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, sO0j!;N
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, `c /mmS
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? P"<,@Mn
那些系数是通过对29525*10阶的矩阵每列的值算出来的嘛? :z a:gs0
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function z = zernfun(n,m,r,theta,nflag) {7d\du&G
%ZERNFUN Zernike functions of order N and frequency M on the unit circle. Tu7sA.73k
% Z = ZERNFUN(N,M,R,THETA) returns the Zernike functions of order N ;)'
% and angular frequency M, evaluated at positions (R,THETA) on the mecm,xwm
% unit circle. N is a vector of positive integers (including 0), and ?vV&tqnx%
% M is a vector with the same number of elements as N. Each element r"=6s/q7
% k of M must be a positive integer, with possible values M(k) = -N(k) >f-*D25f%
% to +N(k) in steps of 2. R is a vector of numbers between 0 and 1, 0`
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% and THETA is a vector of angles. R and THETA must have the same nx|b9W<
% length. The output Z is a matrix with one column for every (N,M) J:G~9~V^
% pair, and one row for every (R,THETA) pair. ,xuA%CF-S
% T )"Uq
% Z = ZERNFUN(N,M,R,THETA,'norm') returns the normalized Zernike 9t_N9@
% functions. The normalization factor sqrt((2-delta(m,0))*(n+1)/pi), Nj$h/P
% with delta(m,0) the Kronecker delta, is chosen so that the integral V J]S"
% of (r * [Znm(r,theta)]^2) over the unit circle (from r=0 to r=1, nW!pOTJq21
% and theta=0 to theta=2*pi) is unity. For the non-normalized C25 2E
% polynomials, max(Znm(r=1,theta))=1 for all [n,m]. /..a9x{At>
% :y3e-lr
% The Zernike functions are an orthogonal basis on the unit circle. OuV
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% They are used in disciplines such as astronomy, optics, and < SvjvV
% optometry to describe functions on a circular domain. .Uh|V-
% EbMG9
% The following table lists the first 15 Zernike functions. lWWy|r'il
% !y-,r4\@`
% n m Zernike function Normalization GOj<>h}r
% -------------------------------------------------- 6/l{e)rX2o
% 0 0 1 1 Is#w=s}2
% 1 1 r * cos(theta) 2 q
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% 1 -1 r * sin(theta) 2 al{}p
% 2 -2 r^2 * cos(2*theta) sqrt(6) 9P\R?~3
% 2 0 (2*r^2 - 1) sqrt(3) q.Vcb!*$
% 2 2 r^2 * sin(2*theta) sqrt(6) ~#nbD-*#
% 3 -3 r^3 * cos(3*theta) sqrt(8) -|YDKcL
% 3 -1 (3*r^3 - 2*r) * cos(theta) sqrt(8) ;ep@
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% 3 1 (3*r^3 - 2*r) * sin(theta) sqrt(8) @;g|styh^
% 3 3 r^3 * sin(3*theta) sqrt(8) oz#;7
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% 4 -4 r^4 * cos(4*theta) sqrt(10) ;SVAar4r
% 4 -2 (4*r^4 - 3*r^2) * cos(2*theta) sqrt(10) 9t o2V
% 4 0 6*r^4 - 6*r^2 + 1 sqrt(5) )&wJ