiAn Institute of Optics and Precision Mechanics of CAS
Original Assignee
XiAn Institute of Optics and Precision Mechanics of CAS
Priority date (The priority date is an assumption and is not a legal conclusion. Google has not performed a legal analysis and makes no representation as to the accuracy of the date listed.)
Filing date
Publication date
Application filed by XiAn Institute of Optics and Precision Mechanics of CAS filed Critical XiAn Institute of Optics and Precision Mechanics of CAS
Priority to CN201210232916.0A priority Critical patent/CN102749184B/en
Publication of CN102749184A publication Critical patent/CN102749184A/en
Application granted granted Critical
Publication of CN102749184B publication Critical patent/CN102749184B/en
Active legal-status Critical Current
Anticipated expiration legal-status Critical

Links

Images

Landscapes

  • Photometry And Measurement Of Optical Pulse Characteristics (AREA)
  • Investigating Or Analysing Materials By Optical Means (AREA)

Abstract

一种大视场杂散光PST测试方法及装置,包括大动态范围光源、平行光管、洁净室、高负载转台、EMCCD以及数据采集及处理系统;平行光管设置在大动态范围光源的出射光路上;EMCCD设置在高负载转台上并与数据采集及处理系统电性相连;大动态范围光源与数据采集及处理系统电性相连;高负载转台设置在经平行光管后的出射光路上;大动态范围光源、平行光管、高负载转台、EMCCD以及数据采集及处理系统设置在洁净室内部。本发明提供了一种能够有效的在地面对航天相机遮光罩的杂散光抑制能力进行考核、对相机的整机信噪比进行估算、可保证航天相机发射上天后能够清晰成像以及具有超大视场和高精度的大视场杂散光PST测试方法及装置。

Figure 201210232916

A large field of view stray light PST test method and device, including a large dynamic range light source, a collimator, a clean room, a high-load turntable, an EMCCD, and a data acquisition and processing system; on the road; the EMCCD is set on the high-load turntable and electrically connected with the data acquisition and processing system; the large dynamic range light source is electrically connected with the data acquisition and processing system; the high-load turntable is set on the exit light path after the collimator; the large The dynamic range light source, collimator, high load turntable, EMCCD and data acquisition and processing system are set inside the clean room. The invention provides a method that can effectively evaluate the stray light suppression ability of the space camera hood on the ground, estimate the signal-to-noise ratio of the whole camera, ensure clear imaging of the space camera after it is launched into the sky, and have a super large field of view. Field and high-precision large-field stray light PST test method and device.

