Statistical Interpolation Method of Turbulent Phase Screen


Autoria(s): Wu HL(吴晗玲); Yan HX(严海星); Li XY; Li SS(李树山)
Data(s)

2009

Resumo

A relative displacement between the grid points of optical fields and those of phase screens may occur in the simulation of light propagation through the turbulent atmosphere. A statistical interpolator is proposed to solve this problem in this paper. It is evaluated by the phase structure function and numerical experiments of light propagation through atmospheric turbulence with/without adaptive optics (AO) and it is also compared with the well-known linear interpolator under the same condition. Results of the phase structure function show that the statistical interpolator is more accurate in comparison with the linear one, especially in the high frequency region. More importantly, the long-exposure results of light propagation through the turbulent atmosphere with/without AO also show that the statistical interpolator is more accurate and reliable than the linear one. (C) 2009 Optical Society of America.

Identificador

http://dspace.imech.ac.cn/handle/311007/26501

http://www.irgrid.ac.cn/handle/1471x/2584

Idioma(s)

英语

Palavras-Chave #流体力学::湍流 #PERFORMANCE ANALYSIS #WAVE-FRONTS #SIMULATION #PROPAGATION #ATMOSPHERE #GENERATOR #SERIES #LONG
Tipo

期刊论文