GSTDTAP  > 气候变化
DOI10.1002/2017GL073592
Preliminary JIRAM results from Juno polar observations: 3. Evidence of diffuse methane presence in the Jupiter auroral regions
Moriconi, M. L.1,2; Adriani, A.1; Dinelli, B. M.1,2; Fabiano, F.2,3; Altieri, F.1; Tosi, F.1; Filacchione, G.1; Migliorini, A.1; Gerard, J. C.4; Mura, A.1; Grassi, D.1; Sindoni, G.1; Piccioni, G.1; Noschese, R.1; Cicchetti, A.1; Bolton, S. J.5; Connerney, J. E. P.6; Atreya, S. K.7; Bagenal, F.8; Gladstone, G. R.5; Hansen, C.9; Kurth, W. S.10; Levin, S. M.11; Mauk, B. H.12; McComas, D. J.13; Turrini, D.1,14; Stefani, S.1; Olivieri, A.15; Amoroso, M.15
2017-05-28
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2017
卷号44期号:10
文章类型Article
语种英语
国家Italy; Belgium; USA; Chile
英文摘要

Throughout the first orbit of the NASA Juno mission around Jupiter, the Jupiter InfraRed Auroral Mapper (JIRAM) targeted the northern and southern polar regions several times. The analyses of the acquired images and spectra confirmed a significant presence of methane (CH4) near both poles through its 3.3m emission overlapping the H-3(+) auroral feature at 3.31m. Neither acetylene (C2H2) nor ethane (C2H6) have been observed so far. The analysis method, developed for the retrieval of H-3(+) temperature and abundances and applied to the JIRAM-measured spectra, has enabled an estimate of the effective temperature for methane peak emission and the distribution of its spectral contribution in the polar regions. The enhanced methane inside the auroral oval regions in the two hemispheres at different longitude suggests an excitation mechanism driven by energized particle precipitation from the magnetosphere.


英文关键词JIRAM spectrometer Jupiter atmosphere methane fluorescence
领域气候变化
收录类别SCI-E
WOS记录号WOS:000404131900032
WOS关键词X-RAY-EMISSION ; BRIGHTENINGS
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/27107
专题气候变化
作者单位1.INAF, Ist Astrofis & Planetol Spaziali, Rome, Italy;
2.CNR, Ist Sci Atmosfera & Clima, Bologna, Italy;
3.Univ Bologna, Dipartimento Fis & Astron, Bologna, Italy;
4.Univ Liege, Lab Phys Atmospher & Planetaire, Liege, Belgium;
5.Southwest Res Inst, Space Sci & Engn Div, San Antonio, TX USA;
6.NASA, Goddard Space Flight Ctr, Greenbelt, MD USA;
7.Univ Michigan, Planetary Sci Lab, 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.Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA;
12.Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA;
13.Princeton Univ, Plasma Phys Lab, Princeton, NJ 08544 USA;
14.Univ Atacama, Dept Fis, Copiapo, Chile;
15.Agenzia Spaziale Italiana, Rome, Italy
推荐引用方式
GB/T 7714
Moriconi, M. L.,Adriani, A.,Dinelli, B. M.,et al. Preliminary JIRAM results from Juno polar observations: 3. Evidence of diffuse methane presence in the Jupiter auroral regions[J]. GEOPHYSICAL RESEARCH LETTERS,2017,44(10).
APA Moriconi, M. L..,Adriani, A..,Dinelli, B. M..,Fabiano, F..,Altieri, F..,...&Amoroso, M..(2017).Preliminary JIRAM results from Juno polar observations: 3. Evidence of diffuse methane presence in the Jupiter auroral regions.GEOPHYSICAL RESEARCH LETTERS,44(10).
MLA Moriconi, M. L.,et al."Preliminary JIRAM results from Juno polar observations: 3. Evidence of diffuse methane presence in the Jupiter auroral regions".GEOPHYSICAL RESEARCH LETTERS 44.10(2017).
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