下面这个函数大家都不会陌生,计算zernike函数值的,并根据此可以还原出图像来, KDP"z
我输入10阶的n、m,r,theta为38025*1向量,最后得到的z是29525*10阶的矩阵, pU'${Z~b
这个,跟我们用zygo干涉仪直接拟合出的36项zernike系数,有何关系呢? {~w( pAx
那些系数是通过对29525*10阶的矩阵每列的值算出来的嘛? m(o`;
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function z = zernfun(n,m,r,theta,nflag) ^$}O?y7O
%ZERNFUN Zernike functions of order N and frequency M on the unit circle. bI|{TKKN&P
% Z = ZERNFUN(N,M,R,THETA) returns the Zernike functions of order N 'J3yJ{
% and angular frequency M, evaluated at positions (R,THETA) on the ` &bF@$((
% unit circle. N is a vector of positive integers (including 0), and ,]nRnI^
% M is a vector with the same number of elements as N. Each element Wp+lI1t
% k of M must be a positive integer, with possible values M(k) = -N(k) %hN(79:g
% to +N(k) in steps of 2. R is a vector of numbers between 0 and 1, DaJ,(DJY
% and THETA is a vector of angles. R and THETA must have the same 8#g}ev@|u
% length. The output Z is a matrix with one column for every (N,M) ITg:OOQ
% pair, and one row for every (R,THETA) pair. 'wtb"0 }
% 0|J9Btbp
% Z = ZERNFUN(N,M,R,THETA,'norm') returns the normalized Zernike ~JNE]mg
% functions. The normalization factor sqrt((2-delta(m,0))*(n+1)/pi), ~cyKPg6
% with delta(m,0) the Kronecker delta, is chosen so that the integral *xmC`oP
% of (r * [Znm(r,theta)]^2) over the unit circle (from r=0 to r=1, rk4KAX_[
% and theta=0 to theta=2*pi) is unity. For the non-normalized jSM`bE+"
% polynomials, max(Znm(r=1,theta))=1 for all [n,m]. 4w'&:k47
% 6rj iZ%
% The Zernike functions are an orthogonal basis on the unit circle. QlV(D<
% They are used in disciplines such as astronomy, optics, and Q)BSngW+
% optometry to describe functions on a circular domain. EpKZ.lCU
% $y,KDR7^
% The following table lists the first 15 Zernike functions. Fx}v.A5
% TB?'<hD:
% n m Zernike function Normalization '
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% -------------------------------------------------- ]
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% 0 0 1 1 (gPB@hAv
% 1 1 r * cos(theta) 2 qo7<g*kf~
% 1 -1 r * sin(theta) 2 ("ix!\1K@
% 2 -2 r^2 * cos(2*theta) sqrt(6) H! 5Ka#B
% 2 0 (2*r^2 - 1) sqrt(3) R+0gn/a[ G
% 2 2 r^2 * sin(2*theta) sqrt(6) -?:8sv*X
% 3 -3 r^3 * cos(3*theta) sqrt(8) rqiH!R
% 3 -1 (3*r^3 - 2*r) * cos(theta) sqrt(8) tmoCy0qWz
% 3 1 (3*r^3 - 2*r) * sin(theta) sqrt(8) SmD#hE[
% 3 3 r^3 * sin(3*theta) sqrt(8) TTl9xs,nO
% 4 -4 r^4 * cos(4*theta) sqrt(10) d*e8P ep
% 4 -2 (4*r^4 - 3*r^2) * cos(2*theta) sqrt(10) ks("(
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% 4 0 6*r^4 - 6*r^2 + 1 sqrt(5) )m3emMO2
% 4 2 (4*r^4 - 3*r^2) * cos(2*theta) sqrt(10) {fDRVnI?
% 4 4 r^4 * sin(4*theta) sqrt(10) V"(5U(v{~
% -------------------------------------------------- wBg?-ji3<
% N0}[&rE 8
% Example 1: 568M4xzi
% X_nbNql
% % Display the Zernike function Z(n=5,m=1) .sQV0jF {
% x = -1:0.01:1; Z:,\FB_U
% [X,Y] = meshgrid(x,x); #:yAi_Ct
% [theta,r] = cart2pol(X,Y); {+cx} `
% idx = r<=1; ;`c:Law4
% z = nan(size(X)); @HB=hN
% z(idx) = zernfun(5,1,r(idx),theta(idx)); \'u+iB
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% figure
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% pcolor(x,x,z), shading interp i
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