Figure 201210232916

Description

Big visual field parasitic light PST method of testing and device
Technical field
The invention belongs to optical field; The method of testing and the device that relate to parasitic light inhibition ability outside a kind of optical system visual field; Relate in particular to a kind of all kinds of optical cameras examination to its parasitic light inhibition ability before the ray machine butt joint that is mainly used in; Especially in the performance test of target detection class camera before emission a little less than the space flight, guaranteed the butt joint of camera ray machine and launch successfully after can blur-free imaging the big visual field parasitic light PST method of testing and the device of purpose.
Background technology
In recent years, along with high sensitivity, the development of low detection threshold detector has had higher requirement to the inhibition of Space Optical System parasitic light, and this just requires the parasitic light measuring system that higher precision is arranged.
Stray light emission is meant in the optical system and is spread in detector (or imaging) lip-deep other non-target (or non-imaging) light radiation ability except target (or imaging light), and arrives the target light beta radiation ability of detector through improper light path.Spaceborne various camera is operated in the rugged surroundings that the intense radiation source is arranged outside the system visual field mostly; Simultaneously; The detected target signal is very faint again; These strong veiling glare radiation usually exceed several magnitude than institute's detection of a target radiation intensity, and through the diffraction in optical system aperture, and the scattering of structure and optical element surface, reflection arrive image planes detector formation parasitic light.The reason that it produces is intricate; Not only relevant with technology, the material of making optical system, also relevant with aberration characteristic, diffraction phenomena, target signature, it obviously reduces camera contrast and modulation transfer function; Whole image planes level reduces; Sharpness degenerates, even forms the veiling glare spot, when serious echo signal is flooded fully by the stray light emission noise.
Parasitic light is one of principal element that influences optical system imaging, and it brightens the detector face background, causes image planes contrast and modulation transfer function to descend, and system signal noise ratio reduces, thereby influence image definition, in the time of seriously even can make thrashing.The outer parasitic light method of testing in the visual field of research is that to survey a type camera with space flight at the high picture element of rail be background, launches that parasitic light inhibition ability calibration technology is studied on ground to camera space.Behind present numerous space flight optics load Heaven, the image quality decrease that all exists the parasitic light problem to bring will directly reduce its transport function like this, influence image quality.
The reason that parasitic light produces mainly contains 3: the scattering of optical system visual field external radiation, optical system internal radiation and imaging light.What the conventional optical systems parasitic light was measured generally use is the blackspot method of testing with integrating sphere after the integral coating.This method of testing can only be verified the stray light emission of target source through producing after the optical system, yet receives the stray light emission that other radiation sources produce outside the visual field for space flight high sensitivity detection class phase chance, and the target contrast that causes descends.Such as; The intense radiation of bright object outside the visual field (sun, the moon, atmosphere system etc.) produces the ground unrest radiation with the parasitic light form on detector after the camera optics system; Influence the detectivity of camera optics system, therefore must study the inhibition problem of parasitic light outside the optical system visual field.Point source transmitance PST (Point Source Transmittance) is an optical system veiling glare index science, detectable, and it has been widely used in design and has estimated high-sensitive target detection system, and has obtained good result.
At present; In the development of various camera spaces; Common parasitic light method of testing or be exactly parasitic light coefficient test in the blackspot method visual field; Be exactly small-bore, small field of view PST test, though these method of testings in the past can satisfy corresponding the use to a certain extent, yet for high sensitivity, diffraction limit level camera; That method of testing in the past seems is less with regard to test specification, measuring accuracy is too low, and parasitic light suppresses the capacity reliability assessment outside the visual field of this type camera thereby can not satisfy.
In the past PST test macro adopts all be high sensitivity PMT detector as receiver, laser instrument is accomplished test as light source; If adopt PMT as detector; Because himself dynamic range when the single photon magnitude is surveyed is less; Often adopt the attenuator group to carry out optical energy attenuation, yet adopt the attenuator group can make luminous energy produce the measuring error that repeatedly reflects and cause in the attenuator component internal; PMT is when surveying faint light simultaneously, and its less stable tends to receive the influence of environment temperature and electromagnetic interference (EMI), and the defective that therefore has to the PMT detector should be studied other a kind of weak light detection method.In addition, if adopt laser instrument as light source, though can obtain higher outgoing luminous energy, in different polychromatic light cameras tests, it is consistent with service condition then can not to satisfy test condition, and luminous energy linear regulation in real time, promptly the light energy output dynamic range is little; Meanwhile, the use of this superpower laser tends to make parallel light tube primary mirror glass surface burn.
Summary of the invention
In order to solve the above-mentioned technical matters that exists in the background technology, the invention provides a kind of can be effectively examine, the machine-noise ratio of camera is estimated, can be guaranteed in the face of the parasitic light inhibition ability of camera space light shield on ground after camera space is launched successfully can blur-free imaging and have ultra-large vision field and high-precision big visual field parasitic light PST method of testing and device.
Technical solution of the present invention is: the invention provides a kind of big visual field parasitic light PST method of testing, its special character is: said method comprising the steps of:
When 1) the collection point target is without optical system to be measured at the responsiveness E of entrance pupil place illumination o
2) install and adjust the position of optical system to be measured, the responsiveness E that the collection point target produces at the image planes place of optical system to be measured during by parasitic light irradiation in different field positions through optical system to be measured d(θ);
3) calculating optical system to be measured field angle outside the visual field according to formula
Figure BDA00001859711000031
is PST (θ) value of θ.
