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环形光源斐索干涉系统光学设计

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针对斐索干涉系统抑制相干噪声和提高面形误差检测能力的需求,阐述环形光源抑制相干噪声的原理,介绍干涉仪的仪器传递函数(ITF)理论与台阶板检测ITF的方法,提出了被测面口径分别为φ100 mm、φ810 mm的两套环形光源斐索干涉系统的方案,使用轴锥镜产生实环形光源,并采用了 φ100mm、φ810 mm系统复用部分镜组的设计思路,可有效降低φ810 mm系统装调的难度。搭建实验系统时发现相干噪声得到了较好的抑制,但是用台阶板测得的系统的ITF较差。实验发现部分由台阶板反射回来的光无法进入成像镜组,更换为口径更大的成像镜组后,能使更多的光通过,且此时测得的ITF有了显著提高。分析了产生这一现象的原因,并采用了可以同时优化干涉系统的干涉光路与成像光路的方案,进而设计出了具有7。2 mm-1面形误差检测能力的φ100 mm系统以及0。4 mm-1面形误差检测能力的φ810 mm系统。
Optical Design of Fizeau Interference System with Ring Light Source
Objective In modern optical processing and inspection,laser interferometers are widely employed to detect the surface shape of optical components.In the process of surface shape detection,due to the temporal coherence of the laser,the optical elements in the interferometer such as bubbles,scratches,defects,and surface dust will produce coherent noises.As a result,these noises will change the phase distribution of the interference signal,affect the results of the interferometry,and need to be suppressed.The ring light source can be produced by axicon,and it can reduce the influence of interferometer coherent noise.Additionally,with the development of optical technology,there is a growing demand for the ability of interferometers to detect surface errors at higher spatial frequencies.The instrument transfer function(ITF)of an interferometer can be utilized to evaluate the ability to resolve surface errors of different spatial frequencies and is an important performance index of an interferometer system.Meanwhile,this function is usually measured by a standard step plate.In our study,two sets of ring light source Fizeau interference systems with diameters of φ100 mm and φ810 mm are proposed.Methods The axicon is employed to generate a solid ring light source,and the design idea that φ100 mm and φ810 mm systems leverage common lens groups is adopted,which can lower the difficulty in the installation of φ810 mm systems.It is found that the coherent noise is suppressed well,but the ITF of the system measured by the step plate is poor.Additionally,part of the light reflected by the step plate can not enter the imaging lens group,and more light can pass through after replacing the imaging lens group with a larger aperture.Since the analysis of the imaging process of the interference system to the step plate shows that the interference optical path and imaging optical path of the system can be adopted for simulation,the scheme of optimizing the interference path and imaging path simultaneously is chosen to design the interference system with the ability to detect the middle-frequency surface shape errors.Results and Discussions We design the φ100 mm and φ810 mm systems with a completely consistent ring light source,beam splitter prism,beam expanding lens group,and imaging lens group,which can greatly reduce the installation difficulty.During optimization,the angle between the edge rays and the normal lines of each lens surface is limited to more than 3° for reducing the stray light that is not ideally reflected by the surface of each lens of the beam expanding collimator group(Fig.4).The peak valley(PV)and root mean square(RMS)values of wavefront difference of each system are better than 0.01λ and 0.002λ respectively(Fig.5),with the tolerances of the system analyzed.A φ100 mm experimental system is built,and the coherent noise of the system in the ring light source mode is significantly suppressed compared with the point light source mode(Fig.6).The ITF curve of the φ100 mm experimental system is poor(Fig.7).After replacing the small-caliber imaging lens group with a large-caliber lens with worse wavefront quality,the ITF curve of the φ100 mm experimental system has been significantly improved(Fig.8),and then the reason of this phenomenon is analyzed.In the design of the φ100 mm and φ810 mm systems with the detection ability of intermediate frequency surface shape error,the interference path and imaging path are optimized at the same time.The PV of each interference path is better than 0.01λ,and the RMS of the wavefront difference is better than 0.002λ.The modulation transfer function values of each imaging path at corresponding spatial frequencies are all higher than 0.67(Figs.10 and 11),and the tolerances of the system are analyzed.Conclusions Two sets of ring light source Fizeau interference systems with diameters of φ100 mm and φ810 mm are designed.The axicon is employed to produce a real ring light source.The two systems adopt the design idea of re-using parts of the lens group,which can reduce the difficulty in φ810 mm system installation.In optimization,the idea of a"small aberration complement"is adopted to reduce the tolerance sensitivity of the lens surface.The φ100 mm experimental system has a sound coherent noise suppression effect,but the ITF of the system decreases seriously in the middle-frequency band.The experiment indicates that some light reflected by the step plate has a large deviation from the normal light path and cannot enter the imaging lens group.The reason for this phenomenon is that diffraction occurs at the step of the step plate,and this part of the light will form a certain aperture angle and enter the φ100 mm experimental system.In the system,the first surface of the imaging lens group becomes the aperture stop due to its small aperture.Most of the diffracted light of the step plate is blocked to result in a significant decrease in the ITF of the system.Therefore,based on the original design,the interference path and imaging path of the interference system can be optimized simultaneously by setting a reasonable stop position and setting a paraxial plane on the camera sensor and the measured surface of the interference path.Finally,the ring light source Fizeau interference system able to detect the surface shape error of the intermediate frequency is designed.

optical designring light sourceinstrument transfer functionre-using part of lens groupinterference optical path and imaging optical path

文豪东、刘东、沈亦兵、徐兆锐、彭韶婧、白剑

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浙江大学极端光学技术与仪器全国重点实验室,浙江杭州 310058

浙江大学光电科学与工程学院,浙江杭州 310027

浙江大学杭州国际科创中心,浙江 杭州 311215

光学设计 环形光源 仪器传递函数 复用镜组 干涉光路与成像光路

2024

光学学报
中国光学学会 中国科学院上海光学精密机械研究所

光学学报

CSTPCD北大核心
影响因子:1.931
ISSN:0253-2239
年,卷(期):2024.44(13)
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