Airglow and Aurorae at Dome A, Antarctica
文献类型:期刊论文
作者 | Sims, Geoff1; Ashley, Michael C. B.1; Cui, Xiangqun2; Everett, Jon R.1,4,5; Feng, LongLong3; Gong, Xuefei2; Hengst, Shane1; Hu, Zhongwen2; Lawrence, Jon S.; Luong-Van, Daniel M.1 |
刊名 | PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC |
出版日期 | 2012-06-01 |
卷号 | 124期号:916页码:637-649 |
ISSN号 | 0004-6280 |
英文摘要 | Despite the absence of artificial light pollution at Antarctic plateau sites such as Dome A, other factors such as airglow, aurorae, and extended periods of twilight have the potential to adversely affect optical observations. We present a statistical analysis of the airglow and aurorae at Dome A using spectroscopic data from Nigel, an optical/near-IR spectrometer operating in the 300-850 nm range. These data complement photometric images from Gattini, a wide-field (90 degrees) CCD camera with B, V, and R filters, allowing the background sky brightness to be disentangled from the various airglow and auroral emission lines. The median auroral contribution to the B, V, and R photometric bands is found to be 22.9, 23.4, and 23.0 mag arcsec(-2), respectively. Auroral emissions most frequently occur between 10-23 hr local time, when up to 50% of observations are above airglow-level intensities. While infrequent, the strongest emissions detected occurred in the hours just prior to magnetic midnight. We are also able to quantify the amount of annual dark time available as a function of wavelength, as well as in the standard BV R photometric bands. On average, twilight ends when the Sun reaches a zenith distance of 102.6 degrees. |
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] | MEDIUM INTENSITY AURORA ; CAP ABSORPTION EVENTS ; 558 NM EMISSION ; SKY BRIGHTNESS ; NIGHT-SKY ; QUANTITATIVE SPECTROSCOPY ; LOWER THERMOSPHERE ; MAGNETIC ACTIVITY ; SOLAR-CYCLE ; DYNAMICS |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000305839900013 |
公开日期 | 2013-01-31 |
源URL | [http://libir.pmo.ac.cn/handle/332002/8017] |
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.Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia 2.Nanjing Inst Astron Opt & Technol, Nanjing 210042, Jiangsu, Peoples R China 3.Acad Sinica, Purple Mt Observ, Nanjing 210008, Peoples R China 4.Macquarie Univ, Dept Phys & Astron, Sydney, NSW 2109, Australia 5.Australian Astron Observ, Sydney, NSW 1710, Australia 6.Caltech Opt Observ, Pasadena, CA 91125 USA 7.Tianjin Normal Univ, Tianjin 300074, Peoples R China 8.Univ Western Sydney, Sydney, NSW, Australia 9.Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA 10.Polar Res Inst China, Shanghai 200136, Peoples R China |
推荐引用方式 GB/T 7714 | Sims, Geoff,Ashley, Michael C. B.,Cui, Xiangqun,et al. Airglow and Aurorae at Dome A, Antarctica[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,2012,124(916):637-649. |
APA | Sims, Geoff.,Ashley, Michael C. B..,Cui, Xiangqun.,Everett, Jon R..,Feng, LongLong.,...&Zhu, Zhenxi.(2012).Airglow and Aurorae at Dome A, Antarctica.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,124(916),637-649. |
MLA | Sims, Geoff,et al."Airglow and Aurorae at Dome A, Antarctica".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 124.916(2012):637-649. |
入库方式: OAI收割
来源:紫金山天文台
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