Representative optical turbulence profiles for ESO Paranal by hierarchical clustering
O. J. D. Farley, J. Osborn, T. Morris, M. Sarazin, T. Butterley, M. J., Townson, P. Jia, and R. W. Wilson

TL;DR
This paper introduces a hierarchical clustering method to condense large turbulence profile datasets into a small, representative set for adaptive optics simulations, demonstrated on ESO Paranal data.
Contribution
It presents a novel application of hierarchical clustering to derive representative turbulence profiles from large datasets for AO system modeling.
Findings
Two sets of 18 representative profiles effectively capture turbulence variability.
Hierarchical clustering outperforms simple averaging in representing turbulence profile diversity.
Small profile sets struggle to fully encapsulate turbulence variability based on integrated parameters.
Abstract
Knowledge of the optical turbulence profile is important in adaptive optics (AO) systems, particularly tomographic AO systems such as those to be employed by the next generation of 40 m class extremely large telescopes (ELTs). Site characterisation and monitoring campaigns have produced large quantities of turbulence profiling data for sites around the world. However AO system design and performance characterisation is dependent on Monte-Carlo simulations that cannot make use of these large datasets due to long computation times. Here we address the question of how to reduce these large datasets into small sets of profiles that can feasibly be used in such Monte-Carlo simulations, whilst minimising the loss of information inherent in this effective compression of the data. We propose hierarchical clustering to partition the dataset according to the structure of the turbulence profiles…
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