Ollie Farley o.j.d.farley@durham.ac.uk
Post Doctoral Research Associate
Limitations imposed by optical turbulence profile structure and evolution on tomographic reconstruction for the ELT
Farley, OJD; Osborn, J; Morris, T; Fusco, T; Neichel, B; Correia, C; Wilson, RW
Authors
Professor James Osborn james.osborn@durham.ac.uk
Professor
Professor Timothy Morris t.j.morris@durham.ac.uk
Professor
T Fusco
B Neichel
C Correia
RW Wilson
Abstract
The performance of tomographic adaptive optics (AO) systems is intrinsically linked to the vertical profile of optical turbulence. First, a sufficient number of discrete turbulent layers must be reconstructed to model the true continuous turbulence profile. Secondly over the course of an observation, the profile as seen by the telescope changes and the tomographic reconstructor must be updated. These changes can be due to the unpredictable evolution of turbulent layers on meteorological time-scales as short as minutes. Here, we investigate the effect of changing atmospheric conditions on the quality of tomographic reconstruction by coupling fast analytical AO simulation to a large data base of 10 691 high-resolution turbulence profiles measured over two years by the Stereo-SCIDAR instrument at ESO Paranal, Chile. This work represents the first investigation of these effects with a large, statistically significant sample of turbulence profiles. The statistical nature of the study allows us to assess not only the degradation and variability in tomographic error with a set of system parameters (e.g. number of layers and temporal update period), but also the required parameters to meet some error threshold. In the most challenging conditions where the profile is rapidly changing, these parameters must be far more tightly constrained in order to meet this threshold. By providing estimates of these constraints for a wide range of system geometries as well as the impact of different temporal optimization strategies we may assist the designers of tomographic AO for the extremely large telescope to dimension their systems.
Citation
Farley, O., Osborn, J., Morris, T., Fusco, T., Neichel, B., Correia, C., & Wilson, R. (2020). Limitations imposed by optical turbulence profile structure and evolution on tomographic reconstruction for the ELT. Monthly Notices of the Royal Astronomical Society, 494(2), 2773-2784. https://doi.org/10.1093/mnras/staa795
Journal Article Type | Article |
---|---|
Acceptance Date | Mar 16, 2020 |
Online Publication Date | Apr 2, 2020 |
Publication Date | 2020-05 |
Deposit Date | Jun 10, 2020 |
Publicly Available Date | Jun 10, 2020 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 494 |
Issue | 2 |
Pages | 2773-2784 |
DOI | https://doi.org/10.1093/mnras/staa795 |
Public URL | https://durham-repository.worktribe.com/output/1269085 |
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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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