Location of energy source for coronal heating on the photosphere
文献类型：期刊论文
| 作者 | Hong, Zhen-Xiang1,2; Yang, Xu3; Wang, Ya1,2; Ji KF(季凯帆)4 ; Ji, Hai-Sheng2,3; Cao, Wen-Da2,3
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| 刊名 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS
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| 出版日期 | 2017-02-01 |
| 卷号 | 17期号:3 |
| 关键词 | Sun: atmosphere Sun: photosphere Sun: transition region Sun: corona |
| ISSN号 | 1674-4527 |
| 产权排序 | 第4完成单位 |
| 通讯作者 | Hong, Zhen-Xiang(Univ Chinese Acad Sci CAS, Beijing 100049, Peoples R China) |
| 英文摘要 | It is reported that ultra-fine dynamic ejections along magnetic loops of an active region originate from intergranular lanes and they are associated with subsequent heating in the corona. As continuing work, we analyze the same set of data but focus on a quiet region and the overlying EUV/UV emission as observed by the Atmospheric Imaging Assembly (AIA) on board Solar Dynamics Observatory (SDO). We find that there appear to be dark patches scattered across the quiet region and the dark patches always stay along intergranular lanes. Over the dark patches, the average UV/EUV emission at 131, 171, 304 and 1600 angstrom (middle temperature) is more intense than that of other regions and EUV brightness is negatively correlated with 10830 angstrom intensity, though, such a trend does not exist for high temperature lines at 94, 193, 211 and 335 angstrom. For the same quiet region, where both TiO 7057 angstrom broad band images and 10830 angstrom filtergrams are available, contours for the darkest lane areas on TiO images and dark patches on 10830 angstrom filtergrams frequently differ in space. The results suggest that the dark patches do not simply reflect the areas with the darkest lanes but are associated with a kind of enhanced absorption (EA) at 10830 angstrom. A strict definition for EA with narrow band 10830 angstrom filtergrams is found to be difficult. In this paper, we define enhanced absorption patches (EAPs) of a quiet region as the areas where emission is less than similar to 90% of the mean intensity of the region. The value is equivalent to the average intensity along thin dark loops connecting two moss regions of the active region. A more strict definition for EAPs, say 88%, gives even more intense UV/EUV emission over those in the middle temperature range. The results provide further observational evidence that energy for heating the upper solar atmosphere comes from the intergranular lane area where the magnetic field is constantly brought in by convection motion in granules. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | 天文学 |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | FAST SOLAR-WIND ; ALFVENIC WAVES ; HELIUM ; REGION ; POWER |
| 收录类别 | SCI |
| 原文出处 | http://stacks.iop.org/1674-4527/17/i=3/a=25?key=crossref.192d153dbec2c2818cec6f76343b34fa |
| 语种 | 英语 |
| WOS记录号 | WOS:000397210100004 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/9996]  |
| 专题 | 天文技术实验室 |
| 作者单位 | 1.University of Chinese Academy of Sciences (CAS), Beijing 100049, China 2.Key Laboratory of DMSA, Purple Mountain Observatory, CAS, Nanjing 210008, China 3.Big Bear Solar Observatory, NJIT, 40386 North Shore Dr, Big Bear City, CA 92314, USA 4.Yunnan Observatories, CAS, Kunming 650011, China |
| 推荐引用方式 GB/T 7714 | Hong, Zhen-Xiang,Yang, Xu,Wang, Ya,et al. Location of energy source for coronal heating on the photosphere[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2017,17(3). |
| APA | Hong, Zhen-Xiang,Yang, Xu,Wang, Ya,Ji KF,Ji, Hai-Sheng,&Cao, Wen-Da.(2017).Location of energy source for coronal heating on the photosphere.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,17(3). |
| MLA | Hong, Zhen-Xiang,et al."Location of energy source for coronal heating on the photosphere".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 17.3(2017). |
入库方式： OAI收割
来源：云南天文台
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