優化放大率重點有三 SUS=sR/N
1) 保持物鏡焦距 。 DiFLat]X
2) 保持目鏡焦距 。 H C iRk1
3) 調整二鏡間距，以保持(主光線出射角)和(主光線入射角)的比值。 fz'qB-F
Y
N'
hT
假如你有 Code V 10.7 版，可以執行以下程式 }b_O b
MAh1tYs4D
res telescope1 (x=$b(I
del z2 H& |/|\8F
AuNUW0/
7
^EFLObj == (efy s1..3) e@D_0OZ
^EFLEye == (efy s5..12) HNzxF nh
^AngMag == (UCY SI-1)/(UCY S0) pH '_k k
nY'V, v [F
aut Z.VKG1e}
efy s1..3 = 200 d |17G
efy s5..12 = 40 ASqYA1p.
@AngMag == (UCY SI-1)/(UCY S0) {
I #>6
@AngMag = -5 BP/nK.
dra; kR =sr/{
go mU5Ox4>&9
W +h2 rv
wri "Before Optimization:" BgQEd@cN
wri " EFL of the objective lens = " ^EFLObj "\|P 6H
wri " EFL of the eyepiece = " ^EFLEye rc_m{.b
wri " Angular magnification = " ^AngMag >kXscbRL7
wri abo=v<m R
wri "After Optimization:" qb>ULP0
wri " EFL of the objective lens = " (efy s1..3) oe<i\uX8z
wri " EFL of the eyepiece = " (efy s5..12) 4@9Pd &I
wri " Angular magnification = " (UCY SI-1)/(UCY S0) IeYYG^V<A
