THE CONTRIBUTION OF HIGH-ORDER ZERNIKE MODES TO WAVE-FRONT TILT

被引：8
|
作者：
TENBRUMMELAAR, TA
机构：
[1] Center for High Angular Resolution Astronomy, Georgia State University, Atlanta
来源：
OPTICS COMMUNICATIONS | 1995年 / 115卷 / 5-6期
基金：
美国国家科学基金会; 澳大利亚研究理事会;
关键词：
D O I：
10.1016/0030-4018(95)00053-B
中图分类号：
O43 [光学];
学科分类号：
070207 ; 0803 ;
摘要：
The contribution of high order Zemike modes on average phase gradient is investigated. The resulting temporal power spectra are compared to data collected using the tip/tilt servo at the Sydney University Stellar Interferometer (SUSI). The low frequency part of the power spectrum follows a -2/3 power law which is in agreement with other similar work. Due to the effect of higher order terms, the high frequency power law for average phase gradient becomes -11/3 rather than the -17/3 predicted for the 'tilt' component of the Zemike representation of the wavefront.
引用
收藏
页码：417 / 424
页数：8
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