Wavefront sensing and control for a segmented primary mirror

2008 ◽  
Author(s):  
Bing Dong ◽  
Xin Yu ◽  
Xiaofang Zhang ◽  
Baiwei Guo ◽  
Lei Zhao
Photonics ◽  
2020 ◽  
Vol 8 (1) ◽  
pp. 3
Author(s):  
Shun Qin ◽  
Wai Kin Chan

Accurate segmented mirror wavefront sensing and control is essential for next-generation large aperture telescope system design. In this paper, a direct tip–tilt and piston error detection technique based on model-based phase retrieval with multiple defocused images is proposed for segmented mirror wavefront sensing. In our technique, the tip–tilt and piston error are represented by a basis consisting of three basic plane functions with respect to the x, y, and z axis so that they can be parameterized by the coefficients of these bases; the coefficients then are solved by a non-linear optimization method with the defocus multi-images. Simulation results show that the proposed technique is capable of measuring high dynamic range wavefront error reaching 7λ, while resulting in high detection accuracy. The algorithm is demonstrated as robust to noise by introducing phase parameterization. In comparison, the proposed tip–tilt and piston error detection approach is much easier to implement than many existing methods, which usually introduce extra sensors and devices, as it is a technique based on multiple images. These characteristics make it promising for the application of wavefront sensing and control in next-generation large aperture telescopes.


1970 ◽  
Vol 14 (1) ◽  
pp. 39-51
Author(s):  
A. A. Nemiro ◽  
W. Fricke ◽  
A. N. Adams ◽  
P. Lacroute ◽  
R. H. Stoy ◽  
...  

It is with deep regret that we mention the death, on 15 July 1969, of Prof. Dr G. Demetrescu who has done so much for the development of Astronomy in Roumania.This report is based on letters received from members of the Commission, whom I wish to thank most cordially.The most important events in the development of positional astronomy during the three past years were:(1)The construction and use of new types of astronomical instruments based on new techniques, and(2)The collective observations of large numbers of stars, especially in the Southern hemisphere on the basis of international cooperation.At the USNO a design study for a ten-inch automatic meridian circle (ATC)was completed in 1968. Construction and installation should be completed by the end of 1970. A modified Cassegrainian optical system with a Cer-Vit primary mirror is being used. For some other important parts of the instrument new materials will also be used. At each end of the horizontal axis of the instrument Inductosyns will be mounted.An Inductosyn system for digital readout of the pointing angle of the telescope was installed on the six-inch transit circle of the USNO in 1967 for testing and calibration. An IBM-1800 data acquisition and control system was on line with the same instrument.


2004 ◽  
Author(s):  
Daniel S. Acton ◽  
Paul D. Atcheson ◽  
Mick Cermak ◽  
Lana K. Kingsbury ◽  
Fang Shi ◽  
...  

Author(s):  
Steven P. Bos ◽  
Kelsey L. Miller ◽  
Julien Lozi ◽  
Olivier Guyon ◽  
Vikram Mark Radhakrishnan ◽  
...  

1998 ◽  
Author(s):  
Claudia M. LeBoeuf ◽  
Pamela S. Davila ◽  
David C. Redding ◽  
Armando Morrell ◽  
Andrew E. Lowman ◽  
...  

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