A Solar Blowout Jet Caused by the Eruption of a Magnetic Flux Rope
文献类型:期刊论文
作者 | Cheng, Xin1,5; Huang, Chong2,3,6; Wang, Huaning4,6![]() ![]() ![]() ![]() |
刊名 | ASTROPHYSICAL JOURNAL LETTERS
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出版日期 | 2017-08-01 |
卷号 | 844期号:2 |
关键词 | Sun: Activity Sun: Chromosphere Sun: Corona Sun: Magnetic Fields |
DOI | 10.3847/2041-8213/aa8033 |
文献子类 | Article |
英文摘要 | We investigate the three-dimensional (3D) magnetic structure of a blowout jet originating in the western edge of NOAA active region (AR) 11513 on 2012 July 2 by means of recently developed forced field extrapolation model. The results show that the blowout jet was caused by the eruption of the magnetic flux rope (MFR) consisting of twisted field lines. We further calculate the twist number T-w and squashing factor Q of the reconstructed magnetic field and find that (1) the MFR corresponds well with the high T-w region, and (2) the MFR outer boundary corresponds well with the high Q region, probably interpreting the bright structure at the base of the jet. The twist number of the MFR is estimated to be T-w = -1.54 +/- 0.67. Thus, the kink instability is regarded as the initiation mechanism of the blowout jet as T-w reaches or even exceeds the threshold value of the kink instability. Our results also indicate that the bright point at the decaying phase is actually composed of some small loops that are heated by the reconnection occurring above. In summary, the blowout jet is mostly consistent with the scenario proposed by Moore et al., except that the kink instability is found to be a possible trigger. |
WOS关键词 | FORCED FIELD EXTRAPOLATION ; X-RAY JETS ; CORONAL HOLE ; TWIST ; DICHOTOMY ; EVOLUTION ; TOPOLOGY ; FLARES |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000406597400002 |
资助机构 | National Natural Science Foundation of China (NSFC)(11403044 ; National Natural Science Foundation of China (NSFC)(11403044 ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201609) ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201609) ; Natural Science Foundation of Shandong Province(ZR2014AP010) ; Natural Science Foundation of Shandong Province(ZR2014AP010) ; NJIT, US NSF(AGS-1250818) ; NJIT, US NSF(AGS-1250818) ; NASA(NNX13AG14G) ; NASA(NNX13AG14G) ; 11673035 ; 11673035 ; 11273031) ; 11273031) ; National Natural Science Foundation of China (NSFC)(11403044 ; National Natural Science Foundation of China (NSFC)(11403044 ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201609) ; CAS Key Laboratory of Solar Activity, National Astronomical Observatories(KLSA201609) ; Natural Science Foundation of Shandong Province(ZR2014AP010) ; Natural Science Foundation of Shandong Province(ZR2014AP010) ; NJIT, US NSF(AGS-1250818) ; NJIT, US NSF(AGS-1250818) ; NASA(NNX13AG14G) ; NASA(NNX13AG14G) ; 11673035 ; 11673035 ; 11273031) ; 11273031) |
源URL | [http://ir.bao.ac.cn/handle/114a11/20067] ![]() |
专题 | 国家天文台_太阳物理研究部 |
作者单位 | 1.Nanjing Univ, Nanjing, Jiangsu, Peoples R China 2.Shandong Univ, Inst Space Sci, Weihai 264209, Peoples R China 3.Shandong Univ, Sch Space Sci & Phys, Weihai 264209, Peoples R China 4.Univ Chinese Acad Sci, Beijing, Peoples R China 5.Nanjing Univ, Minist Educ, Key Lab Modern Astron & Astrophys, Nanjing 210093, Jiangsu, Peoples R China 6.Chinese Acad Sci, Key Lab Solar Act, Natl Astron Observ, Beijing, Peoples R China |
推荐引用方式 GB/T 7714 | Cheng, Xin,Huang, Chong,Wang, Huaning,et al. A Solar Blowout Jet Caused by the Eruption of a Magnetic Flux Rope[J]. ASTROPHYSICAL JOURNAL LETTERS,2017,844(2). |
APA | Cheng, Xin,Huang, Chong,Wang, Huaning,Zhu, Xiaoshuai,Zhu,Xiaoshuai,&Wang,Huaning.(2017).A Solar Blowout Jet Caused by the Eruption of a Magnetic Flux Rope.ASTROPHYSICAL JOURNAL LETTERS,844(2). |
MLA | Cheng, Xin,et al."A Solar Blowout Jet Caused by the Eruption of a Magnetic Flux Rope".ASTROPHYSICAL JOURNAL LETTERS 844.2(2017). |
入库方式: OAI收割
来源:国家天文台
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