Huizhe Yang
Laboratory demonstration of an alternative laser guide stars wavefront sensing technique—projected pupil plane pattern
Yang, Huizhe; Bharmal, Nazim; Myers, Richard; Younger, Eddy
Authors
Dr Nazim Bharmal n.a.bharmal@durham.ac.uk
Senior Adaptive Optics Scientist
Richard Myers r.m.myers@durham.ac.uk
Emeritus Professor
Eddy Younger
Abstract
Adaptive optics (AO) is widely used in optical/near-infrared telescopes to remove the effects of atmospheric distortion, and laser guide stars (LGSs) are commonly used to ease the requirement for a bright, natural reference source close to the scientific target in an AO system. However, focus anisoplanatism renders single LGS AO useless for the next generation of extremely large telescopes. Here, we describe proof-of-concept experimental demonstrations of a LGS alternative configuration, which is free of focus anisoplanatism, with the corresponding wavefront sensing and reconstruction method, termed projected pupil plane pattern (PPPP). This laboratory experiment is a critical milestone between the simulation and on-sky experiment, for demonstrating the feasibility of PPPP technique and understanding technical details, such as extracting the signal and calibrating the system. Three major processes of PPPP are included in this laboratory experiment: the upward propagation, return path, and reconstruction process. From the experimental results, it has been confirmed that the PPPP signal is generated during the upward propagation and the return path is a reimaging process whose effect can be neglected (if the images of the backscattered patterns are binned to a certain size). Two calibration methods are used: the theoretical calibration is used for the wavefront measurement, and the measured calibration is used for closed-loop control. From both the wavefront measurement and closed-loop results, we show that PPPP achieves equivalent performance to a Shack–Hartmann wavefront sensor.
Citation
Yang, H., Bharmal, N., Myers, R., & Younger, E. (2019). Laboratory demonstration of an alternative laser guide stars wavefront sensing technique—projected pupil plane pattern. Journal of Astronomical Telescopes, Instruments, and Systems, 5(2), Article 029002. https://doi.org/10.1117/1.jatis.5.2.029002
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 12, 2019 |
Online Publication Date | May 7, 2019 |
Publication Date | May 7, 2019 |
Deposit Date | May 7, 2019 |
Publicly Available Date | May 8, 2019 |
Journal | Journal of Astronomical Telescopes, Instruments, and Systems |
Electronic ISSN | 2329-4221 |
Publisher | Society of Photo-optical Instrumentation Engineers |
Peer Reviewed | Peer Reviewed |
Volume | 5 |
Issue | 2 |
Article Number | 029002 |
DOI | https://doi.org/10.1117/1.jatis.5.2.029002 |
Public URL | https://durham-repository.worktribe.com/output/1302191 |
Files
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Copyright Statement
Huizhe Yang, Nazim Bharmal, Richard Myers, Eddy Younger, “Laboratory demonstration of an alternative
laser guide stars wavefront sensing technique—projected pupil plane pattern,” J. Astron. Telesc.
Instrum. Syst. 5(2), 029002 (2019), doi: 10.1117/1.JATIS.5.2.029002.
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