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Measurement of submillimeter zenith atmospheric opacity at 492 GHz
Yang, J; Sun, CH; Huang, SP; Ohishi, M; Miyazawa, K
2004-07-01
Source PublicationCHINESE ASTRONOMY AND ASTROPHYSICS
ISSN0275-1062
Volume28Issue:3Pages:367-376
AbstractPresented are measurements of the zenith opacity (tau(0)) of the earth's atmosphere at 492 GHz made with the Portable Submillimeter Telescope (POST) at the observing station (elevation 3200 meters) located in the Qinghai-Tibet Plateau and belonging to Purple Mountain Observatory. The measurement spanned about 870 hours in the two winter seasons of 1999-2000 and 2000-2001, and resulted in 25842 sets of tau(0) values. The measured values of tau(0) are mainly distributed between 1.5 and 3.0, and about 3 percent of the total observing time had tau(0) less than or equal to1.0. A preliminary comparison is made with data obtained at other available submillimeter observing sites in the world.
KeywordSubmillimeter Wave Atmospheric Opacity Site Selecting
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1016/j.chinastron.2004.07.012
WOS KeywordSOUTH-POLE ; MILLIMETER
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000223946500013
Citation statistics
Cited Times:2[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/7699
Collection分子云与恒星形成研究团组
Affiliation1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
2.NAOJ, Nobeyama Radio Observ, Nagano 3841503, Japan
Recommended Citation
GB/T 7714
Yang, J,Sun, CH,Huang, SP,et al. Measurement of submillimeter zenith atmospheric opacity at 492 GHz[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2004,28(3):367-376.
APA Yang, J,Sun, CH,Huang, SP,Ohishi, M,&Miyazawa, K.(2004).Measurement of submillimeter zenith atmospheric opacity at 492 GHz.CHINESE ASTRONOMY AND ASTROPHYSICS,28(3),367-376.
MLA Yang, J,et al."Measurement of submillimeter zenith atmospheric opacity at 492 GHz".CHINESE ASTRONOMY AND ASTROPHYSICS 28.3(2004):367-376.
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