Forecasting precipitable water vapour at the Roque de los Muchachos Observatory
2010
Modern optical and infrared astronomical sites are getting used to a flexible way of operation, namely queue
modes, allowing astronomical observations in the most appropriate weather conditions for each specific observing
scientific program. The forecast of weather conditions is then a mandatory issue to plan in advance the
observations queue for each night in order to exploit efficiently the astronomical facilities with the largest high
quality data output for scientific exploitation. The precipitable water vapour is the parameter accounting for
the infrared (IR) quality of an astronomical site. The temporal fluctuation of this parameter drastically affects
the quality of the IR data recorded at ground telescopes. An optical/IR telescope needs the forecasting of the
precipitable water vapour for a proper queue scheduling of IR observations. The Roque de los Muchachos Observatory
(ORM) on the island of La Palma (Spain) presents an abrupt topography which difficult the forecasting
at this astronomical site. We discuss the performance of a mesoscale numerical weather model (WRF, Weather
Research and Forecasting) applied to ORM region including the comparison with local precipitable water vapour
estimations from GPS (Global Positioning System).
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