Origin of the Chromospheric Umbral Waves in Sunspots | |
Zhang XS(张鑫生)1,2; Yan XL(闫晓理)1,3; Xue ZK(薛志科)1,3; Wang JC(王金成)1,3; Xu Z(徐喆)1,3; Li, Qiaoling4,5; Peng Y(彭洋)1,2; Yang LP(杨丽平)1,2 | |
发表期刊 | SOLAR PHYSICS |
2024-05 | |
卷号 | 299期号:5 |
DOI | 10.1007/s11207-024-02323-w |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Sunspots Chromosphere Oscillations Magnetohydrodynamics |
摘要 | Oscillations are ubiquitous in sunspots and the associated higher atmospheres. However, it is still unclear whether these oscillations are driven by the external acoustic waves (p-modes) or generated by the internal magnetoconvection. To obtain clues about the driving source of umbral waves in sunspots, we analyzed the spiral wave patterns (SWPs) in two sunspots registered by IRIS MgII 2796 & Aring; slit-jaw images. By tracking the motion of the SWPs, we found for the first time that two one-armed SWPs coexist in the umbra, and they can rotate either in the same or opposite directions. Furthermore, by analyzing the spatial distribution of the oscillation centers of the one-armed SWPs within the umbra (the oscillation center is defined as the location where the SWP first appears), we found that the chromospheric umbral waves repeatedly originate from the regions with high oscillation power and most of the umbral waves occur in the dark nuclei and strong magnetic field regions of the umbra. Our study results indicate that the chromospheric umbral waves are likely excited by the p-mode oscillations. |
资助项目 | Strategic Priority Research Program of the Chinese Academy of Sciences |
项目资助者 | Strategic Priority Research Program of the Chinese Academy of Sciences |
语种 | 英语 |
学科领域 | 天文学 ; 太阳与太阳系 |
文章类型 | Article |
出版者 | SPRINGER |
出版地 | VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS |
ISSN | 0038-0938 |
URL | 查看原文 |
WOS记录号 | WOS:001235325500003 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | P-MODE ABSORPTION ; MAGNETIC-FIELDS ; PENUMBRAL WAVES ; OSCILLATIONS ; SIMULATIONS ; GENERATION ; IMAGE |
引用统计 | |
文献类型 | 期刊论文 |
版本 | 出版稿 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/27346 |
专题 | 抚仙湖太阳观测和研究基地 光纤阵列太阳光学望远镜研究组 |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China; 2.University of Chinese Academy of Sciences, Beijing, 100049, China; 3.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming, 650216, China; 4.Department of Physics, Yunnan University, Kunming, 650091, China; 5.Department of Astronomy, Key Laboratory of Astroparticle Physics of Yunnan Province, Yunnan University, Kunming, 650091, China |
第一作者单位 | 中国科学院云南天文台 |
推荐引用方式 GB/T 7714 | Zhang XS,Yan XL,Xue ZK,et al. Origin of the Chromospheric Umbral Waves in Sunspots[J]. SOLAR PHYSICS,2024,299(5). |
APA | 张鑫生.,闫晓理.,薛志科.,王金成.,徐喆.,...&杨丽平.(2024).Origin of the Chromospheric Umbral Waves in Sunspots.SOLAR PHYSICS,299(5). |
MLA | 张鑫生,et al."Origin of the Chromospheric Umbral Waves in Sunspots".SOLAR PHYSICS 299.5(2024). |
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Origin of the Chromo(4435KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
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