Application of a Regional Model to Astronomical Site Testing in Western Antarctica
Mark Falvey, Patricio M. Rojo

TL;DR
This study demonstrates that the Polar WRF climate model can effectively assist in preliminary site assessment for astronomical observatories in Western Antarctica by simulating local atmospheric conditions.
Contribution
The paper applies the Polar WRF model to assess site suitability in Western Antarctica, showing its effectiveness in preliminary screening for observatory site selection.
Findings
Model accurately captures wind, temperature, and humidity variability.
Identifies zones of high winds and thermal inversions.
Model may underestimate cloud cover.
Abstract
The quality of ground based astronomical observations are significantly affected by telluric conditions, and the search for best sites has led to the construction of observatories at remote locations, including recent initiatives on the high plateaus of E Antarctica where the calm, dry and cloud free conditions during winter are recognized as amongst the best. Site selection is an important phase of any observatory development project, and candidate sites must be tested with specialized equipment, a process both time consuming and costly. A potential screening of site locations before embarking on field testing is through the use of climate models. Here, we describe the application of the Polar version of the Weather Research and Forecast (WRF) model to the preliminary site suitability assessment of an unstudied region in W Antarctica. Numerical simulations with WRF were carried out for…
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