The proving installation of a kind of big visual field parasitic light PST method of testing, its special character is: said proving installation comprises great dynamic range light source, parallel light tube, toilet, is used to adjust high capacity turntable, EMCCD and data acquisition and the disposal system of the different off-axis angles of optical system to be measured; Said parallel light tube is arranged on the emitting light path of great dynamic range light source; Said EMCCD is arranged on the high capacity turntable and with data acquisition and disposal system and is electrical connected; Said great dynamic range light source and data acquisition and disposal system are electrical connected; Said high capacity turntable is arranged on the emitting light path behind the parallel light tube; Said great dynamic range light source, parallel light tube, high capacity turntable, EMCCD and data acquisition and disposal system are arranged on inside, toilet.
Above-mentioned great dynamic range light source comprises integrating sphere, xenon lamp, iris and brightness detector; Said xenon lamp is arranged on integrating sphere inside; The inwall of said integrating sphere is provided with light source inlet and light source outlet; Said light source porch is provided with iris; Said light source exit is provided with brightness detector.
Above-mentioned big visual field parasitic light PST proving installation also comprises chopper and digital lock-in amplifier; Said chopper is arranged on the emitting light path of great dynamic range light source; Said EMCCD links to each other with chopper through digital lock-in amplifier; Said data acquisition and disposal system are electrical connected with chopper and digital lock-in amplifier respectively.
Above-mentioned big visual field parasitic light PST proving installation also comprises and is used to eliminate and reduces environment parasitic light that the outlet reflected light of optical system to be measured the causes twin columns jar to target source parasitic light tests affect; It is inner that said EMCCD and optical system to be measured are arranged on the twin columns jar.
Above-mentioned big visual field parasitic light PST proving installation comprises that also cover is connected to optical system to be measured and is used to suppress the eliminate stray light light shield that parasitic light is treated the optical property influence of photometry system, and it is inner that said eliminate stray light light shield is arranged on the twin columns jar.
Above-mentioned toilet is not less than 100 grades toilet.
Above-mentioned parallel light tube is from the axle parallel light tube.
Advantage of the present invention is:
The present invention has analyzed back, camera space Heaven because the problem that parasitic light brought outside the visual field; In conjunction with parasitic light test philosophy outside traditional blackspot method and the low precision visual field; A kind of method and device that suppresses ability at ground calibration camera space parasitic light proposed; Can effectively face the parasitic light inhibition ability of camera space light shield and examine, the machine-noise ratio of camera is estimated, propose light shield modified form design proposal on ground; Guaranteed that camera space can blur-free imaging after launching successfully, its beneficial effect is:
Method provided by the present invention can accurately be verified the inhibition ability of camera parasitic light in different visual fields, and its test PST test specification can extend to 10 -1~10 -12Guarantee camera space ability blur-free imaging behind the Heaven fully; This method of accurately testing in the face of the camera space parasitic light on ground will become the gordian technique of camera space at the rail blur-free imaging; Consider that this important function for of research is the gordian technique that is used in the test of rail camera space parasitic light, this Study on Technology success is with indicating that domestic camera space parasitic light ground calibration technique gets into a new step.Therefore, carry out the big visual field of camera space, high precision parasitic light Study on Technology, will play the promotion effect the development of China's space flight optics load.
The present invention the big visual field of the high precision parasitic light PST proving installation that provided; Utilize point source transmitance principle,, proposed parasitic light method of testing outside the visual field, the big visual field of a kind of high precision in conjunction with traditional parasitic light method of testing; Its measuring accuracy is broken through measuring accuracy in the past, and the PST measured value is from original 10 -8Be increased to 10 -12Simultaneously,, first whole experiment device is arranged on class 100 clean room in order to eliminate the influence of environment parasitic light, thus reduce micronic dust particle in the air to cause Rayleigh scattering and the environment parasitic light that produces to the influence of test; The 3rd, the present invention utilizes optics wave chopping technology and digital lock-in technique, has realized the purpose of the faint parasitic light signal extraction of the dark target of bright background; The 4th, the present invention has adopted a kind of great dynamic range light source, and at a kind of detector that can monitor outlet luminous energy in real time of light source set inside, has guaranteed that outgoing luminous energy is 10 -4~10 4W/m 2/ sr is accurately adjustment dynamically, and this method has substituted attenuator decay lumen method in the past fully, thereby has improved measuring accuracy; The 5th, the present invention adopts special twin columns jar section structure, is to be installed in the twin columns jar with tested camera optics, can effectively eliminate and reduce the influence of environmental radiation parasitic light to measuring that optical system reflection to be measured produces; The 6th, the present invention has also disposed the heavy caliber parallel light tube, has broken through and can survey the little defective in parasitic light visual field ± 30 ° in the past, and its parasitic light can survey field range and be extended to ± and 65 °.
Description of drawings
Fig. 1 is the structural representation of proving installation provided by the present invention;
1-100 level toilet; 2-twin columns jar; 3-high capacity turntable; 4-EMCCD; 5-optical system to be measured; 6-eliminate stray light light shield; 7-is from the axle parallel light tube; 8-data acquisition and disposal system; The 9-digital lock-in amplifier; 10-great dynamic range light source; The 11-chopper.
Embodiment
The invention provides a kind of big visual field parasitic light PST method of testing, this method comprises:
When 1) the collection point target is without optical system to be measured at the responsiveness E of entrance pupil place illumination o
2) install and adjust the position of optical system to be measured, the responsiveness E that the collection point target produces at the image planes place of optical system to be measured during by parasitic light irradiation in different field positions through optical system to be measured d(θ);
3) calculating optical system to be measured field angle outside the visual field according to formula
Figure BDA00001859711000051
is PST (θ) value of θ.
Simultaneously, the present invention also provides based on the formed a kind of big visual field of this method parasitic light PST proving installation when big visual field parasitic light PST method of testing is provided.Referring to Fig. 1, big visual field provided by the present invention parasitic light PST device comprises: class 100 clean room 1, twin columns jar 2, high capacity turntable 3, EMCCD4, optical system to be measured 5, eliminate stray light light shield 6, form 8 from an axle parallel light tube 7, digital lock-in amplifier 9, great dynamic range light source 10, chopper 11 and data acquisition and disposal system.
Parallel light tube is arranged on the emitting light path of great dynamic range light source 10; EMCCD4 is arranged on the high capacity turntable 3 and with data acquisition and disposal system 8 and is electrical connected; Great dynamic range light source and data acquisition and disposal system are electrical connected; The high capacity turntable is arranged on the emitting light path behind the parallel light tube; Great dynamic range light source, parallel light tube, high capacity turntable, EMCCD and data acquisition and disposal system are arranged on inside, toilet.
