The water vapour radiometer of Paranal: homogeneity of precipitable water vapour from two years of operations

Adapting to the Atmosphere Conference 2014

物理学;地球科学

Kerber, Florian^1 ; Querel, Richard R.^2 ; Neureiter, Bianca^3

European Southern Observatory, Karl-Schwarzschild-Str. 2, Garching

85748, Germany^1

National Institute of Water and Atmospheric Research (NIWA), Lauder, New Zealand^2

Ludwig-Maximilians-Universität, Geschwister-Scholl-Platz 1, München

80539, Germany^3

关键词: Astronomical data;    Climate studies;    Infra-red cameras;    Microwave radiometers;    Mode of operations;    Precipitable water vapour;    Science operations;    Temporal and spatial;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/595/1/012017/pdf
DOI  :  10.1088/1742-6596/595/1/012017

来源: IOP

【 摘 要 】

A Low Humidity and Temperature Profiling (LHATPRO) microwave radiometer, manufactured by Radiometer Physics GmbH (RPG), is used to monitor sky conditions over ESO's Paranal observatory in support of VLT science operations. The unit measures several channels across the strong water vapour emission line at 183 GHz, necessary for resolving the low levels of precipitable water vapour (PWV) that are prevalent on Paranal (median ∼2.4 mm). The instrument consists of a humidity profiler (183-191 GHz), a temperature profiler (51-58 GHz), and an infrared camera (∼10 μm) for cloud detection. We present a statistical analysis of the homogeneity of all-sky PWV using 24 months of PWV observations. The question we tried to address was whether PWV is homogeneous enough across the sky such that service mode observations with the VLT can routinely be conducted with a user-provided constraint for PWV measured at zenith. We find the PWV over Paranal to be remarkably homogeneous across the sky down to 27.5° elevation with a median variation of 0.07 mm (rms). The homogeneity is a function of the absolute PWV but the relative variation is fairly constant at 2 to 3% (rms). Such variations will not be a significant issue for analysis of astronomical data. Users at ESO can specify PWV - measured at zenith - as an ambient constraint in service mode to enable, for instance, very demanding observations in the infrared. We conclude that in general it will not be necessary to add another observing constraint for PWV homogeneity to ensure integrity of observations. For demanding observations requiring very low PWV, where the relative variation is higher, the optimum support could be provided by observing with the LHATPRO in the same line-of-sight simultaneously. Such a mode of operations has already been tested but will have to be justified in terms of scientific gain before implementation can be considered. We plan to extend our analysis of PWV variations covering a larger parameters space for temporal and spatial resolution in the future. Also for climate studies such data sets will be relevant.