An episode of extremely low precipitable water vapour over Paranal observatory

被引:28
|
作者
Kerber, F. [1 ]
Querel, R. R. [2 ,3 ]
Rondanelli, R. [4 ,5 ]
Hanuschik, R. [1 ]
van den Ancker, M. [1 ]
Cuevas, O. [6 ]
Smette, A. [7 ]
Smoker, J. [7 ]
Rose, T. [8 ]
Czekala, H. [8 ]
机构
[1] ESO, Karl Schwarzschild Str 2, D-85748 Garching, Germany
[2] Univ Chile, Dept Ingn Elect, Santiago, Chile
[3] Natl Inst Water & Atmospher Res NIWA, Lauder, New Zealand
[4] Univ Chile, Dept Geofis, Santiago, Chile
[5] Ctr Climate & Resilience Res CR2, Santiago, Chile
[6] Univ Valparaiso, Dept Fis & Astron, Valparaiso, Chile
[7] ESO, Santiago, Chile
[8] Radiometer Phys GmbH, D-53340 Meckenheim, Germany
关键词
atmospheric effects; methods observational; site testing; infrared: general; SITE; ANTARCTICA; RADIOMETER; TELESCOPE; ESO;
D O I
10.1093/mnras/stt2404
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on an episode of extremely low precipitable water vapour (PWV) of approximately 0.1mm with a duration of more than 12 h at European Southern Observatory's Paranal observatory [2635m above sea level (asl)]. Such conditions are more commonly expected at sites at much higher altitude such as ALMA on the Chajnantor plateau (5000m asl) or otherwise particularly dry sites such as locations in Antarctica. We provide a full account of the measurements of PWV and other relevant atmospheric parameters. An explanation of the observed conditions is given in terms of the prevailing meteorological pattern. Based on statistical evidence from measurements by VLT spectrographs (UVES and CRIRES) covering more than a decade, we find that PWV < 0.2mm can be expected on less than 1 per cent of the nights, while < 0.5mm is encountered on 6-7 nights per year (approximate to 2 per cent). The scientific potential of using this small but significant fraction of observing time is illustrated in the context of service mode observing.
引用
收藏
页码:247 / 255
页数:9
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