Institutional Repository of Key Laboratory of Earth and Planetary Physics, Chinese Academy of Sciences
| On the Relation Between Auroral Morphologies and Compression Conditions of Jupiter's Magnetopause: Observations From Juno and the Hubble Space Telescope | |
| Yao, Z. H.1,2,3; Bonfond, B.2; Grodent, D.2; Chane, E.4; Dunn, W. R.5; Kurth, W. S.6; Connerney, J. E. P.7,8; Nichols, J. D.9; Palmaerts, B.2; Guo, R. L.2; Hospodarsky, G. B.6; Mauk, B. H.10; Kimura, T.11; Bolton, S. J.12 | |
| 2022-10-01 | |
| Source Publication | JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
 |
| ISSN | 2169-9380 |
| Volume | 127Issue:10Pages:17 |
| Abstract | Jupiter displays the most powerful auroral emissions in our solar system, which result from strong energy dissipation in Jupiter's surrounding space environment. Although mass and energy in Jupiter's magnetosphere mostly come from the innermost Galilean moon Io's volcanic activity and Jupiter's rotation, solar wind perturbations can play crucial roles in releasing magnetospheric energy. The systematic response of the aurora to a solar wind compression remains poorly understood because of timing uncertainties. Here we report the analysis of a set of auroral images from the Hubble Space Telescope with contemporaneous in situ magnetopause detections from Juno, allowing for a more direct comparison. By analyzing the dawn side main auroral emission, we distinguish two non-mutually exclusive types of auroral enhancements: auroral dawn storm (ADS) featured with latitudinal extension in limited longitudes, and a long-lasting main auroral brightening with limited extension in latitudes while extending over a large longitude range. Only the latter systematically appears under a compressed magnetopause, while the dawn storms could occur whatever the state of the magnetopause. The results could provide important constraints to improve theoretical models and numerical simulations. During expanded magnetopause conditions, Jupiter's aurora displayed either quiet or dawn storm morphology. The result is consistent with recent discovery of the initiation of ADSs in midnight and post-midnight, possibly driven by magnetic reconnection plasma instabilities in night magnetotail. Our results show that some typical auroral morphologies could be used as a diagnostic of solar wind conditions at Jupiter. |
| Keyword | Jovian aurora solar wind field-aligned current auroral dawn storm |
| DOI | 10.1029/2021JA029894 |
| Funding Organization | National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; NASA ; NASA ; NASA ; NASA ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; NASA ; NASA ; NASA ; NASA ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; NASA ; NASA ; NASA ; NASA ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; NASA ; NASA ; NASA ; NASA ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) |
| WOS Keyword | SOLAR-WIND ; ELECTRON ACCELERATION ; RADIO EMISSIONS ; ALFVEN WAVES ; MAGNETOSPHERE ; INJECTIONS ; SHOCK |
| Language | 英语 |
| Funding Project | National Key R&D Program of China[2021YFA0718600] ; National Science Foundation of China[42074211] ; Key Research Program of the Institute of Geology Geophysics CAS[IGGCAS-201904] ; NASA's New Frontiers Program for Juno ; Southwest Research Institute ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; NASA[699041X] ; International Space Science Institute in Beijing (ISSI-BJ) |
| Funding Organization | National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; NASA ; NASA ; NASA ; NASA ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; NASA ; NASA ; NASA ; NASA ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; NASA ; NASA ; NASA ; NASA ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Key R&D Program of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; National Science Foundation of China ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; Key Research Program of the Institute of Geology Geophysics CAS ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; NASA's New Frontiers Program for Juno ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Southwest Research Institute ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; NASA ; NASA ; NASA ; NASA ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) ; International Space Science Institute in Beijing (ISSI-BJ) |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:000861895300001 |
| Publisher | AMER GEOPHYSICAL UNION |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.iggcas.ac.cn/handle/132A11/108338 |
| Collection | 地球与行星物理院重点实验室 |
| Corresponding Author | Yao, Z. H. |
| Affiliation | 1.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China 2.Univ Liege, Lab Phys Atmospher & Planetaire, STAR Inst, Liege, Belgium 3.Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R China 4.Katholieke Univ Leuven, Ctr Math Plasma Astrophys, Leuven, Belgium 5.Univ Coll London, Mullard Space Sci Lab, Dorking, Surrey, England 6.Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA 7.Space Res Corp, Annapolis, MD USA 8.NASA, Goddard Space Flight Ctr, Greenbelt, MD USA 9.Univ Leicester, Dept Phys & Astron, Leicester, Leics, England 10.Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA 11.Tohoku Univ, Frontier Res Inst Interdisciplinary Sci, Sendai, Miyagi, Japan 12.Southwest Res Inst, San Antonio, TX USA |
| First Author Affilication | Key Laboratory of Earth and Planetary Physics, Chinese Academy of Sciences |
| Corresponding Author Affilication | Key Laboratory of Earth and Planetary Physics, Chinese Academy of Sciences |
| Recommended Citation GB/T 7714 | Yao, Z. H.,Bonfond, B.,Grodent, D.,et al. On the Relation Between Auroral Morphologies and Compression Conditions of Jupiter's Magnetopause: Observations From Juno and the Hubble Space Telescope[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2022,127(10):17. |
| APA | Yao, Z. H..,Bonfond, B..,Grodent, D..,Chane, E..,Dunn, W. R..,...&Bolton, S. J..(2022).On the Relation Between Auroral Morphologies and Compression Conditions of Jupiter's Magnetopause: Observations From Juno and the Hubble Space Telescope.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,127(10),17. |
| MLA | Yao, Z. H.,et al."On the Relation Between Auroral Morphologies and Compression Conditions of Jupiter's Magnetopause: Observations From Juno and the Hubble Space Telescope".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 127.10(2022):17. |
| Files in This Item: | There are no files associated with this item. | |||||
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment