NEW METHOD FOR ESTIMATING WAVE-FRONT FROM CURVATURE SIGNAL BY CURVE-FITTING

被引:19
作者
HAN, I [1 ]
机构
[1] UNIV PITTSBURGH,ALLEGHENY OBSERV,PITTSBURGH,PA
关键词
ABERRATIONS; WAVE-FRONT ESTIMATION; ASTRONOMY; TELESCOPE OPTICS;
D O I
10.1117/12.196542
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We present a new method to estimate the wavefront with the curvature-sensing technique proposed by F. Roddier. Instead of solving a Poisson equation for the curvature signal, we estimate the wavefront by direct least-squares curve fitting of the curvature signal with derivatives of Zernike polynomials. It is computationally simpler and faster. From computer simulations, it is shown that the curve-fitting method gives quite accurate wavefront estimation. It is especially useful when only a fixed number of aberration modes are of interest, as in the optical-axis adjustment of a telescope.
引用
收藏
页码:1232 / 1237
页数:6
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