Atmospheric scintillation at Dome C

Dome C, Antarctica is one of the most promising astronomical sites in the world (Fossat & Candidi 2003, and references therein). Dome C boasts low wind speeds, very cold temperatures and little precipitation. The atmospheric turbulence is very weak compared to temperate sites, leading to sub-arc...

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Main Authors: Suzanne L. Kenyon, Jon S. Lawrence, Michael C. B. Ashley, John W. V. Storey, Andrei Tokovinin, Eric Fossat
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
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Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.157.6383
http://www.phys.unsw.edu.au/~mcba/pubs/kenyon07a.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.157.6383 2023-05-15T13:40:39+02:00 Atmospheric scintillation at Dome C Suzanne L. Kenyon Jon S. Lawrence Michael C. B. Ashley John W. V. Storey Andrei Tokovinin Eric Fossat The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.157.6383 http://www.phys.unsw.edu.au/~mcba/pubs/kenyon07a.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.157.6383 http://www.phys.unsw.edu.au/~mcba/pubs/kenyon07a.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.phys.unsw.edu.au/~mcba/pubs/kenyon07a.pdf text ftciteseerx 2016-01-07T15:33:35Z Dome C, Antarctica is one of the most promising astronomical sites in the world (Fossat & Candidi 2003, and references therein). Dome C boasts low wind speeds, very cold temperatures and little precipitation. The atmospheric turbulence is very weak compared to temperate sites, leading to sub-arcsecond seeing conditions (Lawrence et al. 2004; Text Antarc* Antarctica Unknown
institution Open Polar
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description Dome C, Antarctica is one of the most promising astronomical sites in the world (Fossat & Candidi 2003, and references therein). Dome C boasts low wind speeds, very cold temperatures and little precipitation. The atmospheric turbulence is very weak compared to temperate sites, leading to sub-arcsecond seeing conditions (Lawrence et al. 2004;
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author Suzanne L. Kenyon
Jon S. Lawrence
Michael C. B. Ashley
John W. V. Storey
Andrei Tokovinin
Eric Fossat
spellingShingle Suzanne L. Kenyon
Jon S. Lawrence
Michael C. B. Ashley
John W. V. Storey
Andrei Tokovinin
Eric Fossat
Atmospheric scintillation at Dome C
author_facet Suzanne L. Kenyon
Jon S. Lawrence
Michael C. B. Ashley
John W. V. Storey
Andrei Tokovinin
Eric Fossat
author_sort Suzanne L. Kenyon
title Atmospheric scintillation at Dome C
title_short Atmospheric scintillation at Dome C
title_full Atmospheric scintillation at Dome C
title_fullStr Atmospheric scintillation at Dome C
title_full_unstemmed Atmospheric scintillation at Dome C
title_sort atmospheric scintillation at dome c
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.157.6383
http://www.phys.unsw.edu.au/~mcba/pubs/kenyon07a.pdf
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source http://www.phys.unsw.edu.au/~mcba/pubs/kenyon07a.pdf
op_relation http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.157.6383
http://www.phys.unsw.edu.au/~mcba/pubs/kenyon07a.pdf
op_rights Metadata may be used without restrictions as long as the oai identifier remains attached to it.
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