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The Lyman-alpha Solar Telescope (LST) for the ASO-S mission - I. Scientific objectives and overview

文献类型:期刊论文

作者Li, Hui5,6; Chen, Bo4; Feng, Li5,6; Li, Ying5,6; Huang, Yu5,6; Li, Jing-Wei5,6; Lu, Lei5,6; Xue, Jian-Chao5,6; Ying, Bei-Li5,6; Zhao, Jie5,6
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2019-11-01
卷号19期号:11页码:10
ISSN号1674-4527
关键词Sun: flares Sun: coronal mass ejections (CMEs) Sun: filaments, prominences Sun: corona Sun: chromosphere Sun: UV radiation
DOI10.1088/1674-4527/19/11/158
通讯作者Li, Hui(nj.lihui@pmo.ac.cn)
英文摘要As one of the payloads for the Advanced Space-based Solar Observatory (ASO-S) mission, the Lyman-alpha (Ly alpha) Solar Telescope (LST) is aimed at imaging the Sun and the inner corona up to 2.5 R-circle dot (mean solar radius) in both the Ly alpha (121.6 nm) and visible wavebands with high temporo-spatial resolution, mainly targeting solar flares, coronal mass ejections (CMEs) and filaments/prominences. LST observations allow us to trace solar eruptive phenomena from the disk center to the inner corona, to study the relationships between eruptive prominences/filaments, solar flares and CMEs, to explore the dynamical processes and evolution of solar eruptions, to diagnose solar winds, and to derive physical parameters of the solar atmosphere. LST is actually an instrument suite, which consists of a Solar Disk Imager (SDI), a Solar Corona Imager (SCI), aWhite-light Solar Telescope (WST) and two Guide Telescopes (GTs). This is the first paper in a series of LST-related papers. In this paper, we introduce the scientific objectives, present an overview of the LST payload and describe the planned observations. The detailed design and data along with potential diagnostics are described in the second (Paper II) and third (Paper III) papers, respectively, appearing in this issue.
WOS关键词CORONAL MASS EJECTION ; WHITE-LIGHT FLARE ; CONTINUUM EMISSION ; ACCELERATION ; MODEL
WOS研究方向Astronomy & Astrophysics
语种英语
出版者NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
WOS记录号WOS:000507468400004
源URL[http://libir.pmo.ac.cn/handle/332002/35436]  
专题中国科学院紫金山天文台
通讯作者Li, Hui
作者单位1.Chinese Acad Sci, Innovat Acad Microsatellites, Shanghai 201210, Peoples R China
2.Chinese Acad Sci, Xian Inst Opt & Precis Mech, Xian 710119, Peoples R China
3.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Peoples R China
4.Chinese Acad Sci, Changchun Inst Opt Fine Mech & Phys, Changchun 130033, Peoples R China
5.Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China
6.Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 20034, Peoples R China
推荐引用方式
GB/T 7714
Li, Hui,Chen, Bo,Feng, Li,et al. The Lyman-alpha Solar Telescope (LST) for the ASO-S mission - I. Scientific objectives and overview[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2019,19(11):10.
APA Li, Hui.,Chen, Bo.,Feng, Li.,Li, Ying.,Huang, Yu.,...&Yang, Zhong-Guang.(2019).The Lyman-alpha Solar Telescope (LST) for the ASO-S mission - I. Scientific objectives and overview.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,19(11),10.
MLA Li, Hui,et al."The Lyman-alpha Solar Telescope (LST) for the ASO-S mission - I. Scientific objectives and overview".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 19.11(2019):10.

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