中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
首页 机构 成果 学者
  
  1. CAS IR Grid
  2. 地质与地球物理研究所
  3. 中国科学院地质与地球物理研究所
  4. 中国科学院地球与行星物理重点实验室
Temporal and Spectral Studies by XMM-Newton of Jupiter's X-ray Auroras During a Compression Event

文献类型：期刊论文

作者Wibisono, A. D.10,11; Branduardi-Raymont, G.10,11; Dunn, W. R.9,10,11; Coates, A. J.10,11; Weigt, D. M.8; Jackman, C. M.7,8; Yao, Z. H.6; Tao, C.5; Allegrini, F.1,4; Grodent, D.3
刊名JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
出版日期2020-05-01
卷号125期号:5页码:20
ISSN号2169-9380
关键词fast Fourier transform X-rays aurora Jupiter quasiperiodic pulsation spectroscopy
DOI10.1029/2019JA027676
英文摘要We report the temporal and spectral results of the first XMM-Newton observation of Jupiter's X-ray auroras during a clear magnetospheric compression event on June 2017 as confirmed by data from the Jovian Auroral Distributions Experiment (JADE) instrument onboard Juno. The northern and southern auroras were visible twice and thrice respectively as they rotated in and out of view during the similar to 23-hr (almost 2.5 Jupiter rotations) long XMM-Newton Jovian-observing campaign. Previous auroral observations by Chandra and XMM-Newton have shown that the X-ray auroras sometimes pulse with a regular period. We applied wavelet and fast Fourier transforms (FFTs) on the auroral light curves to show that, following the compression event, the X-ray auroras exhibited a recurring 23- to 27-min periodicity that lasted over 12.5 hr (longer than a Jupiter rotation). This periodicity was observed from both the northern and southern auroras, suggesting that the emission from both poles was caused by a shared driver. The soft X-ray component of the auroras is due to charge exchange processes between precipitating ions and neutrals in Jupiter's atmosphere. We utilized the Atomic Charge Exchange (ACX) spectral package to produce solar wind and iogenic plasma models to fit the auroral spectra in order to identify the origins of these ions. For this observation, the iogenic model gave the best fit, which suggests that the precipitating ions are from iogenic plasma in Jupiter's magnetosphere. Plain Language Summary The solar wind is a continuous stream of charged particles released by the Sun that flows out toward the edge of the Solar System. It meets obstacles along the way, such as the magnetic fields of planets like the Earth to create a magnetic bubble around them called a magnetosphere. The magnetosphere prevents most of these charged particles from reaching the Earth's atmosphere. Those that make their way through interact with the gas molecules in the atmosphere above the polar regions and cause them to glow to produce the auroras or the northern and southern lights. Jupiter's auroras are much more powerful than the Earth's, and they emit different types of radiation, including X-rays. It is currently unclear as to what causes Jupiter's X-ray auroras. Its moon, Io, spews volcanic material into the magnetosphere that can be accelerated into the planet's atmosphere. We created models that consisted of the particles found in the solar wind and in the material from Io's volcanoes to see which one was responsible for Jupiter's X-ray auroras. In this case, it was Io's volcanoes. We also found that the auroras pulsate every similar to 23-27 min in the north and similar to 23-33 min in the south. Key Points XMM-Newton observed Jupiter on 19 June 2017 during a magnetospheric compression event Fast Fourier transform analysis shows that the X-ray auroras pulsated over multiple Jupiter rotations Spectral analysis shows precipitating ions from Io and not the solar wind are responsible for the X-ray auroras
WOS关键词PHOTON IMAGING CAMERA ; CHANDRA ; WAVES
资助项目Science and Technology Facilities Council (STFC)[2062546] ; Science and Technology Facilities Council (STFC)[2115044] ; STFC Consolidated Grant[ST/S000240/1] ; SAO fellowship ; European Space Agency (ESA) Contract[4000120752/17/NL/MH] ; STFC Ernest Rutherford Fellowship[ST/L004399/1] ; Science Foundation Ireland Grant[18/FRL/6199] ; Strategic Priority Research Programof Chinese Academy of Sciences[XDA17010201] ; Japan Society for the Promotion of Science (JSPS) KAKENHI Grant[19H01948] ; National Aeronautics and Space Administration (NASA) ; Belgian Federal Science Policy Office (BELSPO) via the PRODEX Programme of ESA ; NASA/ESA Hubble Space Telescope[HST GO-14634]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者AMER GEOPHYSICAL UNION
WOS记录号WOS:000540229100012
