概述 fU\k?'x_ ASY查看倾斜数据 d m/-} MC PLOT预估公差Monte-Carlo分析 Vu_7uSp,) W)G2Cs?p
bW,BhUb,| 设置工作目录 LZ=wz.'u 选择Dbook工作目录 jV(xYA3
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T%;k% 参考Donald Dilworth《Lens Design Automatic and quasi-autonomous computational methods and techniques》第28章 'Qp&,xK 9b"}CEw
~Hp#6+ 初始透镜 y\r^\ S9% p 02nd.R6 点击
打开C28M1,点击
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%eDFZ 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 ^VM"!O;h{
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tkm~KLWV&7 准备Monte-Carlo分析 B` t6H 在Command Window中输入LM MCFILE 'PmHBQvt& MCFILE是调整MACro,是Monte-Carlo分析的一部分 XZUB*P}]D 点击
运行MCFIlE y{&{=1# 点击
打开C28M2.MAC,点击
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+Tgy,oD0 有透镜都有楔角 YG}p$\R 在Command Window中输入GET 5 (FjsN5 在C28M2中注释掉TEST,更改SAMPLES 1为SAMPLES 100 Kd AR)EU> 点击
运行C28M2 .>AFf9P 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。 /Gh
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ur~Tql n##w[7B* 图像质量直方图 +Zty}fe $h|I7` 在Command Window中输入MC PLOT nkr,
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gw ASY查看倾斜数据 ?=|)n% 在C28M2中取消注释TEST,并在TEST前加入命令WEDGES CLOCK,点击
运行C28M2 ^)%wq@Hi 在Command Window中输入ASY !)51v {
E``!-W |aOnV,} 表面 1,5,7,9 和 12 已经被分配了组倾斜 '%eaK_+7 U#FJ8CD&u
:`Zl\!]E`o 增加伽马倾斜变量 -67f33 更改MCFILE.MAC为 mXN1b! PANT Ekg N6S`} VY 14 TH Rm[rQ}: VY 5 GPG ! Vary group gamma tilt on surfaces 5, 7, 9, and 12 (but not surface 1). ,Rr&. VY 7 GPG b/D9P~cE VY 9 GPG NZw[.s>n
VY 12 GPG 9cw4tqTm END j.yr5% DY+8m8!4H
Do[ F+Y AANT B#Oc8`1Y M 0 1 A P YA ! Control the boresight error this way. +=29y@c M 0 1 A P XA ?XTg%U
GSR .5 10 5 M 0 0 0 F ! Correct over the full pupil since the lens no longer has |]]pHC_/W GNR .5 2 3 M .7 0 0 F ! bilateral symmetry. ke;*uS GNR .5 1 3 M 1 0 0 F |Z^c#R GNR .5 2 3 M -.7 0 0 F ! For the same reason we also control the negative field. @gl%A&a GNR .5 1 3 M -1 0 0 F 7]HIE]# END _>:=<xyOq SYNOPSYS 10 q%=7<( w MC RGPU~L ;Cp/2A}Xx
\ /X!tlwxh 图像质量直方图 U~zN*2- 在Command Window中输入GET 5 xx`8>2T#e 在C28M2中注释掉TEST 7gR; 点击
运行C28M2 iR}i42Cu 在Command Window中输入MC PLOT iHG:W wM &
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|yl0}.() 更改MCFILE +EB,7<5< 在MCFILE.MAC中的命令SYNOPSYS 10和MC之间添加如下命令 G]3ML)l Z1 = XA IN COLOR 1 ! Get the actual X coordinate of the chief ray in color 1. ,aj+mlZd2 RMS 1 0 555 ! Run the RMS command, which also finds the centroid. GzZ|T7fm Z2 = FILE 4 ! This is the X-centroid location, relative to the chief ray, B6!<@*BI Z3 = FILE 5 ! and this is the Y. Drq{)#7 Z4 = YA IN COLOR 1 ! Also get the actual Y coordinate. u>i+R"hi" Z5 = XA IN COLOR 3 ! Do the same thing in color 3. '>WuukC RMS 3 0 555 Bc"}nSjH Z6 = FILE 4 O t4+VbB6 Z7 = FILE 5 X=c
,`&^ Z8 = YA IN COLOR 3 LXEu^F~{u# = SQRT((Z1 + Z2 - Z5 - Z6)**2 + (Z3 + Z4 - Z7 - Z8)**2) ! The separation. !&:W1Jkp( Z9 = FILE 1 ! Load it into variable Z9, and tell MC I9j+x]) MC IZ9 "RedCen-BlueCen" ! to gather the statistics and plot Z9 with this label. Ai_|) #/sE{jm
/dvnQW4}8 G|Yp<W%o 调整参数直方图 Vi-!E 在Command Window中输入MC PLOT uc (yos
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DBh/V#* D 总结 d~f0]O 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。 hw.demD %m\G'hY2
xbH!:R; 感谢 f!kdcr=/"
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