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