High-resolution Observations of an X-1.0 White-light Flare with Moving Flare Ribbons
文献类型：期刊论文
| 作者 | Yang, Xu5; Wang, Meiqi6; Cao, Andrew1; Ji KF(季凯帆)2 ; Yurchyshyn, Vasyl5; Qiu, Jiong4; Yu, Sijie6; Shen, Jinhua3; Cao, Wenda5,6
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| 刊名 | ASTROPHYSICAL JOURNAL LETTERS
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| 出版日期 | 2025-02-01 |
| 卷号 | 979期号:2 |
| ISSN号 | 2041-8205 |
| DOI | 10.3847/2041-8213/ada9e4 |
| 产权排序 | 第4完成单位 |
| 文献子类 | Article |
| 英文摘要 | We analyze high-resolution observations of an X-1.0 white-light flare, triggered by a filament eruption, on 2022 October 2. The full process of filament formation and subsequent eruption was captured in the H alpha passband by the Visible Imaging Spectrograph (VIS) on board the Goode Solar Telescope (GST) within its center field of view. White-light emissions appear in flare ribbons following the filament eruption and H alpha ribbon brightening. GST Broadband Filter Imager data show that the continuum intensity, as compared to the nearby quiet-Sun area, has increased by up to 20% in the photospheric TiO band around 7057 & Aring;. The Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory reported 10% contrast enhancement in the continuum near Fe i 6173 & Aring; line. The separation motion of two white-light kernels is recorded by the high-cadence GST/TiO images and is well accompanied by the motion of the VIS H alpha flare ribbon leading edge. One kernel, located in a 150 Gauss field within a granulation area, exhibited an average apparent motion speed of 55 km s-1, which is the highest average speed ever reported. The other kernel drifted at 9 km s-1 in an 800 Gauss magnetic field area. Hard X-ray (HXR) emissions reaching up to 300 keV have been observed for this flare. The simultaneous occurrence of high-cadence HXR, microwave, and white-light emissions strongly suggests that the energetic particles from the flare directly contribute to the heating. The inverted HXR energy flux density corresponding to 10% TiO brightening is 2.07 +/- 0.23 x 1011 erg cm-2 s-1 during the flare peak. |
| 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 |
| WOS关键词 | SOLAR-FLARES ; EMISSION ; TELESCOPE ; ELECTRON ; RECONNECTION ; IONIZATION ; TRANSIENT ; CONTINUUM ; HYDROGEN ; FIELDS |
| 资助项目 | NSF divided by GEO divided by Division of Atmospheric and Geospace Sciences (AGS)https://doi.org/10.13039/100000159[AGS-2309939]; US NSF; New Jersey Institute of Technology (NJIT); Korea Astronomy and Space Science Institute; Seoul National University[AST-2407849]; Seoul National University[AGS-2401228]; NSF |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:001408887800001 |
| 出版者 | IOP Publishing Ltd |
| 资助机构 | NSF divided by GEO divided by Division of Atmospheric and Geospace Sciences (AGS)https://doi.org/10.13039/100000159[AGS-2309939] ; US NSF ; New Jersey Institute of Technology (NJIT) ; Korea Astronomy and Space Science Institute ; Seoul National University[AST-2407849, AGS-2401228] ; NSF |
| 版本 | 出版稿 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/28069]  |
| 专题 | 天文技术实验室 |
| 作者单位 | 1.Union County Vocational-Technical Schools, 1776 Raritan Rd., Scotch Plains, NJ 07076, USA; 2.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Kunming, Yunnan 650011, People's Republic of China; 3.Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150 Science 1-Street, Urumqi, Xinjiang 830011, People's Republic of China 4.Department of Physics, Montana State University, Bozeman, MT 59717, USA; 5.Big Bear Solar Observatory, 40386 N Shore Ln., Big Bear, CA 92314, USA; Xu.Yang@njit.edu, wenda.cao@njit.edu; 6.Center for Solar-Terrestrial Research, New Jersey Institute of Technology, 323 Martin Luther King Jr Blvd., Newark, NJ 07102-1982, USA; |
| 推荐引用方式 GB/T 7714 | Yang, Xu,Wang, Meiqi,Cao, Andrew,et al. High-resolution Observations of an X-1.0 White-light Flare with Moving Flare Ribbons[J]. ASTROPHYSICAL JOURNAL LETTERS,2025,979(2). |
| APA | Yang, Xu.,Wang, Meiqi.,Cao, Andrew.,季凯帆.,Yurchyshyn, Vasyl.,...&Cao, Wenda.(2025).High-resolution Observations of an X-1.0 White-light Flare with Moving Flare Ribbons.ASTROPHYSICAL JOURNAL LETTERS,979(2). |
| MLA | Yang, Xu,et al."High-resolution Observations of an X-1.0 White-light Flare with Moving Flare Ribbons".ASTROPHYSICAL JOURNAL LETTERS 979.2(2025). |
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来源：云南天文台
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