Abstract
We report on a tapered three-core optical fibre that can be used as a tip-tilt wavefront sensor. In this device, a coupled region of a few millimetres at the sensing tip of the fibre converts fragile phase information from an incoming wavefront into robust intensity information within each of the cores. The intensity information can be easily converted to linear wavefront error over small ranges, making it ideal for closed loop systems. The sensor uses minimal information to infer tip-tilt and is compatible with remote detector arrays. We explore its application within adaptive optics and present a validation case to show its applicability to astronomy.
Original language | English |
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Pages (from-to) | 5422-5428 |
Number of pages | 7 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 514 |
Issue number | 4 |
Early online date | 15 Jun 2022 |
DOIs | |
Publication status | Published - 1 Aug 2022 |
Bibliographical note
Funding Information:This work w as supported by the European Union's Horizon 2020 research and innovation programme under grant no. 730890 (OPTICON-Optical Infrared Coordination Network for Astronomy).
Data Availability
Data underlying the results presented are available in Wright et al. (2022).
Keywords
- instrumentation: adaptive optics
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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Wright, T. (Creator), Yerolatsitis, S. (Creator), Harrington, K. (Creator), Harris, R. (Creator) & Birks, T. (Creator), University of Bath, 13 Jun 2022
DOI: 10.15125/BATH-01135
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