2014
DOI: 10.1086/678327
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Meteorological Data for the Astronomical Site at Dome A, Antarctica

Abstract: We present an analysis of the meteorological data collected at Dome A, Antarctica by the Kunlun Automated Weather Station, including temperatures and wind speeds at eight elevations above the snow surface between 0 m and 14.5 m. The average temperatures at 2 m and 14.5 m are −54 • C and −46 • C, respectively. We find that a strong temperature inversion existed at all heights for more than 70% of the time, and the temperature inversion typically lasts longer than 25 hours, indicating an extremely stable atmosph… Show more

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Cited by 64 publications
(25 citation statements)
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References 19 publications
(23 reference statements)
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“…The entire observatory is controlled remotely using the Iridium satellite system to transmit operational commands. Dome A is a site with the lowest temperature and the lowest absolute humidity on earth [34,36,37,38]. The weather conditions are suitable for taking data for over 95% of the time during the winter.…”
Section: Instrument Observations and Data Reductionmentioning
confidence: 99%
“…The entire observatory is controlled remotely using the Iridium satellite system to transmit operational commands. Dome A is a site with the lowest temperature and the lowest absolute humidity on earth [34,36,37,38]. The weather conditions are suitable for taking data for over 95% of the time during the winter.…”
Section: Instrument Observations and Data Reductionmentioning
confidence: 99%
“…The Antarctic plateau offers a number of unique advantages for precision, ground-based, time-domain as-tronomy, such as the ability to observe continuously during winter, low scintillation noise, excellent seeing above a very low boundary layer, low airmass variations, low aerosols, low water vapor, more stable atmospheric transmission, wider wavelength windows, and a dark sky in the infrared (Lawrence et al 2004(Lawrence et al , 2006(Lawrence et al , 2008Moore et al 2008;Kulesa et al 2008;Aristidi et al 2009;Burton 2010;Zou et al 2010;Yang et al 2010;Sims et al 2010;Bonner et al 2010;Lascaux et al 2011;Tremblin et al 2011;Pei et al 2011Pei et al , 2012Sims et al 2012a,b;Giordano et al 2012;Storey 2013;Hu et al 2014;Ashley 2013;Yang et al 2016). There is thus considerable interest in overcoming the technical challenges of operating in Antarctica, so that the advantages for astronomy can be realized (Tothill et al 2008;Kulesa et al 2008;Crouzet et al 2010;Chapellier et al 2016;Mékarnia et al 2016).…”
Section: Introductionmentioning
confidence: 99%
“…At Dome A, most of the turbulence integral is contributed by the GL. The wind velocity in this layer is typically quite small, having a yearly average of 3 − 5 m s −1 (Hu et al 2014(Hu et al , 2019. For the AST3 telescopes, and a wind speed of 5 m s −1 , the characteristic time is T0 = 0.3 s. From Fig.…”
Section: Resultsmentioning
confidence: 94%