资助机构Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; STFC Consolidated Grant ; STFC Consolidated Grant ; SAO fellowship ; SAO fellowship ; European Space Agency (ESA) Contract ; European Space Agency (ESA) Contract ; STFC Ernest Rutherford Fellowship ; STFC Ernest Rutherford Fellowship ; Science Foundation Ireland Grant ; Science Foundation Ireland Grant ; Strategic Priority Research Programof Chinese Academy of Sciences ; Strategic Priority Research Programof Chinese Academy of Sciences ; Japan Society for the Promotion of Science (JSPS) KAKENHI Grant ; Japan Society for the Promotion of Science (JSPS) KAKENHI Grant ; National Aeronautics and Space Administration (NASA) ; National Aeronautics and Space Administration (NASA) ; 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/ESA Hubble Space Telescope ; NASA/ESA Hubble Space Telescope ; Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; STFC Consolidated Grant ; STFC Consolidated Grant ; SAO fellowship ; SAO fellowship ; European Space Agency (ESA) Contract ; European Space Agency (ESA) Contract ; STFC Ernest Rutherford Fellowship ; STFC Ernest Rutherford Fellowship ; Science Foundation Ireland Grant ; Science Foundation Ireland Grant ; Strategic Priority Research Programof Chinese Academy of Sciences ; Strategic Priority Research Programof Chinese Academy of Sciences ; Japan Society for the Promotion of Science (JSPS) KAKENHI Grant ; Japan Society for the Promotion of Science (JSPS) KAKENHI Grant ; National Aeronautics and Space Administration (NASA) ; National Aeronautics and Space Administration (NASA) ; 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/ESA Hubble Space Telescope ; NASA/ESA Hubble Space Telescope ; Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; STFC Consolidated Grant ; STFC Consolidated Grant ; SAO fellowship ; SAO fellowship ; European Space Agency (ESA) Contract ; European Space Agency (ESA) Contract ; STFC Ernest Rutherford Fellowship ; STFC Ernest Rutherford Fellowship ; Science Foundation Ireland Grant ; Science Foundation Ireland Grant ; Strategic Priority Research Programof Chinese Academy of Sciences ; Strategic Priority Research Programof Chinese Academy of Sciences ; Japan Society for the Promotion of Science (JSPS) KAKENHI Grant ; Japan Society for the Promotion of Science (JSPS) KAKENHI Grant ; National Aeronautics and Space Administration (NASA) ; National Aeronautics and Space Administration (NASA) ; 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/ESA Hubble Space Telescope ; NASA/ESA Hubble Space Telescope ; Science and Technology Facilities Council (STFC) ; Science and Technology Facilities Council (STFC) ; STFC Consolidated Grant ; STFC Consolidated Grant ; SAO fellowship ; SAO fellowship ; European Space Agency (ESA) Contract ; European Space Agency (ESA) Contract ; STFC Ernest Rutherford Fellowship ; STFC Ernest Rutherford Fellowship ; Science Foundation Ireland Grant ; Science Foundation Ireland Grant ; Strategic Priority Research Programof Chinese Academy of Sciences ; Strategic Priority Research Programof Chinese Academy of Sciences ; Japan Society for the Promotion of Science (JSPS) KAKENHI Grant ; Japan Society for the Promotion of Science (JSPS) KAKENHI Grant ; National Aeronautics and Space Administration (NASA) ; National Aeronautics and Space Administration (NASA) ; 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/ESA Hubble Space Telescope ; NASA/ESA Hubble Space Telescope
源URL[http://ir.iggcas.ac.cn/handle/132A11/96912]  
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Wibisono, A. D.
作者单位1.Univ Texas San Antonio, San Antonio, TX USA
2.St Gilgen Int Sch, Dept Sci, St Gilgen, Austria
3.Univ Liege, Lab Phys Atmospher & Planetaire, Liege, Belgium
4.Southwest Res Inst, San Antonio, TX USA
5.Natl Inst Informat & Communicat Technol, Koganei, Tokyo, Japan
6.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
7.Dublin Inst Adv Studies, Dublin, Ireland
8.Univ Southampton, Dept Phys & Astron, Southampton, Hants, England
9.Harvard Smithsonian Ctr Astrophys, Smithsonian Astrophys Observ, 60 Garden St, Cambridge, MA 02138 USA
10.UCL Birkbeck, Ctr Planetary Sci, London, England
推荐引用方式
GB/T 7714		 Wibisono, A. D.,Branduardi-Raymont, G.,Dunn, W. R.,et al. Temporal and Spectral Studies by XMM-Newton of Jupiter's X-ray Auroras During a Compression Event[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2020,125(5):20.
APA Wibisono, A. D..,Branduardi-Raymont, G..,Dunn, W. R..,Coates, A. J..,Weigt, D. M..,...&Fleming, D..(2020).Temporal and Spectral Studies by XMM-Newton of Jupiter's X-ray Auroras During a Compression Event.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,125(5),20.
MLA Wibisono, A. D.,et al."Temporal and Spectral Studies by XMM-Newton of Jupiter's X-ray Auroras During a Compression Event".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 125.5(2020):20.

入库方式： OAI收割

来源：地质与地球物理研究所

浏览0
下载0
收藏0
其他版本

除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。