非常感谢啊,我手上也有zernike多项式的拟合的源程序,也不知道对不对,不怎么会有 ocuVDC
function z = zernfun(n,m,r,theta,nflag) v4>"p!_C
%ZERNFUN Zernike functions of order N and frequency M on the unit circle. c'#J{3d
% Z = ZERNFUN(N,M,R,THETA) returns the Zernike functions of order N X@AkA9'fq
% and angular frequency M, evaluated at positions (R,THETA) on the eW*ae;-
% unit circle. N is a vector of positive integers (including 0), and ;{q) |GRF
% M is a vector with the same number of elements as N. Each element )(!Z90@
% k of M must be a positive integer, with possible values M(k) = -N(k) /e?ux ~f|
% to +N(k) in steps of 2. R is a vector of numbers between 0 and 1, .yfqS|(
% and THETA is a vector of angles. R and THETA must have the same V =aoB
Z
% length. The output Z is a matrix with one column for every (N,M) S}[:;p?F`
% pair, and one row for every (R,THETA) pair. +ZA\M:^b
% Fx99"3`3
% Z = ZERNFUN(N,M,R,THETA,'norm') returns the normalized Zernike &aAo:pj
% functions. The normalization factor sqrt((2-delta(m,0))*(n+1)/pi), O-lh\9{'R
% with delta(m,0) the Kronecker delta, is chosen so that the integral ;6 qdOD6
% of (r * [Znm(r,theta)]^2) over the unit circle (from r=0 to r=1, >\.[}th}
% and theta=0 to theta=2*pi) is unity. For the non-normalized fQ.>G+0I>
% polynomials, max(Znm(r=1,theta))=1 for all [n,m]. `L*;58MA
% e, 0I~:
% The Zernike functions are an orthogonal basis on the unit circle. F4<2.V)#-
% They are used in disciplines such as astronomy, optics, and s&`XK$p
% optometry to describe functions on a circular domain. YB3=ij!K
% M@X#[w:
% The following table lists the first 15 Zernike functions. g7z9i[
% ^t
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% n m Zernike function Normalization ftH%, /,
% -------------------------------------------------- "sx&