中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。