首页|折/衍混合光学系统在纳型星敏感器中的应用

折/衍混合光学系统在纳型星敏感器中的应用

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微纳卫星是一种新兴的微小卫星,与之适配的纳型星敏感器的光学系统应在小型化的同时实现大相对孔径、高成像质量。针对这一需求,由星敏感器的系统设计精度和探测星等分配了光学系统设计参数及指标,设计了一种全视场17°、焦距25 mm、相对孔径1∶1。086、光学系统总长36。4 mm的七片式折衍混合结构的星敏感器光学系统。根据衍射元件的负色散特性,用折衍混合透镜代替常规材料正负透镜组合的方式减少了镜片数量,缩短了光学系统长度,并提高了光学系统的成像质量,使点扩散函数趋于正态分布,有利于质心提取精度的提高。所设计的光学系统在3×3像元内的能量集中度超过90%;最大畸变仅0。013%;全视场垂轴色差小于0。6 μm。通过标量衍射理论计算衍射元件在520~780 nm内衍射效率可以达80%以上,通过杂散光分析软件ASAP对系统进行了视场内鬼像分析,系统在多级衍射时探测目标成像光斑路径下的光通量与最亮鬼像光斑路径下的光通量之比大于3。17×104,验证了在极限星等为6。5时满足信噪比大于8。1的结论。最后对所设计的系统进行了公差分析,结果表明加工后该光学系统可满足微纳卫星对星敏感器的使用要求。
Application of Refraction/diffraction Hybrid Optical System in Nano Star Sensor
Micro-nano satellite is a new kind of micro-satellite and is widely used.Nano sensor adapted to it should have the characteristics of small size,high precision and high detection sensitivity.Therefore,the optical system of nano star sensor should achieve large relative aperture and high imaging quality while miniaturization.Aiming at the requirement of nano star sensor optical system,the field of view and focal length of optical system are calculated by the system design accuracy index of star sensor.From the detection magnitude and SNR,the sensitivity model of star sensor and the diffraction efficiency formula are used to calculate the optical system's entry pupil aperture and detection band.A star sensor optical system with full field of view of 17°,focal length of 25 mm and relative aperture of 1:1.086 is designed.According to the negative dispersion characteristics of diffractive elements,the number of lenses is reduced by using a hybrid lens instead of a set of conventional material positive and negative lenses,and the total length of the optical system is shortened from 48 mm to 36.4 mm.In order to illustrate the advantages of this structure,various imaging indexes are compared.The results show that the addition of diffraction surface makes the point diffusion function tend to normal distribution,which is conducive to improving the accuracy of centroid extraction.The optical modulation transfer function at Nyquist frequency increases above 0.4.The maximum dispersion spot size of the optical system is 4.333 μm,and the value is 7.277 μm without addition.The energy concentration in 33 pixels is more than 90%;without joining,the value is 80%;the vertical color difference of the full field of view is less than 0.6 μm,while the value is more than 1.1 μm without addition,so the angle measurement error caused by the color deviation of the center of mass is controlled within 4.75".The diffraction efficiency of the diffraction element in the range of 520~780 nm is calculated by the scalar diffraction theory.The ghost image in the field of view of the system is analyzed by the stray light analysis software ASAP.The results show that,the ratio of luminous flux under the path of the image spot and the brightest ghost spot is greater than 3.94×104 in the primary diffraction,and the ratio of luminous flux under the path of the image spot and the brightest ghost spot is greater than 3.17×104 in the multi-level diffraction.There is no difference in the distribution position of the main ghost image in the two cases,only in the luminous flux value.According to the theoretical calculation of the maximum luminous flux of the system ghost image,when the limit magnitude is 6.5 and the signal-to-noise ratio is 8.1,the luminous flux ratio of the detection target under the image spot path and the luminous flux under the brightest ghost image spot path should be at least greater than 1.42×104.Therefore,the results of ASAP ghost tracking verify that the hybrid system meets the requirement of a signal-to-noise ratio greater than 8.1 when the limit magnitude is 6.5.The results show that when the deviation of aperture number is less than±2,curvature radius,thickness,eccentricity is less than±0.02 mm,inclination is less than±0.02°,refractive index deviation is less than±0.005,Abbe number deviation is less than±0.5,the dispersion spot radius has an 80%probability better than 6.98.It has a 90%probability better than 7.53 μm,which can meet the requirements of energy concentration greater than 90%in 3×3 pixels.

Nano star sensorOptical designRefraction diffraction hybrid optical systemLarge relative apertureDiffraction surfaceGhost image

邓骞、张国玉、孟遥、孙高飞、杜宗育

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长春理工大学 光电工程学院,长春 130022

光电测控与光电信息传输技术教育部重点实验室,长春 130022

吉林省光电测控仪器工程技术研究中心,长春 130022

纳型星敏感器 光学设计 折衍混合光学系统 大相对孔径 衍射面 鬼像

吉林省科技发展计划吉林省教育厅科学技术研究项目

20220201094GXJJKH20220754KJ

2024

光子学报
中国光学学会 中国科学院西安光学精密机械研究所

光子学报

CSTPCD北大核心
影响因子:0.948
ISSN:1004-4213
年,卷(期):2024.53(6)