Global S&T Development Trend Analysis Platform of Resources and Environment
DOI | 10.1002/2017GL072905 |
Preliminary JIRAM results from Juno polar observations: 2. Analysis of the Jupiter southern H-3(+) emissions and comparison with the north aurora | |
Adriani, A.1; Mura, A.1; Moriconi, M. L.2; Dinelli, B. M.2; Fabiano, F.2,3; Altieri, F.1; Sindoni, G.1; Bolton, S. J.4; Connerney, J. E. P.5; Atreya, S. K.6; Bagenal, F.7; Gerard, J. -C. M. C.8; Filacchione, G.1; Tosi, F.1; Migliorini, A.1; Grassi, D.1; Piccioni, G.1; Noschese, R.1; Cicchetti, A.1; Gladstone, G. R.4; Hansen, C.9; Kurth, W. S.10; Levin, S. M.11; Mauk, B. H.12; McComas, D. J.13; Olivieri, A.14; Turrini, D.1; Stefani, S.1; Amoroso, M.14 | |
2017-05-28 | |
发表期刊 | GEOPHYSICAL RESEARCH LETTERS
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ISSN | 0094-8276 |
EISSN | 1944-8007 |
出版年 | 2017 |
卷号 | 44期号:10 |
文章类型 | Article |
语种 | 英语 |
国家 | Italy; USA; Belgium |
英文摘要 | The Jupiter InfraRed Auroral Mapper (JIRAM) aboard Juno observed the Jovian South Pole aurora during the first orbit of the mission. H-3(+) (trihydrogen cation) and CH4 (methane) emissions have been identified and measured. The observations have been carried out in nadir and slant viewing both by a L-filtered imager and a 2-5m spectrometer. Results from the spectral analysis of the all observations taken over the South Pole by the instrument are reported. The coverage of the southern aurora during these measurements has been partial, but sufficient to determine different regions of temperature and abundance of the H-3(+) ion from its emission lines in the 3-4 mu m wavelength range. Finally, the results from the southern aurora are also compared with those from the northern ones from the data taken during the same perijove pass and reported by Dinelli et al. (2017). |
英文关键词 | Jupiter aurora Juno mission JIRAM spectrometer |
领域 | 气候变化 |
收录类别 | SCI-E |
WOS记录号 | WOS:000404131900031 |
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/28686 |
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.Southwest Res Inst, Space Sci Dept, San Antonio, TX USA; 5.NASA, Goddard Space Flight Ctr, Solar Syst Explorat Div, Planetary Magnetospheres Lab, Greenbelt, MD USA; 6.Univ Michigan, Planetary Sci Lab, Ann Arbor, MI USA; 7.Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80309 USA; 8.Univ Liege, Lab Phys Atmospher & Planetaire, Liege, Belgium; 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, Princeton Plasma Phys Lab, Dept Energys, POB 451, Princeton, NJ 08543 USA; 14.Agenzia Spaziale Italiana, Rome, Italy |
推荐引用方式 GB/T 7714 | Adriani, A.,Mura, A.,Moriconi, M. L.,et al. Preliminary JIRAM results from Juno polar observations: 2. Analysis of the Jupiter southern H-3(+) emissions and comparison with the north aurora[J]. GEOPHYSICAL RESEARCH LETTERS,2017,44(10). |
APA | Adriani, A..,Mura, A..,Moriconi, M. L..,Dinelli, B. M..,Fabiano, F..,...&Amoroso, M..(2017).Preliminary JIRAM results from Juno polar observations: 2. Analysis of the Jupiter southern H-3(+) emissions and comparison with the north aurora.GEOPHYSICAL RESEARCH LETTERS,44(10). |
MLA | Adriani, A.,et al."Preliminary JIRAM results from Juno polar observations: 2. Analysis of the Jupiter southern H-3(+) emissions and comparison with the north aurora".GEOPHYSICAL RESEARCH LETTERS 44.10(2017). |
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