The great dynamic range light source comprises integrating sphere, xenon lamp, iris and brightness detector; Xenon lamp is arranged on integrating sphere inside; The inwall of integrating sphere is provided with light source inlet and light source outlet; The light source porch is provided with iris; The light source exit is provided with brightness detector.
Big visual field parasitic light PST proving installation also comprises chopper 11 and digital lock-in amplifier 9; Chopper 11 is arranged on the emitting light path of great dynamic range light source 10; EMCCD4 links to each other with chopper 11 through digital lock-in amplifier 9; Data acquisition and disposal system 8 are electrical connected with chopper 11 and digital lock-in amplifier 9 respectively.It is inner that EMCCD4 and optical system to be measured 5 are arranged on the twin columns jar, and eliminate stray light light shield 6 is arranged on twin columns jar 2 inside, and cover is connected on the optical system 5 to be measured.
The toilet is not less than 100 grades various toilets, and parallel light tube is from an axle parallel light tube.
Principle of work of the present invention is: select for use great dynamic range integrating sphere (great dynamic range light source 10) to be parallel light tube (from axle parallel light tube 7) pointolite; High-power xenon lamp is arranged in the integrating sphere; Simultaneously iris is set,, and near outlet, the spoke brightness detector is set by its outlet spoke brightness of its controller control in integrating sphere inwall light source porch; Can monitor the size of outlet spoke brightness in real time, the whole scope of its emergent light spoke adjustable brightness is 0~10 4W/m 2/ sr.Be arranged on parallel light tube (from axle parallel light tube 7) focal plane place with the integrating sphere outlet this moment, is a uniform heavy caliber light beam through parallel light tube (from axle parallel light tube 7) collimation, can be full of tested optical system (optical system 5 to be measured) entrance pupil fully.
Before parasitic light test, earlier whole testing device is placed in the class 100 clean room 1, can reduce the influence that dust granule in the air causes the environment parasitic light that Rayleigh scattering produces like this.At first high sensitivity EMCCD4 is placed on high precision turntable (high capacity turntable 3) rotation center place; Adjustment integrating sphere outlet spoke brightness size; And EMCCD4 gain and time shutter thereof be set; The response that makes its CCD is in the saturation degree scope, and measure the collimated light beam of outgoing this moment, is the responsiveness of tested optical system entrance pupil place illumination.Again optical system 5 to be measured is positioned on the twin columns jar 2 interior high precision turntable (high capacity turntable 3); Tested camera entrance pupil is overlapped with high precision turntable (the high capacity turntable 3) centre of gyration, guarantee tested camera optical axis and parallel light tube (from axle parallel light tube 7) optical axis coincidence simultaneously.EMCCD4 is installed at optical system (optical system 5 to be measured) image planes place, both position relative fixed of EMCCD4 and optical system (optical system 5 to be measured), and rotate with turntable (high capacity turntable 3).By beginning outside optical system to be measured 5 visual fields; Every at a distance from a fixed angle; Gain and the time shutter of adjustment light source place's spoke brightness and EMCCD4; Guarantee that image planes irradiance at the diverse location place all less than the saturation degree of EMCCD4, gathers the responsiveness of different field positions parasitic light irradiation, the ratio of the responsiveness at this responsiveness and optical system entrance pupil to be measured place is that field angle is the PST value of θ outside its visual field:
PST ( θ ) = E d ( θ ) E o - - - ( 1 )
In the formula: θ is the Point Target of field angle outside the optical system visual field, and PST (θ) is tested camera parasitic light rejection ratio, E d(θ) be the illumination that point target produces at the image planes place through optical system, E oThe illumination that goes out for the optical system entrance pupil.
During test; In order to guarantee that EMCCD4 can respond extremely weak parasitic light luminous energy, in the light source exit chopper 11 is set when off-axis angle is big; Use chopper 11 that light signal is modulated to the high-frequency signal of frequency as 1500HZ; From strong low frequency signal, extract the target parasitic light high-frequency signal that frequency is 1500HZ through digital lock-in amplifier 9, thereby can guarantee that EMCCD4 under extremely weak parasitic light situation, can isolate the echo signal parasitic light from the environment parasitic light.The light energy signal that utilizes data acquisition and disposal system 8 that different visual fields are collected at last can calculate the corresponding PST value of each off-axis angle according to formula (1).
Wherein the function of each several part is introduced as follows:
Class 100 clean room 1 mainly is in order to reduce the Rayleigh scattering that the micronic dust granulin molecule is produced in the air, and then the measuring error that causes the environment parasitic light to cause.
Twin columns jar 2 is mainly in order to eliminate and reduce the influence to the test of target source parasitic light of environment parasitic light that tested camera outlet reflected light causes;
High capacity turntable 3 mainly provides tested camera different off-axis angles, satisfies the parasitic light test of different field angle.
The effect of EMCCD4 mainly is because it has the detectivity of high sensitivity single photon magnitude; Be applicable to very much the detection of this extremely weak parasitic light; In addition, EMCCD4 has the consistent characteristic of great dynamic range detection performance linear response, can satisfy the requirement of great dynamic range PST test.
Optical system 5 to be measured is testpieces of this method of testing, is used to verify the feasibility of this method of testing.
Eliminate stray light light shield 6 links together with optical system 5 to be measured, and mainly in order to suppress parasitic light to tested camera optics Effect on Performance, this test mainly is in order to verify that the optical system 5 to be measured and the parasitic light of eliminate stray light light shield 6 suppress ability.
The point target source of infinite distant place mainly is provided from axle parallel light tube 7.
Data processing, the curve plotting of PST test are accomplished in data acquisition and the disposal system 8 main parasitic light collections of accomplishing optical system 5 to be measured at different off-axis angles simultaneously.
Digital lock-in amplifier 9 is mainly used in and from strong low frequency signal, extracts target parasitic light high-frequency signal.
Chopper 11 is that the light source echo signal is modulated to high-frequency signal; Digital lock-in amplifier 9 cooperates chopper 11 can accomplish the rejecting of weak target parasitic light signal and environment parasitic light, satisfies the effect that the dark target of bright background is extracted.
Great dynamic range light source 10 main light ray radiations in order to provide the simulation test spectral range to use can accurately simulate 10 simultaneously -4~10 4W/m 2The dynamic change of/sr luminous energy has thoroughly improved and had realized the defective that great dynamic range luminous energy changes with attenuator in the past, cooperates the EMCCD of great dynamic range detectivity, can realize that the PST value is 10 -12Test.

