Antarctic Astronomy: from Infrared to Millimeter Wave

. The dry, cold, tenuous and stable air above the Antarctic plateau provides superb conditions for the conduct of many classes of astronomical observations. We review the rationale for undertaking photon astronomy from Antarctica, and the disciplines where telescopes are now operating at the Amundse...

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Bibliographic Details
Main Author: Burton Joint Australian
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Subjects:
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.27.3535
http://www.phys.unsw.edu.au/~mgb/Antbib/pasp97_mgb.ps.gz
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Summary:. The dry, cold, tenuous and stable air above the Antarctic plateau provides superb conditions for the conduct of many classes of astronomical observations. We review the rationale for undertaking photon astronomy from Antarctica, and the disciplines where telescopes are now operating at the Amundsen--Scott South Pole Station. 1. Introduction The Antarctic plateau provides unique conditions on the Earth for the conduct of observational astronomy. Simply stated, the air is thin, dry and cold and the weather stable, attributes all offering gains to the observational astronomer. These conditions are quite different to those experienced at Antarctic coastal locations, which are frequently subject to violent storms. The plateau is over 3,000m in elevation, rising up to 4,300m at Dome Argus. An average year-round temperature of-50 ffi C, falling to-90 ffi C at times, vastly reduces the thermal background in the near--IR. The precipitable water vapour content of the air is typically ar.