[求助]非序列优化数据条件怎么选择，求大神们指点！ [复制链接]

000落月000:哪位大神能做匀光优化啊 (2013-05-21 16:18)  )_&<u\cm L  

K1C
#  
没办法，只能用非序列

只能用非序列，求高手帮一下啊

非序列优化，在zemax说明书里有很详细的说明，看不懂英文，可以看高老师的光学设计指引帖第9贴。里面有非序列优化的详细操作步骤。 PmTA3aH  
根据我个人的使用经验，非序列优化的能力较差，与初始结构相比无重大改善。

不懂。。。

没有NSDD的说明哦！！！

我在用非序列优化时也出现问题了呢，不知是模型建的有问题还是优化哪里设置的不对，优化完基本系统基本没变，想要的结果也没有达到

同问，以前没用过非序列的，现在好不容易把结构弄对了，可是不会优化

lingchen12:同问，以前没用过非序列的，现在好不容易把结构弄对了，可是不会优化 (2013-07-16 18:25)  sBB>O@4  

]qvrpI!E!  
我也是，好不容易结构出来了，非序列优化好迷茫啊

蕴藉之身:没有NSDD的说明哦 (2013-05-16 17:07)  Y=6569U2  

lC|`DG-B  
Non-sequential incoherent intensity data. Surf defines the surface number of the NSC group HQGn[7JW  
(always 1 in pure NSC systems). Det# refers to the object number of the desired detector. If Det# .FYxVF.  
is zero, then all detectors are cleared. If Det# is less than zero, then the detector defined by the z_nv|5"  
absolute value of Det# only is cleared. rr~O6Db  
For Detector Rectangles, Detector Surfaces, and all faceted detectors: If Pix# is a positive integer "T
e[R%aP  
greater than zero, then the data from the specified pixel is returned. Otherwise, the following data f=:ycd!  
is returned depending upon the value of Pix#: ||yx?q6\h  
0: Sum of the total flux in position space, average flux/area in position space, or total flux in angle >h)D~U(H  
space for all pixels for that detector object, for Data = 0, 1, or 2, respectively. uW;[FTcqy$  
-1: Maximum flux or flux/area. %'+}-w  
-2: Minimum flux or flux/area. N(c`h  
-3: Number of rays striking the detector. :O)\+s-  
-4: Standard deviation (RMS from the mean) of all the non-zero pixel data. EC;R^)  
-5: The mean value of all the non-zero pixel data. FWC\(f  
-6, -7, -8: The x, y, or z coordinate of the position or angle Irradiance or Intensity centroid, <UsFBF  
respectively. y Ny,$1  
-9,-10, -11, -12: The RMS radius, x, y, or z distance or angle of all the pixel data with respect to the &;3iHY;  
centroid. \*yH33B9  
Data is 0 for flux, 1 for flux/area, and 2 for flux/solid angle pixel. Only values 0 and 1 (for flux and W2>VgMR [  
flux/area) are supported for faceted detectors. See “Optimizing with sources and detectors in nonsequential Y(mnGaVn  
mode” on page 502 for complete details.

太熬了我