Claims (8)

1.一种大视场杂散光PST测试方法,其特征在于:所述大视场杂散光PST测试方法包括以下步骤:1. a large field of view stray light PST test method, characterized in that: the large field of view stray light PST test method comprises the following steps: 1)采集点目标未经待测光学系统时在入瞳处照度的响应度Eo1) The responsivity E o of the illuminance at the entrance pupil when the target at the collection point is not in the optical system to be tested; 2)安装并调整待测光学系统的位置,采集点目标经过待测光学系统在不同视场位置由杂散光辐照时在待测光学系统的像面处产生的响应度Ed(θ);2) Install and adjust the position of the optical system to be tested, and collect the responsivity E d (θ) generated at the image plane of the optical system to be tested when the target passes through the optical system to be tested and is irradiated by stray light at different positions of the field of view; 3)根据公式
Figure FDA00001859710900011
计算待测光学系统在视场外视场角为θ的PST(θ)值。
3) According to the formula
Figure FDA00001859710900011
Calculate the PST(θ) value of the optical system under test with the field angle θ outside the field of view.
2.一种基于权利要求1所述的大视场杂散光PST测试方法的测试装置,其特征在于:所述测试装置包括大动态范围光源、平行光管、洁净室、用于调整待测光学系统不同离轴角的高负载转台、EMCCD以及数据采集及处理系统;所述平行光管设置在大动态范围光源的出射光路上;所述EMCCD设置在高负载转台上并与数据采集及处理系统电性相连;所述大动态范围光源与数据采集及处理系统电性相连;所述高负载转台设置在经平行光管后的出射光路上;所述大动态范围光源、平行光管、高负载转台、EMCCD以及数据采集及处理系统设置在洁净室内部。2. A test device based on the large field of view stray light PST test method according to claim 1, characterized in that: the test device includes a large dynamic range light source, a collimator, a clean room, and is used to adjust the optical High-load turntables with different off-axis angles, EMCCD and data acquisition and processing systems; the collimator is set on the exit light path of the large dynamic range light source; the EMCCD is set on the high-load turntable and connected with the data acquisition and processing system Electrically connected; the large dynamic range light source is electrically connected to the data acquisition and processing system; the high-load turntable is set on the outgoing light path after passing through the collimator; the large dynamic range light source, collimator, and high-load The turntable, EMCCD and data acquisition and processing system are set inside the clean room. 3.根据权利要求2所述的大视场杂散光PST测试装置,其特征在于:所述大动态范围光源包括积分球、氙灯、可变光阑以及亮度检测器;所述氙灯设置在积分球内部;所述积分球的内壁上设置有光源入口以及光源出口;所述光源入口处设置有可变光阑;所述光源出口处设置有亮度检测器。3. large field of view stray light PST testing device according to claim 2, is characterized in that: described large dynamic range light source comprises integrating sphere, xenon lamp, iris diaphragm and brightness detector; Described xenon lamp is arranged on integrating sphere Inside: a light source inlet and a light source outlet are arranged on the inner wall of the integrating sphere; a variable diaphragm is arranged at the light source inlet; a brightness detector is arranged at the light source outlet. 4.根据权利要求2或3所述的大视场杂散光PST测试装置,其特征在于:所述大视场杂散光PST测试装置还包括斩光器以及数字锁相放大器;所述斩光器设置在大动态范围光源的出射光路上;所述EMCCD通过数字锁相放大器与斩光器相连;所述数据采集及处理系统分别与斩光器和数字锁相放大器电性相连。4. The large-field stray light PST testing device according to claim 2 or 3, characterized in that: the large-field stray light PST testing device also includes a light chopper and a digital lock-in amplifier; the light chopper It is arranged on the exit light path of a large dynamic range light source; the EMCCD is connected to the optical chopper through a digital lock-in amplifier; the data acquisition and processing system is electrically connected to the optical chopper and the digital lock-in amplifier respectively. 5.根据权利要求4所述的大视场杂散光PST测试装置,其特征在于:所述大视场杂散光PST测试装置还包括用于消除和减少待测光学系统的出口反射光造成的环境杂散光对目标源杂散光测试影响的双柱罐;所述EMCCD以及待测光学系统设置在双柱罐内部。5. The large field of view stray light PST test device according to claim 4, characterized in that: the large field of view stray light PST test device also includes an environment for eliminating and reducing the exit reflected light of the optical system to be tested. A double-column tank for the influence of stray light on the target source stray light test; the EMCCD and the optical system to be tested are arranged inside the double-column tank. 6.根据权利要求5所述的大视场杂散光PST测试装置,其特征在于:所述大视场杂散光PST测试装置还包括罩接于待测光学系统并用于抑制杂散光对待测光学系统的光学性能影响的消杂光遮光罩,所述消杂光遮光罩设置在双柱罐内部。6. The large field of view stray light PST test device according to claim 5, characterized in that: the large field of view stray light PST test device also includes a cover connected to the optical system to be tested and used to suppress stray light from the optical system to be tested The stray light shading cover affected by the optical performance, the stray light shading cover is arranged inside the double-column tank. 7.根据权利要求6所述的大视场杂散光PST测试装置,其特征在于:所述洁净室是不低于100级的洁净室。7. The large-field stray light PST test device according to claim 6, characterized in that: the clean room is a clean room not lower than Class 100. 8.根据权利要求7所述的大视场杂散光PST测试装置,其特征在于:所述平行光管是离轴平行光管。8 . The large field of view stray light PST test device according to claim 7 , wherein the collimator is an off-axis collimator.
CN201210232916.0A 2012-07-06 2012-07-06 Large-field-of-view stray light PST (particle swarm optimization) testing method and device Active CN102749184B (en)

