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概述 lb5Y$ZC ASY查看倾斜数据 PmyS6a@ MC PLOT预估公差Monte-Carlo分析 ~ z* mza1Q~< {^>m3 设置工作目录 :M9'wg 选择Dbook工作目录 -MOPm]iA ;({&C34a ]=of=T: 参考Donald Dilworth《Lens Design Automatic and quasi-autonomous computational methods and techniques》第28章 'W usEME 1BwCJ7?8 +u'
?VBv 初始透镜 %5 0}oD@ , .uu/qV}w 点击 打开C28M1,点击 HiCNs;t 此 MACro 将镜头输出并将副本存储在透镜库位置 5,然后创建一个 BTOL 公差分析 GiJ|5" ~b/lr 3&_O\nD _JOrGVmD o1YX^-<[F 准备Monte-Carlo分析 {\jh?P| 在Command Window中输入LM MCFILE VI0^Zq!6R MCFILE是调整MACro,是Monte-Carlo分析的一部分 G<OC99;8 点击 运行MCFIlE "{105&c\ 点击 打开C28M2.MAC,点击 FFb`4. [
\ LA 0RAmwfXm 有透镜都有楔角 SY>i@s+ML 在Command Window中输入GET 5 gN1b?_g 在C28M2中注释掉TEST,更改SAMPLES 1为SAMPLES 100 )a.Y$![ 点击 运行C28M2 _Sy-&}c+
+ 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。 Z0g3> iItM _O2},9L n !ccKbw)J# {[hH:
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zbt\C s$css{(ek 图像质量直方图 z(d@!Cd &$t BD@7 在Command Window中输入MC PLOT K@Q_q/(%; ZQ9!k*
^ 3P~I'FQ /~NsHStn rCi7q]_ _fha9` ASY查看倾斜数据 l-xKfp` 在C28M2中取消注释TEST,并在TEST前加入命令WEDGES CLOCK,点击 运行C28M2 iM+K&\{_h 在Command Window中输入ASY H|k!5W^ <DP_`[+C #Mw|h^Wm 表面 1,5,7,9 和 12 已经被分配了组倾斜 $,4;_4t E</UmM+ R Vd~{SS2> 增加伽马倾斜变量 S`gUSYS"w 更改MCFILE.MAC为 L ?g|: PANT k v1q\ VY 14 TH |ybW VY 5 GPG ! Vary group gamma tilt on surfaces 5, 7, 9, and 12 (but not surface 1). *CZvi0& VY 7 GPG EKoAIC*?p VY 9 GPG #3vq+mcn VY 12 GPG a5ZU"6Hi END 4wh_iO 8Kt_irD {Ak{
ct\t AANT {I+ M 0 1 A P YA ! Control the boresight error this way. n_\VG[f M 0 1 A P XA rq?:I:0 GSR .5 10 5 M 0 0 0 F ! Correct over the full pupil since the lens no longer has i <0H W GNR .5 2 3 M .7 0 0 F ! bilateral symmetry. J/S 47J~ GNR .5 1 3 M 1 0 0 F xO)vn\uJ GNR .5 2 3 M -.7 0 0 F ! For the same reason we also control the negative field. jjbBv~vs GNR .5 1 3 M -1 0 0 F /Y@^B,6\ END H6(kxpOI\ SYNOPSYS 10 ^N}zePy0 MC g3Q]W(F%$ qawb9Iud0 D,%R[F?5O 图像质量直方图 "@U9'rKx 在Command Window中输入GET 5 =KqcWN3k 在C28M2中注释掉TEST x'kwk 点击 运行C28M2 .4Ob?ZS( 在Command Window中输入MC PLOT S'M=P_-7 wJ@8-H 8} wEL$QOu$ WqP>cl2Lm maQE Bi, 更改MCFILE 6}^0/76^, 在MCFILE.MAC中的命令SYNOPSYS 10和MC之间添加如下命令 rB|Mp!g%@ Z1 = XA IN COLOR 1 ! Get the actual X coordinate of the chief ray in color 1. ^{&Vv(~!Q RMS 1 0 555 ! Run the RMS command, which also finds the centroid. RaT(^b( Z2 = FILE 4 ! This is the X-centroid location, relative to the chief ray, Gc2sY 0 Z3 = FILE 5 ! and this is the Y. ._@Scd Z4 = YA IN COLOR 1 ! Also get the actual Y coordinate. #k2&2W=x Z5 = XA IN COLOR 3 ! Do the same thing in color 3. %}jwuNGA RMS 3 0 555 aiVd^( Z6 = FILE 4 7NC"}JB& Z7 = FILE 5 }@MOkj Z8 = YA IN COLOR 3 U ^1Xc#Ff = SQRT((Z1 + Z2 - Z5 - Z6)**2 + (Z3 + Z4 - Z7 - Z8)**2) ! The separation. p'UY Ht Z9 = FILE 1 ! Load it into variable Z9, and tell MC & V:q}Q MC IZ9 "RedCen-BlueCen" ! to gather the statistics and plot Z9 with this label. OJ8 ac6cJ ,ButNBv {[WEA^C~Q la#f,C3_ 调整参数直方图 <,p|3p3 在Command Window中输入MC PLOT ].53t"* 2%4dA$H#4w mqgA f`'? 2 Eyi^N0 总结 xLX< |