GSTDTAP  > 气候变化
DOI10.1002/2017GL072954
Infrared observations of Jovian aurora from Juno's first orbits: Main oval and satellite footprints
Mura, A.1; Adriani, A.1; Altieri, F.1; Connerney, J. E. P.2; Bolton, S. J.3; Moriconi, M. L.4; Gerard, J-C5; Kurth, W. S.6; Dinelli, B. M.4; Fabiano, F.1,4; Tosi, F.1; Atreya, S. K.7; Bagenal, F.8; Gladstone, G. R.3; Hansen, C.9; Levin, S. M.10; Mauk, B. H.11; McComas, D. J.12; Sindoni, G.1; Filacchione, G.1; Migliorini, A.1; Grassi, D.1; Piccioni, G.1; Noschese, R.1; Cicchetti, A.1; Turrini, D.1,13; Stefani, S.1; Amoroso, M.14; Olivieri, A.14
2017-06-16
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2017
卷号44期号:11
文章类型Article
语种英语
国家Italy; USA; Belgium; Chile
英文摘要

The Jovian Infrared Auroral Mapper (JIRAM) is an imager/spectrometer on board NASA/Juno mission for the study of the Jovian aurorae. The first results of JIRAM's imager channel observations of the H-3(+) infrared emission, collected around the first Juno perijove, provide excellent spatial and temporal distribution of the Jovian aurorae, and show the morphology of the main ovals, the polar regions, and the footprints of Io, Europa and Ganymede. The extended Io tail persists for similar to 3h after the passage of the satellite flux tube. Multi-arc structures of varied spatial extent appear in both main auroral ovals. Inside the main ovals, intense, localized emissions are observed. In the southern aurora, an evident circular region of strong depletion of H-3(+) emissions is partially surrounded by an intense emission arc. The southern aurora is brighter than the north one in these observations. Similar, probably conjugate emission patterns are distinguishable in both polar regions.


英文关键词aurora Jupiter
领域气候变化
收录类别SCI-E
WOS记录号WOS:000404382600008
WOS关键词IO FLUX TUBE ; ULTRAVIOLET ; JUPITER ; EMISSION ; IONOSPHERE ; MORPHOLOGY ; SPOTS ; MODEL
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/25628
专题气候变化
作者单位1.INAF, Ist Astrofis & Planetol Spaziali, Rome, Italy;
2.NASA, Goddard Space Flight Ctr, Greenbelt, MD USA;
3.Southwest Res Inst, San Antonio, TX USA;
4.CNR, Ist Sci Atmosfera & Clima, Bologna, Italy;
5.Univ Liege, LPAP, Liege, Belgium;
6.Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA;
7.Univ Michigan, Dept Atmospher Ocean & Space Sci, Ann Arbor, MI 48109 USA;
8.Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80309 USA;
9.Planetary Sci Inst, Tucson, AZ USA;
10.CALTECH, Jet Prop Lab, Pasadena, CA USA;
11.Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA;
12.Princeton Univ, PPPL, Princeton, NJ 08544 USA;
13.Univ Atacama, Dept Fis, UDA, Copiapo, Chile;
14.Agenzia Spaziale Italiana, Rome, Italy
推荐引用方式
GB/T 7714
Mura, A.,Adriani, A.,Altieri, F.,et al. Infrared observations of Jovian aurora from Juno's first orbits: Main oval and satellite footprints[J]. GEOPHYSICAL RESEARCH LETTERS,2017,44(11).
APA Mura, A..,Adriani, A..,Altieri, F..,Connerney, J. E. P..,Bolton, S. J..,...&Olivieri, A..(2017).Infrared observations of Jovian aurora from Juno's first orbits: Main oval and satellite footprints.GEOPHYSICAL RESEARCH LETTERS,44(11).
MLA Mura, A.,et al."Infrared observations of Jovian aurora from Juno's first orbits: Main oval and satellite footprints".GEOPHYSICAL RESEARCH LETTERS 44.11(2017).
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