Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-27T00:47:09.424Z Has data issue: false hasContentIssue false
  • English
  • Français

Extremely Large Telescopes on the Antarctic plateau

Published online by Cambridge University Press:  30 March 2016

J.S. Lawrence
J.S. Lawrence*
Affiliation:
School of Physics, University of New South Wales, NSW 2052, Australia

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The primary limitation to the performance of any large ground-based telescope is the atmospheric properties of its site, particularly the sky emission and the turbulence structure. There are several sites on the Antarctic plateau (South Pole, Dome C and Dome A) for which the increase in infrared sensitivity relative to a mid-latitude site should be as much as two orders of magnitude. The unique turbulent structure above Dome C indicates that an extremely large telescope equipped with only a natural guide star adaptive optics system should achieve equivalent resolution to a mid-latitude extremely large telescope with a multi-conjugate multi-laser guide star system.

Type
II. Special Scientific Sessions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 956 - 957
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Aristidi, E., Agabi, E., Vernin, J., Azouit, M., Martin, F., Ziad, A., and Fossat, E. 2003, A&A, 406, L19 Google Scholar
Chamberlain, R. A. 2001 J. Geophys. Research, 106, 20101 Google Scholar
Phillips, A., Burton, M.G., Ashley, M.C.B., Storey, J.W.V., Llyod, J.P., Harper, D.A., and Bally, J. 1999, AJ, 527, 1009 Google Scholar
Travouillon, et al. A&A, 400, 1163 Google Scholar