Experiment Layout of Space Laser Communication System Based on Adaptive Optical System

Article Preview

Abstract:

Sixty-one unit adaptive optical system was used to analyze the influence of atmospheric turbulence on laser beam transmission in space laser communication system. From low earth orbit planet to ground station Laser communication system was estimated by means of optical design software. In addition, the compensation results, experimental phenomena and data based on adaptive optics were also analyzed in the paper.

You might also be interested in these eBooks

Info:

Periodical:

Advanced Materials Research (Volumes 287-290)

Pages:

3020-3023

Citation:

Online since:

July 2011

Export:

Price:

Permissions CCC:

Permissions PLS:

Сopyright:

© 2011 Trans Tech Publications Ltd. All Rights Reserved

Share:

Citation:

[1] The research of atmospheric turbulence effects corrected by adaptive optical technology, Anhui Optical and Fine Machine Institute, Doctor thesis, (1992)

Google Scholar

[2] Zhang Deliang, Jiang Wenhan, Wu Xubin,The compensation effects analysis caused by atmospheric turbulence wavefront for adaptive optical system Journal of optics,Vol.18,No.10, 1998, 1372-1379

Google Scholar

[3] K.H. Kudielka, Y.Hayano, W.Klaus, K.Araki, Low-order adaptive optics system for free-space lasercom: design and performance analysis, Intl.Workshop on A.O. for Industry and Medicine, Durham, July (1999)

DOI: 10.1142/9789812817815_0058

Google Scholar

[4] R.J. Sasiela and J.D. Shelton, Transverse spectral filtering and Mellin transform techniques applied to the effect of outer scale on tilt anisoplanatism, J.Opt.Soc. Am.A 10, 1993, 646-660

DOI: 10.1364/josaa.10.000646

Google Scholar

[5] Dessenne,C., Model prediction for closed-loop adaptive optics, Opt.Lett. 20, 1997, 1535-1537

DOI: 10.1364/ol.22.001535

Google Scholar

[6] Sechaud, Wavefront sensing in imaging through the atmosphere: a detector strategy, SPIE, Vol.1543, 1991, 479-490

Google Scholar

[7] G.Rousset, First diffraction-limited astronomical images with adaptive optics, Astron.and Astrophys., Vol.230, 1990, 29-32

Google Scholar