切换到宽版
  • 广告投放
  • 稿件投递
  • 繁體中文
    • 6516阅读
    • 13回复

    [求助]关于出瞳 [复制链接]

    上一主题 下一主题
    离线hopebox
    发帖
    484
    光币
    332
    光券
    0
    只看该作者 10楼 发表于: 2012-08-09
    回 rzyp 的帖子
    rzyp:就是我问一下,细光束0.7071带的子午场曲,弧矢场曲,子午彗差,弧矢彗差在哪里找啊 (2012-08-09 10:32)  m?`Rl6!@8\  
    1uQf}  
    You could check "Scan Type" setting under Field Curvature/Distortion curve to either scan across x or y direction. In addition, you could use Grid Distortion, which give you an overview of distortion. L` "UeNT  
    X*q C:]e  
    For coma, it normally displays as a parabolic curve in Ray Fan plot but it can be a bit complicated to analyse if you also have other dominating aberrations. Another way to look into coma is by looking at Zernike Standard Coefficeint, the term 5 and 6 correspond to coma in y and x orientation respectively. ZERN operands should help to extract these values. ]YzAcB.R  
    .AW*7Pp`f  
    However, these are only for the third order. Once you go higher order aberrations, the conversion between Seidel and Zernike becomes not so stright forward.
    离线rcasiodu
    发帖
    289
    光币
    3053
    光券
    0
    只看该作者 11楼 发表于: 2012-08-10
    回 rzyp 的帖子
    rzyp:就是我问一下,细光束0.7071带的子午场曲,弧矢场曲,子午彗差,弧矢彗差在哪里找啊 (2012-08-09 10:32)  .Ps;O  
    H!u:P?j@\  
    可以利用TRAX TRAY REAX REAY这几个操作数根据像差的定义来描述像差(包括高阶的像差),与transverse ray fan plot类似。
    离线rzyp
    发帖
    427
    光币
    51
    光券
    0
    只看该作者 12楼 发表于: 2012-12-08
    感谢各位的指点
    离线qubaso
    发帖
    147
    光币
    11
    光券
    0
    只看该作者 13楼 发表于: 2013-09-21
    try to use "chief ray angle = 0" solve in "radius" column and limit the distance (mxca operand) in merit function