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作 者:张晓杰 魏炜[1,2,3] 侯永辉 张勇[1,2] 季杭馨[1,2] 李晓飞[1,2] 陆启帅[1,2] 黄康[1,2,3] 刘玉瑶 Zhang Xiaojie;Wei Wei;Hou Yonghui;Zhang Yong;Ji Hangxin;Li Xiaofei;Lu Qishuai;Huang Kang;Liu Yuyao(National Astronomical Observatories/Nanjing Institute of Astronomical Optics&Technology,Chinese Academy of Sciences,Nanjing 210042,China;CAS Key Laboratory of Astronomical Optics&Technology,Nanjing Institute of Astronomical Optics&Technology,Nanjing 210042,China;University of Chinese Academy of Sciences,Beijing 100049,China)
机构地区:[1]中国科学院国家天文台南京天文光学技术研究所,江苏南京210042 [2]中国科学院天文光学技术重点实验室(南京天文光学技术研究所),江苏南京210042 [3]中国科学院大学,北京100049
出 处:《红外与激光工程》2022年第12期314-322,共9页Infrared and Laser Engineering
基 金:国家自然科学基金(12173061);国家重大科研仪器研制项目(12027802)。
摘 要:研究表明,当温度产生一定变化时,会导致大天区面积多目标光纤光谱天文望远镜(LAMOST)光谱仪的内部器件产生热诱导变形,引起CCD靶面上的图像离焦模糊,降低了天文数据测量精度,也大大增加了16台光谱仪的日常维护难度。基于LAMOST运行前拍摄的定标灯谱数据,提出了一种基于多目标图像清晰度评价的离焦诊断方法。该方法通过对不同离焦量下的定标灯谱图像进行分析,提取了一定数量的光斑的半高全宽(FWHM)及其总体分布情况,建立多目标图像清晰度与系统离焦量之间的离焦函数模型,实现对LAMOST成像像质的离焦诊断,为后续智能化主动补偿技术的实现提供了技术支撑。介绍了LAMOST光谱仪的工作原理及结构,给出了光谱仪对调焦精度的需求;详细介绍了光斑FWHM值的测量原理与多目标图像清晰度评价函数的构建方法。与传统图像清晰度评价函数的对比结果显示,文中方法具有更高的清晰度对比率与精度,对定标灯谱图像的离焦诊断误差在10μm以内,有效降低了人为局部诊断带来的误差,提高了16台光谱仪系统一致性,有望提高LAMOST日常运行效率与光谱仪的长期稳定性。The research demonstrates that when the temperature changes a lot,the internal components of the large sky area multi-object fiber spectroscopic telescope(LAMOST)spectrographs will produce thermal-induced flexure,which will cause the image blurring of the CCD.Such image blurring reduces the measurement accuracy of astronomical data and greatly increases the difficulty of the daily maintenance of the 16 spectrographs.Therefore,a defocus diagnosis method for multi-object image definition evaluation is proposed based on the calibration lamp spectrum taken by LAMOST.By analyzing the spectrum image under the different defocusing amounts,the half-height full-width(FWHM)and its distribution of spots are obtained to establish the function model between the multi-target image definition and the defocusing amount of the system.It can realize the fast defocus diagnosis of the spectrum image quality of LAMOST and provide a reference for the realization of intelligent active compensation technology of LAMOST spectrograph.In this paper,the principle and structure of the LAMOST spectrograph are introduced,and the demand for the focusing precision of the spectrograph is given.And the measurement principle of FWHM value and the construction method of the multi-object image definition evaluation function are introduced in detail.Compared with the traditional image definition evaluation function,the results show that the proposed method has a higher definition ratio and accuracy.And the defocus diagnosis error of the spectral image is less than 10μm,which effectively reduces the error caused by artificial diagnosis and improves the consistency of the 16 spectrographs.This method can also improve the daily operation efficiency and long-term stability of the LAMOST spectrographs.
关 键 词:天文技术与方法 多目标图像清晰度评价 离焦函数模型 离焦诊断 像质校正
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