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tOjM ASY查看倾斜数据 ICUI0/J MC PLOT预估公差Monte-Carlo分析 54%h)dLDy J4jL%5t
1VB{dgr 设置工作目录 ju(QSZ|; 选择Dbook工作目录 B^BbA-I m ?jF:]^
zN>tSdNkI- 参考Donald Dilworth《Lens Design Automatic and quasi-autonomous computational methods and techniques》第28章 *
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9`5qVM1O{ 初始透镜 Pql;5
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Uc5BNk7<= 点击打开C28M1,点击 b0[H{q-z{X 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 v:u=.by99 GKf%dKL
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YHI@Cj 准备Monte-Carlo分析 8&++S> < 在Command Window中输入LM MCFILE XXC(R MCFILE是调整MACro,是Monte-Carlo分析的一部分 z?Qt%1q 点击运行MCFIlE
ui1h M 点击 打开C28M2.MAC,点击 pR7 D3Q:^7 jfsbvak
Xv?'*2J 有透镜都有楔角 'L ]k\GO 在Command Window中输入GET 5 2qDVAq^@ 在C28M2中注释掉TEST,更改SAMPLES 1为SAMPLES 100 A9ru]|? 点击运行C28M2 0uS6F8x@ 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。 7A4_b8 n]snD1?KX
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btv.M qb>mUS 图像质量直方图 nVv=smVOt ec"+Il 在Command Window中输入MC PLOT HbQ+:B] 1|3{.Ed
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"D.`:9sk0 D|X@aUp8} ASY查看倾斜数据 F;<cG`|Rx 在C28M2中取消注释TEST,并在TEST前加入命令WEDGES CLOCK,点击运行C28M2 mNnt9F3Eq 在Command Window中输入ASY GB`
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u[b 表面 1,5,7,9 和 12 已经被分配了组倾斜 E:S (v ky|Py
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/*i 增加伽马倾斜变量 Yp8GW1@ 更改MCFILE.MAC为 J?84WS PANT 0Nq6>^
% VY 14 TH Q*l_QnfG VY 5 GPG ! Vary group gamma tilt on surfaces 5, 7, 9, and 12 (but not surface 1). ,[|4{qli\ VY 7 GPG EmubpUS; VY 9 GPG +N>&b% VY 12 GPG zIh`Vw ,t0 END <jHo2U8/"s o%$'-N
rT{+ h}vO AANT Tq`rc"&7u M 0 1 A P YA ! Control the boresight error this way. _!?iiO M 0 1 A P XA Uh8c!CA8:\ GSR .5 10 5 M 0 0 0 F ! Correct over the full pupil since the lens no longer has e BxOa GNR .5 2 3 M .7 0 0 F ! bilateral symmetry. ?(P3ZTk?. GNR .5 1 3 M 1 0 0 F MPF;P&6 GNR .5 2 3 M -.7 0 0 F ! For the same reason we also control the negative field. = ,^eQZR: GNR .5 1 3 M -1 0 0 F y%=t((.Z END pG(%yIiAi SYNOPSYS 10 ;&MI
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cuW&X9\m, 图像质量直方图 C6cEt5 在Command Window中输入GET 5 NY9\a[[^[8 在C28M2中注释掉TEST \oc* 点击运行C28M2 k^v P|*eu 在Command Window中输入MC PLOT Fi_JF; j1U,X
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t/L:Y=7w 更改MCFILE s6| S#
在MCFILE.MAC中的命令SYNOPSYS 10和MC之间添加如下命令 ^YwTO/Q| Z1 = XA IN COLOR 1 ! Get the actual X coordinate of the chief ray in color 1. tp3]?@0 RMS 1 0 555 ! Run the RMS command, which also finds the centroid. K84VeAe Z2 = FILE 4 ! This is the X-centroid location, relative to the chief ray, j`pX2S Z3 = FILE 5 ! and this is the Y. 1Xj>kE: Z4 = YA IN COLOR 1 ! Also get the actual Y coordinate. K|g+Wt^tQ Z5 = XA IN COLOR 3 ! Do the same thing in color 3. UjrML RMS 3 0 555 sGs_w:Hn Z6 = FILE 4 M
h5>@-fEE Z7 = FILE 5 ,ThN/GkSC Z8 = YA IN COLOR 3 $m)[> C = SQRT((Z1 + Z2 - Z5 - Z6)**2 + (Z3 + Z4 - Z7 - Z8)**2) ! The separation. C!Oz'~l Z9 = FILE 1 ! Load it into variable Z9, and tell MC zxffjz,Fe: MC IZ9 "RedCen-BlueCen" ! to gather the statistics and plot Z9 with this label. k1)=xv#S -"Hy%wE
V'jvI `$N()P 调整参数直方图 ^B`*4 在Command Window中输入MC PLOT uF89B-t :]g>8sWL
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@K:TGo,%I 总结 @+P7BE} 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。 3}lT"K c. ;}e:)s
yE4X6 感谢 _bm8m4Lk
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support@asdoptics.com Sdn4y(&TP ltH?Ew<] [ 此帖被optics1210在2019-04-08 10:22重新编辑 ]