| optics1210 |
2019-04-03 10:59 |
SYNOPSYS 每天一例 - 元件时钟楔角误差的公差分析案例和像质误差的 AI 分析
概述 TR%?U/_4;r
ASY查看倾斜数据 ?xG #4P<C=
MC PLOT预估公差Monte-Carlo分析 /? J_7Lg
qmL!"ZRLF
xMuy[)b
设置工作目录 7N XT.E~2
选择Dbook工作目录 UNhD
[attachment=92287] -#Wc@\;
;hZ( 20
参考Donald Dilworth《Lens Design Automatic and quasi-autonomous computational methods and techniques》第28章 < )?&Jf>_
km|~DkJ\a`
XM=`(e
o
初始透镜 qK#* UR0%
UHCx}LGe
点击[attachment=92288]打开C28M1，点击[attachment=92289] f9\ 7v_
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 I'yhxymZ;
[attachment=92290] %
vP{C
Ic r'l$PE
f,uxo AS
T LV) mCZ
准备Monte-Carlo分析 XSD7~X/:
在Command Window中输入LM MCFILE H v
I N'
MCFILE是调整MACro，是Monte-Carlo分析的一部分 `iY)3Rq
点击[attachment=92289]运行MCFIlE tx.YW9xD
点击[attachment=92288] 打开C28M2.MAC，点击[attachment=92289] mC93
&0
Q,DumOq
$L`7 J$'^
有透镜都有楔角 /3c1{%B\
在Command Window中输入GET 5 zf S<X
在C28M2中注释掉TEST，更改SAMPLES 1为SAMPLES 100 u C}YKT>V7
点击[attachment=92289]运行C28M2 H R
V / A
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。 X F40;urm
[attachment=92295] <T&$1 m{
y1AS^'
SB F3\
4u&l@BUr
nh8h?&q|
图像质量直方图 r8>
q*0~s
3N JH"amk
在Command Window中输入MC PLOT L NE]#8ue
[attachment=92296] |Y99s)2&N
0GG;o[<
UU !I@
# K-Q/*
r ms&U)?
ASY查看倾斜数据 G.N3 R
在C28M2中取消注释TEST，并在TEST前加入命令WEDGES CLOCK，点击[attachment=92289]运行C28M2
m$c M+
在Command Window中输入ASY =o-q u^T^u
[attachment=92297] O4#zsr:"
md2kZ.5u
表面 1,5,7,9 和 12 已经被分配了组倾斜 < 37vWK 1+
1|]-F;b
+u
Lu.-N
增加伽马倾斜变量 [v& _MQ
更改MCFILE.MAC为 dEL>Uly
PANT ]#q dA(Kl
VY 14 TH @s[bRp`gd
VY 5 GPG ! Vary group gamma tilt on surfaces 5, 7, 9, and 12 (but not surface 1). aL`pvsnF
VY 7 GPG ~Ch`A@=5
VY 9 GPG {.2C>p
VY 12 GPG YA|*$$
END [_~U<
n/6A@C
A< Na,EC
AANT {u1t .+
M 0 1 A P YA ! Control the boresight error this way. ?|L)!LYx
M 0 1 A P XA M aEh8*
GSR .5 10 5 M 0 0 0 F ! Correct over the full pupil since the lens no longer has jgYiuM3c\
GNR .5 2 3 M .7 0 0 F ! bilateral symmetry. *oPSkEA{
GNR .5 1 3 M 1 0 0 F FJ!>3V;}
GNR .5 2 3 M -.7 0 0 F ! For the same reason we also control the negative field. Pf!K()<uJ
GNR .5 1 3 M -1 0 0 F [ wROIv V
END ~<eiWDf
SYNOPSYS 10 1TVTP2&Rd
MC QO,y/@ Ph
);6zV_^!
vKW%l
图像质量直方图 -R8RAwsLG
在Command Window中输入GET 5 Vr^wesT\Hx
在C28M2中注释掉TEST f+1]#"9i|
点击[attachment=92289]运行C28M2 8O7JuR
在Command Window中输入MC PLOT 3Q #VD)
[attachment=92298] j4l7Tx
e^FS/=
oYF8:PYB
eGE,zkj
FY
更改MCFILE tsk}]@W
在MCFILE.MAC中的命令SYNOPSYS 10和MC之间添加如下命令 pUPb+:^R
Z1 = XA IN COLOR 1 ! Get the actual X coordinate of the chief ray in color 1. }l/md/C0
RMS 1 0 555 ! Run the RMS command, which also finds the centroid. z#\Z|OK U
Z2 = FILE 4 ! This is the X-centroid location, relative to the chief ray, z(]*'0)P
Z3 = FILE 5 ! and this is the Y. XI0O^[/n{
Z4 = YA IN COLOR 1 ! Also get the actual Y coordinate. JvUKfsn u{
Z5 = XA IN COLOR 3 ! Do the same thing in color 3. 0 #q_LB
RMS 3 0 555 n% *u;iG
Z6 = FILE 4 0>'1|8+`(z
Z7 = FILE 5 m$ o|s1t
Z8 = YA IN COLOR 3 w&H
?; 1
= SQRT((Z1 + Z2 - Z5 - Z6)**2 + (Z3 + Z4 - Z7 - Z8)**2) ! The separation. e"b F" L
Z9 = FILE 1 ! Load it into variable Z9, and tell MC ?T^$,1 -
MC IZ9 "RedCen-BlueCen" ! to gather the statistics and plot Z9 with this label. Mz06cw&
dv,8iOL
"qF&%&#r'
e L(T
调整参数直方图 #e#8I7P
在Command Window中输入MC PLOT dRu@5
:BP
[attachment=92299] &o8\ $A
n8iN/Y<%U
W OwIJrP
5~sJ$5<,
总结 S<>e(x3g]
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。 1xx-}AIH#
RJWlG'i
o`#;[
感谢 K.cNx
ASDOPTICS -- Advanced Optical System Design pymT-
www.asdoptics.com Og,,s{\
sales@asdoptis.com ML R3 A
s
support@asdoptics.com 3QF !fll^
qH-dT,`"{
|
|