WHY IS A FLARE-RICH ACTIVE REGION CME-POOR?
文献类型：期刊论文
| 作者 | Liu, Lijuan1,2; Wang, Yuming1,3; Wang, Jingxiu4 ; Shen, Chenglong1,3; Ye, Pinzhong1; Liu, Rui1,2; Chen, Jun1,5; Zhang, Quanhao1,5; Wang, S.1,2; Wang,Jingxiu
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2016-08-01 |
| 卷号 | 826期号:2 |
| 关键词 | Sun: activity Sun: coronal mass ejections (CMEs) Sun: flares Sun: magnetic fields |
| 英文摘要 | Solar active regions (ARs) are the major sources of two of the most violent solar eruptions, namely flares and coronal mass ejections (CMEs). The largest AR in the past 24 years, NOAA AR 12192, which crossed the visible disk from 2014 October 17 to 30, unusually produced more than one hundred flares, including 32 M-class and 6 X-class ones, but only one small CME. Flares and CMEs are believed to be two phenomena in the same eruptive process. Why is such a flare-rich AR so CME-poor? We compared this AR with other four ARs; two were productive in both and two were inert. The investigation of the photospheric parameters based on the SDO/HMI vector magnetogram reveals that the flare-rich AR 12192, as with the other two productive ARs, has larger magnetic flux, current, and free magnetic energy than the two inert ARs but, in contrast to the two productive ARs, it has no strong, concentrated current helicity along both sides of the flaring neutral line, indicating the absence of a mature magnetic structure consisting of highly sheared or twisted field lines. Furthermore, the decay index above the AR 12192 is relatively low, showing strong constraint. These results suggest that productive ARs are always large and have enough current and free energy to power flares, but whether or not a flare is accompanied by a CME is seemingly related to (1) the presence of a mature sheared or twisted core field serving as the seed of the CME, or (2) a weak enough constraint of the overlying arcades. |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | CORONAL MASS EJECTIONS ; MAJOR SOLAR-FLARES ; MAGNETIC-FIELD PROPERTIES ; ELECTRIC-CURRENT HELICITY ; X-CLASS FLARES ; VECTOR MAGNETOGRAMS ; PRODUCTIVITY ; ENERGY ; TWIST ; DEPENDENCE |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000381977900019 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/6882]  |
| 专题 | 国家天文台_太阳物理研究部 |
| 作者单位 | 1.Univ Sci & Technol China, Dept Geophys & Planetary Sci, CAS Key Lab Geospace Environm, Hefei 230026, Anhui, Peoples R China 2.Collaborat Innovat Ctr Astronaut Sci & Technol, Hefei, Peoples R China 3.Univ Sci & Technol China, Synerget Innovat Ctr Quantum Informat & Quantum P, Hefei 230026, Anhui, Peoples R China 4.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 5.Univ Sci & Technol China, Mengcheng Natl Geophys Observ, Hefei, Anhui, Peoples R China |
| 推荐引用方式 GB/T 7714 | Liu, Lijuan,Wang, Yuming,Wang, Jingxiu,et al. WHY IS A FLARE-RICH ACTIVE REGION CME-POOR?[J]. ASTROPHYSICAL JOURNAL,2016,826(2). |
| APA | Liu, Lijuan.,Wang, Yuming.,Wang, Jingxiu.,Shen, Chenglong.,Ye, Pinzhong.,...&Wang,Jingxiu.(2016).WHY IS A FLARE-RICH ACTIVE REGION CME-POOR?.ASTROPHYSICAL JOURNAL,826(2). |
| MLA | Liu, Lijuan,et al."WHY IS A FLARE-RICH ACTIVE REGION CME-POOR?".ASTROPHYSICAL JOURNAL 826.2(2016). |
入库方式： OAI收割
来源：国家天文台
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