Extrasolar Planet Science with the Antarctic Planet Interferometer

The primary limitation to ground based astronomy is the Earth’s atmosphere. The atmosphere above the Antarctic plateau is fundamentally different in many regards compared to the atmosphere at temperate sites. The extreme altitude, cold and low humidity offer a uniquely transparent atmosphere at many...

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Bibliographic Details
Main Authors: James P. Lloyd A, Ben F. Lane A, Mark R. Swain B, John W. Storey C, Tony Travouillon C, Wesley A. Traub D, Chris K. Walker E
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Subjects:
Atmospheric Turbulence
Extrasolar Planets
Interferometry
Antarctic
South Pole
The Antarctic
Antarc*
South pole
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.63.1103
http://www.phys.unsw.edu.au/~mgb/Antbib/apiturb.pdf
Description
Summary:The primary limitation to ground based astronomy is the Earth’s atmosphere. The atmosphere above the Antarctic plateau is fundamentally different in many regards compared to the atmosphere at temperate sites. The extreme altitude, cold and low humidity offer a uniquely transparent atmosphere at many wavelengths. Studies at the South Pole have shown additionally that the turbulence properties of the night time polar atmosphere are unlike any mid latitude sites. Despite relatively strong ground layer turbulence, the lack of high altitude turbulence combined with low wind speeds presents favorable conditions for interferometry. The unique properties of the polar atmosphere can be exploited for Extrasolar Planet studies with differential astrometry, differential phase and nulling interferometers. This paper combines the available data on the properties of the atmosphere at the South Pole and other Antarctic plateau sites for Extrasolar Planet science with interferometry.

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