Optical turbulence forecast: toward a new era of ground-based astronomy
E. Masciadri

TL;DR
This paper discusses the development of optical turbulence forecasting using meso-scale atmospheric models to improve ground-based astronomy, especially for Extremely Large Telescopes, by predicting turbulence effects more accurately.
Contribution
It presents the goals and challenges of a European project aimed at validating and advancing optical turbulence forecasts for astronomical site assessment.
Findings
Feasibility of simulating realistic Cn2 profiles above astronomical sites.
Potential to discriminate between different astronomical sites based on turbulence forecasts.
Advancement in the integration of meteorology and astrophysics for telescope site management.
Abstract
The simulation of the optical turbulence (OT) for astronomical applications obtained with non-hydrostatic atmospherical models at meso-scale presents, with respect to measurements, some advantages. The future of the ground-based astronomy relies upon the potentialities and feasibility of the ELTs. Our ability in knowing, controlling and 'managing' the effects of the turbulence on such a new generation telescopes and facilities are determinant to assure their competitiveness with respect to the space astronomy. In the past several studies have been carried out proving the feasibility of the simulation of realistic Cn2 profiles above astronomical sites. The European Community (FP6 Program) decided recently to fund a Project aiming, from one side, to prove the feasibility of the OT forecasts and the ability of meso-scale models in discriminating astronomical sites from optical turbulence…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
