Presentation
22 November 2024 24hSHIMM: corrections and improving resolution of optical turbulence profiles
Ryan Griffiths, Florian Quatresooz, James Osborn, Richard Wilson
Author Affiliations +
Abstract
Characterisation of day and night atmospheric optical turbulence profiles is vital for validating turbulence forecasting tools and for site characterisation at optical ground stations. A scalable instrument providing accurate and detailed characterisation of optical turbulence conditions is therefore highly desirable. Recent advancements in real-time turbulence monitoring on the 24-hour Shack-Hartmann Image Motion Monitor (24hSHIMM) are discussed. The 24hSHIMM estimates the vertical profile of optical turbulence strength from observations of single stars in the short-wave-infrared. This talk will show how regularisation techniques can be employed on the 24hSHIMM to increase the accuracy of turbulence profiling and how non-zero exposure time and slow-moving, non-Kolmogorov conditions in the local environment can be corrected for. The feasibility of fitting an outer scale is also discussed. These techniques allow for a more complete and accurate characterisation of the optical turbulence which can be applied to any Shack-Hartmann system.
Conference Presentation
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Ryan Griffiths, Florian Quatresooz, James Osborn, and Richard Wilson "24hSHIMM: corrections and improving resolution of optical turbulence profiles", Proc. SPIE 13194, Environmental Effects on Light Propagation and Adaptive Systems VII, 1319406 (22 November 2024); https://doi.org/10.1117/12.3031692
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KEYWORDS
Optical turbulence

Wavefront sensors

Profiling

Equipment

Atmospheric optics

Environmental monitoring

Turbulence

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