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Last name: TRAVOUILLON
First name: T.
SF2A-2005 : Semaine de l'Astrophysique Française, n/a, (2005)
Wide Field Survey Telecopes on Dome C/A, Antarctica, Proceedings of Acta Astronomica Sinica n/a, (2005)
Astron. & Astrophys., 444, pp. 651-659 (2005)
n/a, EAS Publications Series 14, pp. 227-232 (2005)
Dome C Astronomy/Astrophysics meeting, n/a, (2004)
n/a, EAS Publications Series 14, pp. 227-232 (2005)
n/a, eds. M. Giard, F. Casoli and F. Paletou, EAS Publications Series 14, pp. 13-18 (2005). http://dx.doi.org/10.1051/eas:2005004
Dome C Astronomy/Astrophysics meeting, EAS Publications Series 14, p. 13 (2004)
The optical turbulence above Dome C in winter is mainly concentrated in the first tens of meters above the ground. The properties of this so-called surface layer were investigated during the last two winterover by a set of sonics anemometers placed on a 45 m high tower. These anemometers provide measurements of the temperature and the wind...
The ground layer turbulence at Dome C is the cause for more than 90% of the total turbulence column. While the height of this layer has been currently measured to be approximately 30m, no long term statistics is available from this part of the atmosphere. In order to plan the construction of future telescope at this site temperature site,...
Astron. & Astrophys., 430, pp. 739-746 (2005)
The optical turbulence above Dome C in winter is mainly concentrated in the first tens of metres above the ground. Properties of this so-called surface layer (SL) were investigated during the period 2007–2012 by a set of sonic anemometers placed on a 45 m high tower. We present the results of this long-term monitoring of the refractive index...
The Gattini-DomeC project, part of the IRAIT site testing campaign and ongoing since January 2006, consists of two cameras for the measurement of optical sky brightness, large area cloud cover, and auroral detection above the DomeC site, home of the French-Italian Concordia station. The cameras are transit in nature and are virtually identical...
The Gattini cameras are two site testing instruments for the measurement of optical sky brightness, large area cloud cover and auroral detection of the night sky above the high altitude Dome C site in Antarctica. The cameras have been operating since installation in January 2006 and are currently at the end of the first Antarctic winter season....