光电工程
光電工程
광전공정
OPTO-ELECTRONIC ENGINEERING
2014年
10期
55-62
,共8页
王金%鲜浩%王胜千%周龙峰%李斌
王金%鮮浩%王勝韆%週龍峰%李斌
왕금%선호%왕성천%주룡봉%리빈
拼接式望远镜%点扩散函数%斯特列尔比%成像质量
拼接式望遠鏡%點擴散函數%斯特列爾比%成像質量
병접식망원경%점확산함수%사특렬이비%성상질량
segmented telescope%point-spread-function%Strehl ratio%image quality
通过理论及数值仿真分析拼接式望远镜中子镜的平移误差、倾斜误差和子镜间隙对系统成像质量的影响。理论推导了存在不同误差时拼接式望远镜点扩散函数(PSF)及远场光斑斯特列尔比(S.R,用RS.R表示)的表达式,建立了三种误差对拼接式望远镜PSF和远场光斑RS.R的影响的仿真模型,分析了三种误差分别对拼接式望远镜成像质量的影响。分析结果表明:当子镜存在平移误差时,拼接式望远镜成像质量随着子镜平移误差标准差δ增加逐渐变差,当δ<λ/20时,拼接式望远镜远场光斑RS.R>0.9;当子镜存在倾斜误时,拼接式望远镜成像质量随着波前相位均方差(RMS,用erms表示)增加逐渐变差,当erms<0.3 rad时,拼接式望远镜远场光斑RS.R>0.9;当子镜间存在间隙时,拼接式望远镜成像质量随着间隙因子w增大逐渐变差,当w<0.025时,拼接望远镜远场光斑RS.R>0.9。
通過理論及數值倣真分析拼接式望遠鏡中子鏡的平移誤差、傾斜誤差和子鏡間隙對繫統成像質量的影響。理論推導瞭存在不同誤差時拼接式望遠鏡點擴散函數(PSF)及遠場光斑斯特列爾比(S.R,用RS.R錶示)的錶達式,建立瞭三種誤差對拼接式望遠鏡PSF和遠場光斑RS.R的影響的倣真模型,分析瞭三種誤差分彆對拼接式望遠鏡成像質量的影響。分析結果錶明:噹子鏡存在平移誤差時,拼接式望遠鏡成像質量隨著子鏡平移誤差標準差δ增加逐漸變差,噹δ<λ/20時,拼接式望遠鏡遠場光斑RS.R>0.9;噹子鏡存在傾斜誤時,拼接式望遠鏡成像質量隨著波前相位均方差(RMS,用erms錶示)增加逐漸變差,噹erms<0.3 rad時,拼接式望遠鏡遠場光斑RS.R>0.9;噹子鏡間存在間隙時,拼接式望遠鏡成像質量隨著間隙因子w增大逐漸變差,噹w<0.025時,拼接望遠鏡遠場光斑RS.R>0.9。
통과이론급수치방진분석병접식망원경중자경적평이오차、경사오차화자경간극대계통성상질량적영향。이론추도료존재불동오차시병접식망원경점확산함수(PSF)급원장광반사특렬이비(S.R,용RS.R표시)적표체식,건립료삼충오차대병접식망원경PSF화원장광반RS.R적영향적방진모형,분석료삼충오차분별대병접식망원경성상질량적영향。분석결과표명:당자경존재평이오차시,병접식망원경성상질량수착자경평이오차표준차δ증가축점변차,당δ<λ/20시,병접식망원경원장광반RS.R>0.9;당자경존재경사오시,병접식망원경성상질량수착파전상위균방차(RMS,용erms표시)증가축점변차,당erms<0.3 rad시,병접식망원경원장광반RS.R>0.9;당자경간존재간극시,병접식망원경성상질량수착간극인자w증대축점변차,당w<0.025시,병접망원경원장광반RS.R>0.9。
The impact of segmented telescope piston error, tip-tilt error and gap on image quality by theoretical and numerical simulation was analyzed. Different error segmented telescope Point-spread-function (PSF) and the far-field spot Strehl Ratio (S.R) expression were derived theoretically. Then, set up simulation model about three kinds of error effect on segmented telescope PSF and far-field spot S.R, and analyzed three kinds of error influence on imaging quality of splicing telescope. Analysis results show that:when the segmented mirror exist piston error, segmented telescope image quality with piston error standard deviationδincreasing gradually becomes poor;whenδ<λ/20 segmented telescope, the far field spot RS.R>0.9;when the segmented mirror exist tip-tilt error, the segmented telescope imaging quality with the wavefront phase RMS increases gradually worse, when eRMS<0.3 rad, the far-field spot of the segmented telescope RS.R>0.9; when the segmented mirror exist gap, its imaging quality with the gap factor w increases gradually becomes poor, and when w<0.025, a segmented telescope far-field spot RS.R>0.9.