概述 -Lb7=98
ASY查看倾斜数据 Dsc0;7~6
MC PLOT预估公差Monte-Carlo分析 .jC5 y&
q@;1{
.}Ys+d1b9c
设置工作目录 T}29(xz-(h
选择Dbook工作目录 ^e;9_(
W\5 -Yg(@
P{:Z xli0
参考Donald Dilworth《Lens Design Automatic and quasi-autonomous computational methods and techniques》第28章 ^w"hA;
wPu.hVz
]\oT({$6B
初始透镜 v,z~#$T&
KhX)maQ
点击打开C28M1,点击 =n_z `I
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 _5(1T%K)
P/^@t+KC
}A;YM1^$
VlSM/y5
|!7leL
准备Monte-Carlo分析 `-R&4%t%
在Command Window中输入LM MCFILE Gm9
MCFILE是调整MACro,是Monte-Carlo分析的一部分 7#oq|5
点击运行MCFIlE b!Nr
点击 打开C28M2.MAC,点击 7/k7V)
oSf`F1;)HQ
o:"(\$
有透镜都有楔角 KIR3m
)
在Command Window中输入GET 5 $<C",&
在C28M2中注释掉TEST,更改SAMPLES 1为SAMPLES 100 6A|XB3
点击运行C28M2 L+T7Ge
q
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。 i gjn9p&_
U>bIQk"4
C!9mygI
b`j9}tZ
f\Hw Y)^>
Nh/i'q/
图像质量直方图 Kng=v~)N'
8;c\}D
在Command Window中输入MC PLOT O@W/s!&lFa
6#K.n&=*
MU2kA&LH
&2[Xu4*
#R31VQwK5
T /IX(b'<
ASY查看倾斜数据 9) $[W
在C28M2中取消注释TEST,并在TEST前加入命令WEDGES CLOCK,点击运行C28M2 {hN<Ot
在Command Window中输入ASY &y|Ps eH"
ycki0&n3
8'bZR]
表面 1,5,7,9 和 12 已经被分配了组倾斜 U 0~BcFpD
bi+g=cS
Eyk:pnKJb
增加伽马倾斜变量 BD}%RTeWKq
更改MCFILE.MAC为 ? u".*!%
PANT J(maJuY
VY 14 TH \ Ucv<S
VY 5 GPG ! Vary group gamma tilt on surfaces 5, 7, 9, and 12 (but not surface 1). <RbfW'<G
VY 7 GPG *=v%($~PK6
VY 9 GPG l,(:~KH|
VY 12 GPG MZcvr 9y
END ydY 7 :D
t0v>J9
#Dz"g_d
AANT tl7:L>
M 0 1 A P YA ! Control the boresight error this way. _h,_HW)G
M 0 1 A P XA x%goyXK
GSR .5 10 5 M 0 0 0 F ! Correct over the full pupil since the lens no longer has %hZX XpuO
GNR .5 2 3 M .7 0 0 F ! bilateral symmetry. vdB2T2F
GNR .5 1 3 M 1 0 0 F (JnEso-V
GNR .5 2 3 M -.7 0 0 F ! For the same reason we also control the negative field. >=:mtcph
GNR .5 1 3 M -1 0 0 F m$(OQ,E
END QlR~rFs9t
SYNOPSYS 10 8\:>;XG6f
MC ?[>Y@we
matm>3n
$F X$nY
图像质量直方图 omy3<6
在Command Window中输入GET 5 <gH-`3J6
在C28M2中注释掉TEST fO^s4gWTg
点击运行C28M2 /38I(0
在Command Window中输入MC PLOT YPq:z"`-y4
$3&XM
'NfsAE
tSoF!@6
@"/H
er
更改MCFILE {%^4%Eco
在MCFILE.MAC中的命令SYNOPSYS 10和MC之间添加如下命令 !Icznou\
Z1 = XA IN COLOR 1 ! Get the actual X coordinate of the chief ray in color 1. $^czqA-&
RMS 1 0 555 ! Run the RMS command, which also finds the centroid. Oj_F1.
r
Z2 = FILE 4 ! This is the X-centroid location, relative to the chief ray, @icw:68
Z3 = FILE 5 ! and this is the Y. `_ M+=*}
Z4 = YA IN COLOR 1 ! Also get the actual Y coordinate. ,D(Bg9C
Z5 = XA IN COLOR 3 ! Do the same thing in color 3. DcM/p8da
RMS 3 0 555 b2[U3)|oO
Z6 = FILE 4 vSoG] :1
Z7 = FILE 5 (f_J @n
Z8 = YA IN COLOR 3 vUO[V$rx
= SQRT((Z1 + Z2 - Z5 - Z6)**2 + (Z3 + Z4 - Z7 - Z8)**2) ! The separation. KC2Z@
Z9 = FILE 1 ! Load it into variable Z9, and tell MC TqV^\C?
MC IZ9 "RedCen-BlueCen" ! to gather the statistics and plot Z9 with this label. >t'A1`W
+_S0
j;D$qd'J
T@#?{eA
调整参数直方图 h&d"| <
在Command Window中输入MC PLOT C0Fd<