DocumentCode :
2051534
Title :
Bandwidth Improvement of Fast Steering Mirror by FEDA
Author :
Zheng, Yu ; Zhang, Guoyu ; Xu, Bing ; Jiang, Wenhan
Author_Institution :
Dept. of Electrooptical Eng., Changchun Univ. of Sci. & Technol.
fYear :
2006
fDate :
18-21 Jan. 2006
Firstpage :
52
Lastpage :
55
Abstract :
The bandwidth of fast steering mirror (FSM) is about several tens of hertz which is related to Tylar frequency of atmospheric turbulence, and the bandwidth of deformable mirror ranges from several tens to hundreds hertz relates to Greenwood frequency of atmospheric turbulence. According to practical experience, the ratio of fast steering mirror and deformable mirror should be from one is to five to one is to ten when corrects static atmospheric turbulence, and should be one is to two even one is to one when corrects dynamic targets, such as plane and satellite. All these require improve fast steering mirror´s bandwidth to several hundreds frequency. The reason why fast steering mirror´s harmonic frequency lower is analyzed in the paper set out from the point of fast steering mirror´s structural designation, and the way of improve its bandwidth by finite element dynamic analysis (FEDA) is discussed detailed
Keywords :
atmospheric turbulence; finite element analysis; mirrors; FEDA; Greenwood frequency; Tylar frequency; atmospheric turbulence; bandwidth improvement; deformable mirror; fast steering mirror; finite element analysis; finite element dynamic analysis; Adaptive optics; Bandwidth; Error correction; Finite element methods; Frequency; Harmonic analysis; Laser beams; Laser stability; Mirrors; Open loop systems; bandwid; deformable mirror; fast steering mirror; finite element analysis; harmonic frequency;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Nano/Micro Engineered and Molecular Systems, 2006. NEMS '06. 1st IEEE International Conference on
Conference_Location :
Zhuhai
Print_ISBN :
1-4244-0139-9
Electronic_ISBN :
1-4244-0140-2
Type :
conf
DOI :
10.1109/NEMS.2006.334620
Filename :
4134902
Link To Document :
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