Measurement of submillimeter zenith atmospheric opacity at 492 GHz
文献类型：期刊论文
| 作者 | Yang, J ; Sun, CH; Huang, SP; Ohishi, M; Miyazawa, K
|
| 刊名 | CHINESE ASTRONOMY AND ASTROPHYSICS
 |
| 出版日期 | 2004-07-01 |
| 卷号 | 28期号:3页码:367-376 |
| ISSN号 | 0275-1062 |
| 关键词 | submillimeter wave atmospheric opacity site selecting |
| 英文摘要 | Presented 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. |
| 学科主题 | Astronomy & Astrophysics |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | SOUTH-POLE ; MILLIMETER |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000223946500013 |
| 公开日期 | 2012-12-22 |
| 源URL | [http://libir.pmo.ac.cn/handle/332002/7699]  |
| 专题 | 紫金山天文台_分子云与恒星形成研究团组 |
| 作者单位 | 1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China 2.NAOJ, Nobeyama Radio Observ, Nagano 3841503, Japan |
| 推荐引用方式 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. |
入库方式： OAI收割
来源：紫金山天文台
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