Carrington Maps in H i Lyα and Their Relationships with Extreme-ultraviolet and Magnetic-field Maps | |
Li, Shuting3,4; Feng, Li3,4; Ying, Beili4; Lu, Lei4; Ji KF(季凯帆)2; Li, Ying3,4; Shi, Guanglu3,4; Li, Hui3,4; Huang, Yu3,4; Gan, Weiqun1,4 | |
刊名 | ASTROPHYSICAL JOURNAL LETTERS
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2024-07-01 | |
卷号 | 969期号:1 |
ISSN号 | 2041-8205 |
DOI | 10.3847/2041-8213/ad5679 |
产权排序 | 第3完成单位 |
文献子类 | Article |
英文摘要 | H i Ly alpha emission in the chromosphere and transition region is a key ingredient of the incident radiation to coronal neutral hydrogen for modeling corona Ly alpha emission. The Ly alpha emission distribution across the solar disk can be obtained from a Ly alpha Carrington map. Before the launch of the Advanced Space-based Solar Observatory (ASO-S), such a Ly alpha Carrington map was derived from the Carrington map at He ii 30.4 nm and sometimes is even assumed to be uniform. We construct the first Ly alpha Carrington map based on full-disk Ly alpha images acquired by the Solar Disk Imager (SDI) on board ASO-S and present two versions: the standard one is for a CR, and the other is daily updated. For modeling Ly alpha intensities during eruptions, the Carrington map with incorporated flare region is produced. Furthermore, we evaluate the difference between the Ly alpha Carrington map derived with SDI observations and that synthesized from the 30.4 nm data based on an empirical relationship between Ly alpha and He ii 30.4 nm intensities, particularly extended to flare intensities that have not been investigated before. The average difference of 38% proves the importance of the Ly alpha Carrington map built from observations directly. However, the synthetic Ly alpha Carrington map can be used as an approximation before SDI data are available. The comparison between the SDI Ly alpha Carrington map and the corresponding magnetic field synoptic map indicates that active regions in general are brighter in Ly alpha, while the sunspot umbras with strong magnetic field strength are usually weaker in Ly alpha. |
学科主题 | 天文学 ; 太阳与太阳系 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
资助项目 | Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560000]; National Key R&D Program of China[2022YFF0503003 (2022YFF0503000)]; NSFC[11973012]; NSFC[11921003]; NSFC[12233012]; NSFC[12203102]; NSFC[12103090]; NSFC[12373115]; Sino-German Science Center[M-0068] |
WOS关键词 | SOLAR TELESCOPE LST ; ASO-S MISSION ; DIFFERENTIAL EMISSION MEASURE ; LYMAN ; FLUX ; CORONAGRAPHS ; DIAGNOSTICS |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP Publishing Ltd |
WOS记录号 | WOS:001257892500001 |
资助机构 | Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560000] ; National Key R&D Program of China[2022YFF0503003 (2022YFF0503000)] ; NSFC[11973012, 11921003, 12233012, 12203102, 12103090, 12373115] ; Sino-German Science Center[M-0068] |
内容类型 | 期刊论文 |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/27432] ![]() |
专题 | 天文技术实验室 |
作者单位 | 1.University of Chinese Academy of Sciences, Nanjing 211135, People's Republic of China 2.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China; 3.School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, People's Republic of China; 4.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, People's Republic of China; lfeng@pmo.ac.cn; |
推荐引用方式 GB/T 7714 | Li, Shuting,Feng, Li,Ying, Beili,et al. Carrington Maps in H i Lyα and Their Relationships with Extreme-ultraviolet and Magnetic-field Maps[J]. ASTROPHYSICAL JOURNAL LETTERS,2024,969(1). |
APA | Li, Shuting.,Feng, Li.,Ying, Beili.,Lu, Lei.,季凯帆.,...&Gan, Weiqun.(2024).Carrington Maps in H i Lyα and Their Relationships with Extreme-ultraviolet and Magnetic-field Maps.ASTROPHYSICAL JOURNAL LETTERS,969(1). |
MLA | Li, Shuting,et al."Carrington Maps in H i Lyα and Their Relationships with Extreme-ultraviolet and Magnetic-field Maps".ASTROPHYSICAL JOURNAL LETTERS 969.1(2024). |
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