概述 [L`ZE*z ASY查看倾斜数据 :a8 YV!X MC PLOT预估公差Monte-Carlo分析 L$'[5"ma
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|yyO q 参考Donald Dilworth《Lens Design Automatic and quasi-autonomous computational methods and techniques》第28章 "q}FPJ^l_N CO-_ea U(
4${jr\q] 初始透镜 u$%t)2+$4 hPq%Lc 点击打开C28M1,点击 f~E*Zz`; 此 MACro 将镜头输出并将副本存储在透镜库位置 5,然后创建一个 BTOL 公差分析 zX5!vaEv tH=P6vY
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}:: S0l 准备Monte-Carlo分析 "G>3QL+O| 在Command Window中输入LM MCFILE %0#1t 5g MCFILE是调整MACro,是Monte-Carlo分析的一部分
F4=}}kU 点击运行MCFIlE U$oduY# 点击 打开C28M2.MAC,点击 jq'!UN{ l4T7'U>`
80A.<=(=. 有透镜都有楔角 &`b
"a! 在Command Window中输入GET 5 gTRF^knrY 在C28M2中注释掉TEST,更改SAMPLES 1为SAMPLES 100 Z*G(5SqUh" 点击运行C28M2 imQURC 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。 6y%0`! E{6~oZ#L
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JtK6t 图像质量直方图 ]weoTn: zy*/T>{# 在Command Window中输入MC PLOT hdTzCfeZ5@ S9HwIH\m
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,C3,TkA] @aJ!PV'ms ASY查看倾斜数据 VDTcR 在C28M2中取消注释TEST,并在TEST前加入命令WEDGES CLOCK,点击运行C28M2 &.TTJsKG h 在Command Window中输入ASY 12Y W0I#\b18 Z{?G.L*/ 表面 1,5,7,9 和 12 已经被分配了组倾斜 o\vBOp?hj "
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vn/.}GkpU 增加伽马倾斜变量 ">?vir^ 更改MCFILE.MAC为 <nEi<iAY>U PANT [w ;kkMJAy VY 14 TH @{Gncy| VY 5 GPG ! Vary group gamma tilt on surfaces 5, 7, 9, and 12 (but not surface 1). 3Hf0MAt VY 7 GPG g^zs,4pPU< VY 9 GPG &^4++ VY 12 GPG CdL< *AH END 1}~(Yj@f% =B.F;40
vv26I AANT ]qhPd_$?D' M 0 1 A P YA ! Control the boresight error this way. I-OJVZ( V M 0 1 A P XA ;#Q%j%J GSR .5 10 5 M 0 0 0 F ! Correct over the full pupil since the lens no longer has LR"9D GNR .5 2 3 M .7 0 0 F ! bilateral symmetry. ws4cF
N9P? GNR .5 1 3 M 1 0 0 F arf8xqR-U] GNR .5 2 3 M -.7 0 0 F ! For the same reason we also control the negative field. eYx Kp!f GNR .5 1 3 M -1 0 0 F [$[:"N_ END +{/ SYNOPSYS 10 7g_]mG[6 MC I!^O)4QRx 3Gkv4,w<
vTn}*d.K= 图像质量直方图 EYA,hc 在Command Window中输入GET 5 qx%}knB 在C28M2中注释掉TEST $\9~)Rq6 点击运行C28M2 hpU2 在Command Window中输入MC PLOT &c1A*Pl/:G R##~*>#
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!>:?rSg* 更改MCFILE 23gPbtq/ 在MCFILE.MAC中的命令SYNOPSYS 10和MC之间添加如下命令 '(/7[tJ Z1 = XA IN COLOR 1 ! Get the actual X coordinate of the chief ray in color 1.
O#I1V K RMS 1 0 555 ! Run the RMS command, which also finds the centroid. z?35=%~w Z2 = FILE 4 ! This is the X-centroid location, relative to the chief ray, d^`?ed\1 Z3 = FILE 5 ! and this is the Y. !W?gR.0$= Z4 = YA IN COLOR 1 ! Also get the actual Y coordinate. -lv)tHs< Z5 = XA IN COLOR 3 ! Do the same thing in color 3. 5 (A5Y-B RMS 3 0 555 JfPD}w Z6 = FILE 4 P9 Z}H(?C Z7 = FILE 5 0V?F'<qy Z8 = YA IN COLOR 3 6^DR0sO = SQRT((Z1 + Z2 - Z5 - Z6)**2 + (Z3 + Z4 - Z7 - Z8)**2) ! The separation. 64
5z#_}C$ Z9 = FILE 1 ! Load it into variable Z9, and tell MC {p,]oOq\ MC IZ9 "RedCen-BlueCen" ! to gather the statistics and plot Z9 with this label. Dl}$pN Dwzg/F(
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qw --DoB=5%8 调整参数直方图 A~mum+[5 在Command Window中输入MC PLOT G+F:99A =z8f]/k*>
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GAAm0; 总结 Nv"EV;$ 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。 ,UuH}E B-r0"MX&
ccL~#c0P7 感谢 ZWS`\M
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support@asdoptics.com wm^J;<T[ wiBVuj# [ 此帖被optics1210在2019-04-08 10:22重新编辑 ]