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Proceedings Paper

Site evaluations of the summit of Co. Chajnantor for infrared observations
Author(s): Takashi Miyata; Kentaro Motohara; Shigeyuki Sako; Masuo Tanaka; Takeo Minezaki; Natsuko Mitani; Tsutomu Aoki; Takao Soyano; Toshihiko Tanabe; Kimiaki Kawara; Kotaro Kohno; Ken'ichi Tarusawa; Toshihiko Handa; Mamoru Doi; Yuzuru Yoshii; Hajime Ezawa; Leonardo Bronfman; Maria T. Ruiz
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Paper Abstract

Because of the high transparency in infrared wavelength, Co. Chajnantor (5,650m altitude) at Atacama, Chile, is one of the most promising sites for infrared astronomy in the world. For evaluating the site condition quantitatively we carried out weather and cloud emissivity monitoring campaign from April 2006 to April 2007. The ground-level condition such as wind direction, wind speed, air temperature, and humidity was monitored by a weather station installed at the summit. Cloud emissivity was estimated by mid-infrared sky images taken by a whole-sky infrared camera every five minutes for 24 hours a day, every day. Results are summarized as followings. 1) The weather condition at the summit is slightly harsher than the condition at the Pampa la Bola plateau. Maximum speed of the wind is 35m/s, and minimum temperature is about -10 degree. 2) Fraction of "clear+usable" weather (which is defined as the cloud emissivity < 10%)" is 82% in a year. The fraction decrease to 40-50% on Bolivian winter season, and increases to over 90% from April to July. This is comparable or even better than the other astronomical sites.

Paper Details

Date Published: 10 July 2008
PDF: 8 pages
Proc. SPIE 7012, Ground-based and Airborne Telescopes II, 701243 (10 July 2008); doi: 10.1117/12.788264
Show Author Affiliations
Takashi Miyata, Institute of Astronomy, The Univ. of Tokyo (Japan)
Kentaro Motohara, Institute of Astronomy, The Univ. of Tokyo (Japan)
Shigeyuki Sako, Institute of Astronomy, The Univ. of Tokyo (Japan)
Masuo Tanaka, Institute of Astronomy, The Univ. of Tokyo (Japan)
Takeo Minezaki, Institute of Astronomy, The Univ. of Tokyo (Japan)
Natsuko Mitani, Institute of Astronomy, The Univ. of Tokyo (Japan)
Tsutomu Aoki, Kiso Observatory, Institute of Astronomy, The Univ. of Tokyo (Japan)
Takao Soyano, Kiso Observatory, Institute of Astronomy, The Univ. of Tokyo (Japan)
Toshihiko Tanabe, Institute of Astronomy, The Univ. of Tokyo (Japan)
Kimiaki Kawara, Institute of Astronomy, The Univ. of Tokyo (Japan)
Kotaro Kohno, Institute of Astronomy, The Univ. of Tokyo (Japan)
Ken'ichi Tarusawa, Kiso Observatory, Institute of Astronomy, The Univ. of Tokyo (Japan)
Toshihiko Handa, Institute of Astronomy, The Univ. of Tokyo (Japan)
Mamoru Doi, Institute of Astronomy, The Univ. of Tokyo (Japan)
Yuzuru Yoshii, Institute of Astronomy, The Univ. of Tokyo (Japan)
Hajime Ezawa, National Astronomical Observatory of Japan (Japan)
Leonardo Bronfman, Univ. of Chile (Chile)
Maria T. Ruiz, Univ. of Chile (Chile)


Published in SPIE Proceedings Vol. 7012:
Ground-based and Airborne Telescopes II
Larry M. Stepp; Roberto Gilmozzi, Editor(s)

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