概述 <d8 Yk>R ASY查看倾斜数据 q>t#5Z81 MC PLOT预估公差Monte-Carlo分析 0`:0m/fsU *4]}_ .rG#
nPE{Gp) } 设置工作目录 fT Mn 选择Dbook工作目录 nwf(`=TC 
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A|7%j0T 参考Donald Dilworth《Lens Design Automatic and quasi-autonomous computational methods and techniques》第28章 |Y4c+6@_ }get e'I
`@RTfBB g 初始透镜 + JsMYv `f S$@{YI_ 点击
打开C28M1，点击
Ko: <@h 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 y2KR^/LN|Y 
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dSkM A 准备Monte-Carlo分析 p C^d-Ii 在Command Window中输入LM MCFILE MR }=tO MCFILE是调整MACro，是Monte-Carlo分析的一部分 I;FHjnn( 点击运行MCFIlE 50 8v:?^' 点击 打开C28M2.MAC，点击 DZ"'GQSg #A\@)wJ
$Y,y~4I 有透镜都有楔角 evjj~xkte 在Command Window中输入GET 5 kntYj}F( 在C28M2中注释掉TEST，更改SAMPLES 1为SAMPLES 100 9(6f:D 点击运行C28M2 [>
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VkFMr8@| >e>% AMzo[ 图像质量直方图 w {mw? 0 Y
\ Gx| 在Command Window中输入MC PLOT gWQ (B 
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KT[ZOtu ,R. rx oO ASY查看倾斜数据 6%it `A8} 在C28M2中取消注释TEST，并在TEST前加入命令WEDGES CLOCK，点击运行C28M2 zX lcu_rc 在Command Window中输入ASY -^+fZBU; 
;6 :9 EEd >v2/0>U 表面 1,5,7,9 和 12 已经被分配了组倾斜 ~y{_NgMo Jr5dw=B gw
,oykOda:| 增加伽马倾斜变量 t0,=U8]w 更改MCFILE.MAC为 F/ x2}' PANT DL`8qJ'mJs VY 14 TH A3)"+`&PUl VY 5 GPG ! Vary group gamma tilt on surfaces 5, 7, 9, and 12 (but not surface 1). /k8I6 VY 7 GPG 3^ [P VY 9 GPG _B>'07D0 VY 12 GPG wx^Det END eAmI~oku auga`*
T*:w1*: AANT ?VlGTMaS+ M 0 1 A P YA ! Control the boresight error this way. M287Z[ M 0 1 A P XA {n|ah{_p| GSR .5 10 5 M 0 0 0 F ! Correct over the full pupil since the lens no longer has VCfHm"'E8 GNR .5 2 3 M .7 0 0 F ! bilateral symmetry. yts@cd`$ GNR .5 1 3 M 1 0 0 F 793 15A GNR .5 2 3 M -.7 0 0 F ! For the same reason we also control the negative field. hr;^.a^ GNR .5 1 3 M -1 0 0 F )9 ^)t END "4\k1H"_ SYNOPSYS 10 EB|
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9dq"x[ 图像质量直方图 eZEk$W% 在Command Window中输入GET 5 ").gPmC 在C28M2中注释掉TEST Q7rBc
wm5 点击运行C28M2 0N^+d,Xt. 在Command Window中输入MC PLOT h;,1BpbM 
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i,h 30J 更改MCFILE aX`uF<c9 在MCFILE.MAC中的命令SYNOPSYS 10和MC之间添加如下命令 :`e#I/, Z1 = XA IN COLOR 1 ! Get the actual X coordinate of the chief ray in color 1. tPl 4'tW_ RMS 1 0 555 ! Run the RMS command, which also finds the centroid. vo f8bQ{& Z2 = FILE 4 ! This is the X-centroid location, relative to the chief ray, M^[;{p2uZ Z3 = FILE 5 ! and this is the Y. gu3iaM$W Z4 = YA IN COLOR 1 ! Also get the actual Y coordinate. Ym 1 vq= Z5 = XA IN COLOR 3 ! Do the same thing in color 3. ;Ax-f04gG RMS 3 0 555 x(._?5 Z6 = FILE 4 yfK}1mx)j Z7 = FILE 5 X8VBs#tLE Z8 = YA IN COLOR 3 0S^&A?$= = SQRT((Z1 + Z2 - Z5 - Z6)**2 + (Z3 + Z4 - Z7 - Z8)**2) ! The separation. D# UuIZ Z9 = FILE 1 ! Load it into variable Z9, and tell MC g!R7C Rt% MC IZ9 "RedCen-BlueCen" ! to gather the statistics and plot Z9 with this label. \?;
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M ]R_R` X? 调整参数直方图 R| n 在Command Window中输入MC PLOT "aOs#4N 
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i}VF$XN 总结 JcWp 14~e 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。 ]:OrGD" /QY F|%7!
}3^m>i*8 感谢 pASX-rb
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MQq3 0n{.96r0R [ 此帖被optics1210在2019-04-08 10:22重新编辑 ]
