Mechanisms of Saturn's Near-Noon Transient Aurora: In Situ Evidence From Cassini Measurements
文献类型：期刊论文
| 作者 | Yao, Z. H.1,2; Radioti, A.1; Rae, I. J.2; Liu, J.3; Grodent, D.1; Ray, L. C.4; Badman, S. V.4; Coates, A. J.2; Gerard, J. -C.1; Waite, J. H.5 |
| 刊名 | GEOPHYSICAL RESEARCH LETTERS
 |
| 出版日期 | 2017-11-28 |
| 卷号 | 44期号:22页码:11217-11228 |
| ISSN号 | 0094-8276 |
| DOI | 10.1002/2017GL075108 |
| 文献子类 | Article |
| 英文摘要 | Although auroral emissions at giant planets have been observed for decades, the physical mechanisms of aurorae at giant planets remain unclear. One key reason is the lack of simultaneous measurements in the magnetosphere while remote sensing of the aurora. We report a dynamic auroral event identified with the Cassini Ultraviolet Imaging Spectrograph (UVIS) at Saturn on 13 July 2008 with coordinated measurements of the magnetic field and plasma in the magnetosphere. The auroral intensification was transient, only lasting for similar to 30 min. The magnetic field and plasma are perturbed during the auroral intensification period. We suggest that this intensification was caused by wave mode conversion generated field-aligned currents, and we propose two potential mechanisms for the generation of this plasma wave and the transient auroral intensification. A survey of the Cassini UVIS database reveals that this type of transient auroral intensification is very common (10/11 time sequences, and similar to 10% of the total images). |
| WOS关键词 | HUBBLE-SPACE-TELESCOPE ; BURSTY BULK FLOWS ; PI2 PULSATIONS ; STATISTICAL-ANALYSIS ; SUBSTORM ONSET ; PLASMA SHEET ; ALFVEN WAVES ; MAGNETOSPHERE ; RECONNECTION ; MAGNETOPAUSE |
| WOS研究方向 | Geology |
| 语种 | 英语 |
| WOS记录号 | WOS:000419102300001 |
| 出版者 | AMER GEOPHYSICAL UNION |
| 资助机构 | European Union ; European Union ; UK Science and Technology Facilities Council (STFC) at UCL/MSSL(ST/L005638/1) ; UK Science and Technology Facilities Council (STFC) at UCL/MSSL(ST/L005638/1) ; National Science Foundation of China(41525016 ; National Science Foundation of China(41525016 ; Belgian Fund for Scientific Research (FNRS) ; Belgian Fund for Scientific Research (FNRS) ; European Space Agency Research Fellowship ; European Space Agency Research Fellowship ; NASA ; NASA ; ESA ; ESA ; 41404117) ; 41404117) ; European Union ; European Union ; UK Science and Technology Facilities Council (STFC) at UCL/MSSL(ST/L005638/1) ; UK Science and Technology Facilities Council (STFC) at UCL/MSSL(ST/L005638/1) ; National Science Foundation of China(41525016 ; National Science Foundation of China(41525016 ; Belgian Fund for Scientific Research (FNRS) ; Belgian Fund for Scientific Research (FNRS) ; European Space Agency Research Fellowship ; European Space Agency Research Fellowship ; NASA ; NASA ; ESA ; ESA ; 41404117) ; 41404117) ; European Union ; European Union ; UK Science and Technology Facilities Council (STFC) at UCL/MSSL(ST/L005638/1) ; UK Science and Technology Facilities Council (STFC) at UCL/MSSL(ST/L005638/1) ; National Science Foundation of China(41525016 ; National Science Foundation of China(41525016 ; Belgian Fund for Scientific Research (FNRS) ; Belgian Fund for Scientific Research (FNRS) ; European Space Agency Research Fellowship ; European Space Agency Research Fellowship ; NASA ; NASA ; ESA ; ESA ; 41404117) ; 41404117) ; European Union ; European Union ; UK Science and Technology Facilities Council (STFC) at UCL/MSSL(ST/L005638/1) ; UK Science and Technology Facilities Council (STFC) at UCL/MSSL(ST/L005638/1) ; National Science Foundation of China(41525016 ; National Science Foundation of China(41525016 ; Belgian Fund for Scientific Research (FNRS) ; Belgian Fund for Scientific Research (FNRS) ; European Space Agency Research Fellowship ; European Space Agency Research Fellowship ; NASA ; NASA ; ESA ; ESA ; 41404117) ; 41404117) |
| 源URL | [http://ir.iggcas.ac.cn/handle/132A11/93137]  |
| 专题 | 地质与地球物理研究所_中国科学院地球与行星物理重点实验室 |
| 通讯作者 | Yao, Z. H. |
| 作者单位 | 1.Univ Liege, STAR Inst, Lab Phys Atmospher & Planetaire, Liege, Belgium 2.UCL Mullard Space Sci Lab, Dorking, Surrey, England 3.Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA USA 4.Univ Lancaster, Dept Phys, Lancaster, England 5.Southwest Res Inst, San Antonio, TX USA 6.European Space Astron Ctr ESA ESAC, Operat Dept, Madrid, Spain 7.Shandong Univ, Sch Space Sci & Phys, Shandong Prov Key Lab Optic Astron & Solar Terr, Weihai, Peoples R China 8.Chinese Acad Sci, Inst Geol & Geophys, Beijing, Peoples R China 9.Imperial Coll, Fac Nat Sci, Dept Phys, London, England 10.Max Planck Inst Solar Syst Res, Gottingen, Germany |
| 推荐引用方式 GB/T 7714 | Yao, Z. H.,Radioti, A.,Rae, I. J.,et al. Mechanisms of Saturn's Near-Noon Transient Aurora: In Situ Evidence From Cassini Measurements[J]. GEOPHYSICAL RESEARCH LETTERS,2017,44(22):11217-11228. |
| APA | Yao, Z. H..,Radioti, A..,Rae, I. J..,Liu, J..,Grodent, D..,...&Palmaerts, B..(2017).Mechanisms of Saturn's Near-Noon Transient Aurora: In Situ Evidence From Cassini Measurements.GEOPHYSICAL RESEARCH LETTERS,44(22),11217-11228. |
| MLA | Yao, Z. H.,et al."Mechanisms of Saturn's Near-Noon Transient Aurora: In Situ Evidence From Cassini Measurements".GEOPHYSICAL RESEARCH LETTERS 44.22(2017):11217-11228. |
入库方式： OAI收割
来源：地质与地球物理研究所
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