Automatic data analysis for the Sky Brightness Monitor
文献类型：期刊论文
| 作者 | Zhao MY(赵明宇)1 ; Liu Y(刘煜)1,2; Elmhamdi, A1,2; Kordi, AS2; Al-trabulsy, HA2; Zhang XF(张雪飞)1; Song TF(宋腾飞)1; Liu SQ(刘顺庆)1; Shen YD(申远灯)1; Tian ZJ(田占军)1
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| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| 出版日期 | 2014-09-21 |
| 卷号 | 443期号:3页码:1955-1966 |
| 关键词 | atmospheric effects methods: data analysis site testing telescopes surveys Sun: general |
| ISSN号 | 0035-8711 |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Zhao, MY (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China. |
| 英文摘要 | The Sky Brightness Monitor (SBM) is an important instrument for measuring the brightness level for the sky condition, which is a critical parameter when judging a site for solar coronal observations. In this paper, we present an automatic method for processing SBM data in large quantities. This method can separate the regions of the Sun and the nearby sky, as well as recognizing the regions of the supporting arms in the field of view. These processes are implemented on the data acquired by more than one SBM instrument during our site survey project in western China. Applying the result from our processes, an analysis has been carried out for the assessment of the scattered-light levels by the instrument. These results are considerably significant for further investigations and studies, notably to derive a series of other atmospheric parameters, such as extinctions, aerosol content and precipitable water vapour content, that are important for candidate sites. Our processes also provide a possible way for full-disc solar telescopes to track the Sun without an extra guiding system. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Astronomy & Astrophysics |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | TELESCOPE SITE SURVEY |
| 收录类别 | SCI |
| 原文出处 | http://mnras.oxfordjournals.org/content/443/3/1955 |
| 语种 | 英语 |
| WOS记录号 | WOS:000342920400008 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/7193]  |
| 专题 | 云南天文台_选址与日冕观测组 |
| 作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China 2.Department of Physics and Astronomy, King Saud University, PO Box 2455, Riyadh 11451, Saudi Arabia |
| 推荐引用方式 GB/T 7714 | Zhao MY,Liu Y,Elmhamdi, A,et al. Automatic data analysis for the Sky Brightness Monitor[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2014,443(3):1955-1966. |
| APA | Zhao MY.,Liu Y.,Elmhamdi, A.,Kordi, AS.,Al-trabulsy, HA.,...&Miao YH.(2014).Automatic data analysis for the Sky Brightness Monitor.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,443(3),1955-1966. |
| MLA | Zhao MY,et al."Automatic data analysis for the Sky Brightness Monitor".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 443.3(2014):1955-1966. |
入库方式： OAI收割
来源：云南天文台
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