概述 bo\ bs1 ASY查看倾斜数据 tm~9X FQ< MC PLOT预估公差Monte-Carlo分析 t]h_w7!U G"/;Cq=t
Z>g72I%X 设置工作目录 V'kBF2} 选择Dbook工作目录 |5^
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y\??cjWb] 参考Donald Dilworth《Lens Design Automatic and quasi-autonomous computational methods and techniques》第28章 W`[VLi}fe 2u]G]: ml
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初始透镜 f) Qln[/ p/{%%30ke 点击打开C28M1，点击 N foHQU <n 此 MACro 将镜头输出并将副本存储在透镜库位置 5，然后创建一个 BTOL 公差分析 " 9; j,OA>{-$
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z qA>eDx 准备Monte-Carlo分析 7J);{ &x9h 在Command Window中输入LM MCFILE z4YDngf=4 MCFILE是调整MACro，是Monte-Carlo分析的一部分 mnA_$W3~I 点击运行MCFIlE v?He]e' 点击 打开C28M2.MAC，点击 F$UL.`X
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1K/HVj+'. 有透镜都有楔角 f&vMv . 在Command Window中输入GET 5 5Ew( 0K[ 在C28M2中注释掉TEST，更改SAMPLES 1为SAMPLES 100 3eUi9_s+ 点击运行C28M2 ja9u?UbW 元件现在都有楔角误差，因此 PAD 显示不能像以前那样为透镜着色。 q]4h#?.-1v & b (*
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,a>Dv@$Y Z66Xj-o 图像质量直方图 |eRE'Wd0 T={!/y+ 在Command Window中输入MC PLOT vd%AV(]<LJ B 2NIV7
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a uihH")Mo ASY查看倾斜数据 eBa#Z1Z 在C28M2中取消注释TEST，并在TEST前加入命令WEDGES CLOCK，点击运行C28M2 ! >F70 在Command Window中输入ASY r 1HG$^ VP! 4Nob |OLXb+ 7X 表面 1,5,7,9 和 12 已经被分配了组倾斜 ;=joQWNDm XVN JK-B
{>km]CG 增加伽马倾斜变量 O1\4WG% 更改MCFILE.MAC为 <oXBkCi0r PANT Ys.GBSlHG VY 14 TH 1 V]ws}XW VY 5 GPG ! Vary group gamma tilt on surfaces 5, 7, 9, and 12 (but not surface 1). %f C kR`: VY 7 GPG 53hX%{3 VY 9 GPG r0nnmy]{d VY 12 GPG S0StC$$1 END /,S VG1 {_!,T%>+1
G+fo'ThG AANT vVMoCG"f M 0 1 A P YA ! Control the boresight error this way. qMEd
R;o M 0 1 A P XA ^W sgAyCB GSR .5 10 5 M 0 0 0 F ! Correct over the full pupil since the lens no longer has Y -8BL GNR .5 2 3 M .7 0 0 F ! bilateral symmetry. O)W+rmToI GNR .5 1 3 M 1 0 0 F kB?/ _a`] GNR .5 2 3 M -.7 0 0 F ! For the same reason we also control the negative field. <cZ/_+H%C GNR .5 1 3 M -1 0 0 F i+(>w'=m END sf$hsPC^ SYNOPSYS 10 P84YriLo MC [f:&aS+ 7(D)U)9h
/*;a6S8q 图像质量直方图 [ PN2^ 在Command Window中输入GET 5 T}{zh 在C28M2中注释掉TEST <}RD]Sc$1 点击运行C28M2 z#Qe$`4& 在Command Window中输入MC PLOT _<]0hC (Zx--2l c
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&3IkC(yD 更改MCFILE 0Sk~m4fj( 在MCFILE.MAC中的命令SYNOPSYS 10和MC之间添加如下命令 iOfO+3'Z_U Z1 = XA IN COLOR 1 ! Get the actual X coordinate of the chief ray in color 1. r MVcoO@3 RMS 1 0 555 ! Run the RMS command, which also finds the centroid. Xl1% c7r.1 Z2 = FILE 4 ! This is the X-centroid location, relative to the chief ray, `oe=K{aX Z3 = FILE 5 ! and this is the Y. ^O<' Qp,[: Z4 = YA IN COLOR 1 ! Also get the actual Y coordinate. 2u- J+ Z5 = XA IN COLOR 3 ! Do the same thing in color 3. gJp6ReZ# RMS 3 0 555 3{.]! Z6 = FILE 4 )-"<19eu Z7 = FILE 5 5s\;7> Z8 = YA IN COLOR 3 Wgs6}1b g = SQRT((Z1 + Z2 - Z5 - Z6)**2 + (Z3 + Z4 - Z7 - Z8)**2) ! The separation. j =U"t\{ Z9 = FILE 1 ! Load it into variable Z9, and tell MC 4S*ifl MC IZ9 "RedCen-BlueCen" ! to gather the statistics and plot Z9 with this label. &u^]YE{ |%5pzY e
/tG as ?7pn %_S 调整参数直方图 p2(ha3PW 在Command Window中输入MC PLOT gFuK/]gzI =\u,4
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G>:v1lde 总结 94O\M
RQ* 本例讲述了使用 BTOL 来计算八片透镜组的公差分析，然后查看通过时钟单元格中的透镜来补偿楔角误差的情况下的像质统计。 最后，我们将在镜头重新聚焦和时钟元件之后，检查一组 100 个镜头的横向色差的统计数据。 prt(xr4@ vN
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FO(QsR=\s 感谢 "5dk e^yk0
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