Presentation
28 August 2024 A comparative analysis of novel turbulence profiling instrumentation at Paranal Observatory
Author Affiliations +
Abstract
A six-night optical turbulence monitoring campaign has been carried at Cerro Paranal observatory in February and March, 2023 to facilitate the development and characterisation of two novel atmospheric site monitoring instruments - the ring-image next generation scintillation sensor (RINGSS) and 24-hour Shack Hartmann image motion monitor (24hSHIMM) in the context of providing optical turbulence monitoring support for upcoming 20-40m class telescopes. Both instruments offer the potential to replace the outdated MASS-DIMM, utilising new technologies to produce detailed, real-time characterisation of optical turbulence conditions at a site. In addition, the well-characterised Stereo-SCIDAR and 2016-MASS-DIMM were both active throughout the campaign providing further data for comparison. Contemporaneous measurements of both the integrated turbulence parameters - including seeing, free atmosphere seeing, coherence time and angle – and the vertical optical turbulence profile are examined along with the first 24-hour, day and night turbulence measurements at the site.
Conference Presentation
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Ryan Griffiths, Lisa Bardou, Timothy Butterley, James Osborn, Richard Wilson, Edison Bustos, Andrei Tokovinin, Miska Le Louarn, and Angel Otarola "A comparative analysis of novel turbulence profiling instrumentation at Paranal Observatory", Proc. SPIE 13097, Adaptive Optics Systems IX, 130972U (28 August 2024); https://doi.org/10.1117/12.3018432
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