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Correction of finite spatial and temporal sampling effects in stereo-SCIDAR

Butterley, Timothy; Sarazin, Marc; Le Louarn, Miska; Osborn, James; Farley, Ollie J.D.

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Authors

Marc Sarazin

Miska Le Louarn

Profile image of Ollie Farley

Ollie Farley o.j.d.farley@durham.ac.uk
Post Doctoral Research Associate



Abstract

Stereo scintillation detection and ranging (S-SCIDAR) is a development of the well-established SCIDAR turbulence profiling technique. An S-SCIDAR instrument has been installed at the focus of one of the 1.8m Auxiliary Telescopes at Paranal observatory since April 2016. We discuss the limitations imposed by the Paranal S-SCIDAR instrument’s finite pixel size and exposure time. We present Monte Carlo simulation results quantifying the errors due to finite spatial and temporal sampling. We have reprocessed the existing S-SCIDAR dataset to compensate for these error sources; we discuss the impact of these corrections on the measured turbulence statistics.

Citation

Butterley, T., Sarazin, M., Le Louarn, M., Osborn, J., & Farley, O. J. (2020, December). Correction of finite spatial and temporal sampling effects in stereo-SCIDAR. Presented at SPIE Astronomical Telescopes + Instrumentation 2020, Online

Presentation Conference Type Conference Paper (published)
Conference Name SPIE Astronomical Telescopes + Instrumentation 2020
Start Date Dec 13, 2020
End Date Dec 18, 2020
Online Publication Date Dec 13, 2020
Publication Date 2020
Deposit Date Nov 2, 2021
Publicly Available Date Nov 2, 2021
Publisher SPIE
Volume 11448
ISBN 9781510636835
DOI https://doi.org/10.1117/12.2562559
Public URL https://durham-repository.worktribe.com/output/1675963

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Copyright Statement
Copyright 2020 (year) Society of Photo Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.






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