OBSERVATIONS OF EUV RECURRING JETS IN AN ACTIVE REGION CONFINED BY CORONAL LOOPS | |
Zheng YF(郑艳芳)1,2; Wang, F3; Ji, KF3; Deng, H3 | |
刊名 | JOURNAL OF THE KOREAN ASTRONOMICAL SOCIETY |
2013-10-31 | |
卷号 | 46期号:5页码:183-190 |
关键词 | Sun: jets Sun: filament Sun: magnetic fields Sun: coronal loops |
ISSN号 | 1225-4614 |
通讯作者 | Zheng, YF (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Natl Astron Observ, POB 110, Kunming 650011, Peoples R China. |
产权排序 | 第一完成单位 |
英文摘要 | Recurring jets, which are jets ejected from the same site, are a peculiar type among various solar jet phenomena. We report such recurring jets ejecting from the same site above an active region on January 22, 2012 with high-resolution multi-wavelength observations from Solar Dynamics Observatory(SDO). We found that the recurring jets had velocities, lengths and lifetimes, but had similar directions. The visible brightening appeared at the jet base before each jet erupted. All the plasma produced by the recurring jets could not overcome the large coronal loops. It seemed that the plasma ejecting from the jet base was confined and guided by preexisting coronal loops, but their directions were not along the paths of the loops. Two of the jets formed crossing structures with the same preexisting filament. We also examined the photospheric magnetic field at the jet base, and observed a visible flux emergence, convergence and cancellation. The four recurring jets all were associated with the impulsive cancellation between two opposite polarities occurring at the jet base during each eruption. In addition, we suggest that the fluxes, flowing out of the active region, might supply the energy for the recurring jets by examining the SDO/Helioseismic and Magnetic Imager (HMI) successive images. The observational results support the magnetic reconnection model of jets. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | X-RAY JETS ; H-ALPHA SURGES ; TELESCOPE |
收录类别 | SCI |
原文出处 | http://koreascience.or.kr/article/ArticleFullRecord.jsp?cn=CMHHBA_2013_v46n5_183 |
语种 | 英语 |
WOS记录号 | WOS:000326661000001 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/4690] |
专题 | 云南天文台_抚仙湖太阳观测站 |
作者单位 | 1.National Astronomical Observatories, Yunnan Astronomical Observatory, Chinese Academy of Sciences, P. O. Box 110, 650011, Kunming, China 2.University of Chinese Academy of Sciences, Beijing 100049, China 3.Computer Technology Application Key Lab of Yunnan Province, Kunming University of Science and Technology, Kunming, Yunnan 650500, China |
推荐引用方式 GB/T 7714 | Zheng YF,Wang, F,Ji, KF,et al. OBSERVATIONS OF EUV RECURRING JETS IN AN ACTIVE REGION CONFINED BY CORONAL LOOPS[J]. JOURNAL OF THE KOREAN ASTRONOMICAL SOCIETY,2013,46(5):183-190. |
APA | Zheng YF,Wang, F,Ji, KF,&Deng, H.(2013).OBSERVATIONS OF EUV RECURRING JETS IN AN ACTIVE REGION CONFINED BY CORONAL LOOPS.JOURNAL OF THE KOREAN ASTRONOMICAL SOCIETY,46(5),183-190. |
MLA | Zheng YF,et al."OBSERVATIONS OF EUV RECURRING JETS IN AN ACTIVE REGION CONFINED BY CORONAL LOOPS".JOURNAL OF THE KOREAN ASTRONOMICAL SOCIETY 46.5(2013):183-190. |
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