概述 =6Ihk ASY查看倾斜数据 ]]J2#mN:n MC PLOT预估公差Monte-Carlo分析 _ p<s! ,GA2K .:#
S1.w^Ccy 设置工作目录 kTL{?- 选择Dbook工作目录 _t _X` 
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%tT &/F 参考Donald Dilworth《Lens Design Automatic and quasi-autonomous computational methods and techniques》第28章 6V
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a= +qR:wT 初始透镜 }E+#*R3auB ` B}( Ln 点击
打开C28M1，点击
%XM wjBM 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 lED-Jo2 
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\cP\I5IW:s 准备Monte-Carlo分析 I9-vV>:z 在Command Window中输入LM MCFILE 5zWxI]4d\ MCFILE是调整MACro，是Monte-Carlo分析的一部分 Z?kLAhy! 点击运行MCFIlE hiZE8?0+~N 点击 打开C28M2.MAC，点击 tIR"y:U+ 5*l~7R
7aUk?Hf 有透镜都有楔角 P,^`|\#7 在Command Window中输入GET 5 l *T> 9yC 在C28M2中注释掉TEST，更改SAMPLES 1为SAMPLES 100 {f3&s4xj= 点击运行C28M2 BFmd`#{ l 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。 uO%G,b 
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wg\*Ff Qn +YVnA?r? 图像质量直方图 ^A S*X2y ^R',P(@oL 在Command Window中输入MC PLOT |!NKKvf 
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c+|,q m +`O8cHx ASY查看倾斜数据 pCS2sq8RC 在C28M2中取消注释TEST，并在TEST前加入命令WEDGES CLOCK，点击运行C28M2 !$P +hX` 在Command Window中输入ASY RG1~)5AL~Y 
#K:|@d ]y= ff6 Q 表面 1,5,7,9 和 12 已经被分配了组倾斜 PYX]ld.E !g{9]"Z1T
` KBgVhS> 增加伽马倾斜变量 bI/d(Q%#< 更改MCFILE.MAC为 ~?TG SD@( PANT H. U wM VY 14 TH oac e!si VY 5 GPG ! Vary group gamma tilt on surfaces 5, 7, 9, and 12 (but not surface 1). T|dQY~n~ VY 7 GPG !mLQdkTE VY 9 GPG F[uy'~;@ VY 12 GPG 9N5ptdP.d END SA@M J>Z R
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C,T9x m AANT {a -bew M 0 1 A P YA ! Control the boresight error this way. =@$G3DM M 0 1 A P XA 7A'd55I4 GSR .5 10 5 M 0 0 0 F ! Correct over the full pupil since the lens no longer has fZ!fwg$ GNR .5 2 3 M .7 0 0 F ! bilateral symmetry. tr3Rn :0] GNR .5 1 3 M 1 0 0 F Bwv@D4bii GNR .5 2 3 M -.7 0 0 F ! For the same reason we also control the negative field. ma@3 BiM GNR .5 1 3 M -1 0 0 F 2]W"sT[ END }`M53>C,gQ SYNOPSYS 10 ns`|G;1vv MC Ln/6]CMl U%o h ?g
3";Rw9 图像质量直方图 s *$Re)}S 在Command Window中输入GET 5 Du@?j7&l=$ 在C28M2中注释掉TEST
j. UQLi&` 点击运行C28M2 ? ->:,I=<~ 在Command Window中输入MC PLOT t}r`~ AEa! 
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:.KN;+tP 更改MCFILE ^wesuW@= 在MCFILE.MAC中的命令SYNOPSYS 10和MC之间添加如下命令 `; Qw/xl_N Z1 = XA IN COLOR 1 ! Get the actual X coordinate of the chief ray in color 1. {B^V_T X2 RMS 1 0 555 ! Run the RMS command, which also finds the centroid. : C6 Z2 = FILE 4 ! This is the X-centroid location, relative to the chief ray, "[(& $ I Z3 = FILE 5 ! and this is the Y. xszGao' Z4 = YA IN COLOR 1 ! Also get the actual Y coordinate. 7d &_5Tj: Z5 = XA IN COLOR 3 ! Do the same thing in color 3. {;.q?mj RMS 3 0 555 h'T n&2r6 Z6 = FILE 4 O 1T JJ8 Z7 = FILE 5 +oKp>- Z8 = YA IN COLOR 3 D5]4(]k& = SQRT((Z1 + Z2 - Z5 - Z6)**2 + (Z3 + Z4 - Z7 - Z8)**2) ! The separation. ZI"L\q=|0# Z9 = FILE 1 ! Load it into variable Z9, and tell MC z"/Mva3| MC IZ9 "RedCen-BlueCen" ! to gather the statistics and plot Z9 with this label. %JmRJpCvR +-_71rJc.
m# #( uSh x:'M\c 7 调整参数直方图 cI}qMc 在Command Window中输入MC PLOT `m2e
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c)H ( w 总结 .yz-o\,gF% 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。 Tj
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b=:$~N@ Y 感谢 G dZ_
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