Priority Applications (1)

Application Number Priority Date Filing Date Title
CN201210232916.0A CN102749184B (en) 2012-07-06 2012-07-06 Large-field-of-view stray light PST (particle swarm optimization) testing method and device

Applications Claiming Priority (1)

Application Number Priority Date Filing Date Title
CN201210232916.0A CN102749184B (en) 2012-07-06 2012-07-06 Large-field-of-view stray light PST (particle swarm optimization) testing method and device

Publications (2)

Publication Number Publication Date
CN102749184A true CN102749184A (en) 2012-10-24
CN102749184B CN102749184B (en) 2015-01-07

Family

ID=47029552

Family Applications (1)

Application Number Title Priority Date Filing Date
CN201210232916.0A Active CN102749184B (en) 2012-07-06 2012-07-06 Large-field-of-view stray light PST (particle swarm optimization) testing method and device

Country Status (1)

Country Link
CN (1) CN102749184B (en)

Cited By (19)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN103149016A (en) * 2013-02-27 2013-06-12 中国科学院西安光学精密机械研究所 Stray light detection method and system for optical system to be detected
CN103454072A (en) * 2013-08-26 2013-12-18 中国科学院西安光学精密机械研究所 Stray light coefficient and point source transmittance composite test method and system
CN103868526A (en) * 2014-02-24 2014-06-18 北京空间机电研究所 Method for detecting stray light outside field of view of space optical remote senor three-mirror coaxial optical system
CN104655056A (en) * 2015-01-26 2015-05-27 中国空空导弹研究院 System and method for calibrating angle zero position of infrared imaging product
CN104865048A (en) * 2015-06-02 2015-08-26 中国科学院上海技术物理研究所 Stray light measurement device and measurement method
CN105407347A (en) * 2015-10-30 2016-03-16 南京理工大学 Low-illuminance CMOS SNR (single to noise ratio) testing device
CN105445570A (en) * 2015-12-16 2016-03-30 中国科学院西安光学精密机械研究所 Wide-angle lens camera signal-to-noise ratio testing system and measuring method
CN108036928A (en) * 2017-12-15 2018-05-15 中国科学院西安光学精密机械研究所 Entrance pupil voltage value calibration method and system in PST test and PST test system
CN108169187A (en) * 2017-12-15 2018-06-15 中国科学院西安光学精密机械研究所 Test cavity for point source transmittance test
CN108254815A (en) * 2017-12-27 2018-07-06 中国科学院西安光学精密机械研究所 Double-column tank splicing and adjusting method
CN108535862A (en) * 2018-03-09 2018-09-14 中国科学院长春光学精密机械与物理研究所 A kind of emulation modelling method calculating space remote sensing camera black-spot method coefficient of stray light
CN108680188A (en) * 2018-06-21 2018-10-19 中国科学院西安光学精密机械研究所 PST (Power System test) and extremely weak target simulation system and PST and detection capability test method
CN109489940A (en) * 2018-11-02 2019-03-19 中国科学院西安光学精密机械研究所 An accurate time-lapse measurement method for an optical imaging system
CN109813536A (en) * 2019-03-14 2019-05-28 长春理工大学 An infrared optical system external stray light test device and test method
WO2020205425A1 (en) 2019-04-02 2020-10-08 Waymo Llc Stray-light testing station
CN113711002A (en) * 2019-04-17 2021-11-26 伟摩有限责任公司 Stray light testing vehicle for vehicle
CN114236510A (en) * 2021-12-02 2022-03-25 桂林理工大学 System for testing laser radar transmittance stray light in water depth measurement
CN115243017A (en) * 2022-08-03 2022-10-25 上海研鼎信息技术有限公司 Method and equipment for improving image quality
CN115753017A (en) * 2022-11-09 2023-03-07 中国科学院长春光学精密机械与物理研究所 Method for determining stray light of point source of space telescope, optical equipment and medium

