Paper
25 July 2024 A strategy for forecasting the seeing of astronomical site at short and long time-scales
Kang Huang, Yonghui Hou, Tianzhu Hu, Teng Xu
Author Affiliations +
Abstract
Atmospheric seeing, a crucial astronomical meteorological parameter, directly affects the imaging quality of astronomical telescopes. Establishing a reliable mechanism for predicting atmospheric seeing is vital for enabling flexible scheduling of telescope observations and enhancing observational efficiency. This study aims to develop a forecasting mechanism for atmospheric seeing over both short timescales (one to two hours) and long timescales (up to three days), based on a combination of the mesoscale meteorological model Weather Research and Forecasting (WRF) and Recurrent Neural Networks (RNN). The WRF model predicts meteorological parameters for a given future period at the target astronomical site, which, when coupled with an atmospheric seeing analytical model, facilitates seeing forecasts for a long-time scale. Concurrently, the RNN establishes a relationship between observed meteorological parameters and seeing, enabling short time-scale predictions of atmospheric seeing at the site. Experiments conducted at target astronomical observatory demonstrate the reliability of our proposed forecasting strategy.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Kang Huang, Yonghui Hou, Tianzhu Hu, and Teng Xu "A strategy for forecasting the seeing of astronomical site at short and long time-scales", Proc. SPIE 13098, Observatory Operations: Strategies, Processes, and Systems X, 130982F (25 July 2024); https://doi.org/10.1117/12.3018837
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KEYWORDS
Atmospheric modeling

Data modeling

Analytic models

Atmospheric optics

Observatories

Telescopes

Temperature metrology

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