Citations (4)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN101178337A (en) * 2006-11-07 2008-05-14 中国科学院西安光学精密机械研究所 Large-aperture stray light coefficient test method and system based on computational holographic element
CN201359534Y (en) * 2008-11-21 2009-12-09 聚光科技(杭州)有限公司 Device for measuring stray light ratio in spectrometer
CN101750097A (en) * 2008-12-17 2010-06-23 中国科学院西安光学精密机械研究所 Standard starlight simulator and stray light PST optical detection system containing the simulator
CN202710290U (en) * 2012-07-06 2013-01-30 中国科学院西安光学精密机械研究所 Large-view-field stray light PST testing device

Patent Citations (4)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN101178337A (en) * 2006-11-07 2008-05-14 中国科学院西安光学精密机械研究所 Large-aperture stray light coefficient test method and system based on computational holographic element
CN201359534Y (en) * 2008-11-21 2009-12-09 聚光科技(杭州)有限公司 Device for measuring stray light ratio in spectrometer
CN101750097A (en) * 2008-12-17 2010-06-23 中国科学院西安光学精密机械研究所 Standard starlight simulator and stray light PST optical detection system containing the simulator
CN202710290U (en) * 2012-07-06 2013-01-30 中国科学院西安光学精密机械研究所 Large-view-field stray light PST testing device

Non-Patent Citations (1)

* Cited by examiner, † Cited by third party
Title
王治乐等: "基于点源透过率的空间光学系统杂光测量", 《光学技术》 *

Cited By (32)

* Cited by examiner, † Cited by third party
Publication number Priority date Publication date Assignee Title
CN103149016A (en) * 2013-02-27 2013-06-12 中国科学院西安光学精密机械研究所 Stray light detection method and system for optical system to be detected
CN103454072A (en) * 2013-08-26 2013-12-18 中国科学院西安光学精密机械研究所 Stray light coefficient and point source transmittance composite test method and system
CN103454072B (en) * 2013-08-26 2015-12-23 中国科学院西安光学精密机械研究所 stray light coefficient and point source transmittance composite test method and system
CN103868526A (en) * 2014-02-24 2014-06-18 北京空间机电研究所 Method for detecting stray light outside field of view of space optical remote senor three-mirror coaxial optical system
CN104655056A (en) * 2015-01-26 2015-05-27 中国空空导弹研究院 System and method for calibrating angle zero position of infrared imaging product
CN104865048B (en) * 2015-06-02 2017-06-27 中国科学院上海技术物理研究所 A kind of stray light measuring device and measuring method
CN104865048A (en) * 2015-06-02 2015-08-26 中国科学院上海技术物理研究所 Stray light measurement device and measurement method
CN105407347A (en) * 2015-10-30 2016-03-16 南京理工大学 Low-illuminance CMOS SNR (single to noise ratio) testing device
CN105445570B (en) * 2015-12-16 2018-05-29 中国科学院西安光学精密机械研究所 Wide-angle lens camera signal-to-noise ratio testing system and measuring method
CN105445570A (en) * 2015-12-16 2016-03-30 中国科学院西安光学精密机械研究所 Wide-angle lens camera signal-to-noise ratio testing system and measuring method
CN108036928A (en) * 2017-12-15 2018-05-15 中国科学院西安光学精密机械研究所 Entrance pupil voltage value calibration method and system in PST test and PST test system
CN108036928B (en) * 2017-12-15 2023-09-01 中国科学院西安光学精密机械研究所 Entrance pupil voltage calibration method and system in PST test and PST test system
CN108169187A (en) * 2017-12-15 2018-06-15 中国科学院西安光学精密机械研究所 Test cavity for point source transmittance test
CN108169187B (en) * 2017-12-15 2024-05-10 中国科学院西安光学精密机械研究所 Test cavity for testing point source transmittance
CN108254815A (en) * 2017-12-27 2018-07-06 中国科学院西安光学精密机械研究所 Double-column tank splicing and adjusting method
CN108254815B (en) * 2017-12-27 2019-12-03 中国科学院西安光学精密机械研究所 Splicing and adjusting method of double-column tank
CN108535862A (en) * 2018-03-09 2018-09-14 中国科学院长春光学精密机械与物理研究所 A kind of emulation modelling method calculating space remote sensing camera black-spot method coefficient of stray light
CN108535862B (en) * 2018-03-09 2020-02-14 中国科学院长春光学精密机械与物理研究所 Simulation modeling method for calculating stray light coefficient of spatial remote sensing camera black spot method
CN108680188A (en) * 2018-06-21 2018-10-19 中国科学院西安光学精密机械研究所 PST (Power System test) and extremely weak target simulation system and PST and detection capability test method
CN108680188B (en) * 2018-06-21 2023-09-01 中国科学院西安光学精密机械研究所 PST test and extremely weak target simulation system and PST and detection capability test method
CN109489940A (en) * 2018-11-02 2019-03-19 中国科学院西安光学精密机械研究所 An accurate time-lapse measurement method for an optical imaging system
CN109813536A (en) * 2019-03-14 2019-05-28 长春理工大学 An infrared optical system external stray light test device and test method
US11635326B2 (en) 2019-04-02 2023-04-25 Waymo Llc Stray-light testing station
US11933666B2 (en) 2019-04-02 2024-03-19 Waymo Llc Stray-light testing station
WO2020205425A1 (en) 2019-04-02 2020-10-08 Waymo Llc Stray-light testing station
CN113711002B (en) * 2019-04-17 2023-06-06 伟摩有限责任公司 Stray light test vehicle for vehicle
CN113711002A (en) * 2019-04-17 2021-11-26 伟摩有限责任公司 Stray light testing vehicle for vehicle
CN114236510B (en) * 2021-12-02 2023-06-23 桂林理工大学 Depth measurement lidar transmittance stray light test system
CN114236510A (en) * 2021-12-02 2022-03-25 桂林理工大学 System for testing laser radar transmittance stray light in water depth measurement
CN115243017A (en) * 2022-08-03 2022-10-25 上海研鼎信息技术有限公司 Method and equipment for improving image quality
CN115243017B (en) * 2022-08-03 2024-06-07 上海研鼎信息技术有限公司 Method and equipment for improving image quality
CN115753017A (en) * 2022-11-09 2023-03-07 中国科学院长春光学精密机械与物理研究所 Method for determining stray light of point source of space telescope, optical equipment and medium

Also Published As

Publication number Publication date
CN102749184B (en) 2015-01-07

Similar Documents

Publication Publication Date Title
CN102749184A (en) Large-field-of-view stray light PST (particle swarm optimization) testing method and device
CN202710290U (en) Large-view-field stray light PST testing device
CN103234734B (en) large-caliber stray light testing device and testing method
Kern et al. Theoretical description of functionality, applications, and limitations of SO 2 cameras for the remote sensing of volcanic plumes
CN111060289B (en) A high-sensitivity coronagraph stray light detection device
CN102486404A (en) Ultraviolet low-light star equal simulation and star equal calibration system
CN202522516U (en) Optical transmissivity test device
CN103149016A (en) Stray light detection method and system for optical system to be detected
CN102175431A (en) Device for measuring point source stray light transmission coefficient in large dynamic range
CN101750097A (en) Standard starlight simulator and stray light PST optical detection system containing the simulator
CN103454072B (en) stray light coefficient and point source transmittance composite test method and system
CN203479497U (en) Stray light coefficient and point source transmittance composite test system
CN108680188B (en) PST test and extremely weak target simulation system and PST and detection capability test method
Kong et al. Feasibility investigation of a monostatic imaging lidar with a parallel-placed image sensor for atmospheric remote sensing
CN102393212A (en) A Weak Target Ultraviolet Magnitude Calibration System
CN201983798U (en) An ultraviolet weak light magnitude simulation and magnitude calibration system
CN203132818U (en) Stray light detection system of optical system to be detected
CN202420508U (en) Large-caliber stray light eliminating star simulator system
CN103206963B (en) Large-caliber stray light eliminating star simulator system
CN107576390A (en) A kind of atomic weak multiband infrared radiation degree measuring system and method
CN101846528A (en) Detection method for capture capability of photoelectric tracking equipment to target with low contrast
CN108535862A (en) A kind of emulation modelling method calculating space remote sensing camera black-spot method coefficient of stray light
CN117664520A (en) A spatially wide spectrum sun/moon simulator
CN102636336B (en) Method for testing operating distance of active near-infrared camera based on equivalent illumination and MRC (Minimum Resolvable Contrast)
CN114235346B (en) Diffraction stray light inhibition ratio test system and method based on optical cavity absorption

Legal Events

Date Code Title Description
C06 Publication
PB01 Publication
C10 Entry into substantive examination
SE01 Entry into force of request for substantive examination
C14 Grant of patent or utility model
GR01 Patent grant