Global S&T Development Trend Analysis Platform of Resources and Environment
DOI | 10.1002/2017GL072866 |
Juno/JEDI observations of 0.01 to > 10 MeV energetic ions in the Jovian auroral regions: Anticipating a source for polar X-ray emission | |
Haggerty, D. K.1; Mauk, B. H.1; Paranicas, C. P.1; Clark, G.1; Kollmann, P.1; Rymer, A. M.1; Bolton, S. J.2; Connerney, J. E. P.3; Levin, S. M.3,4 | |
2017-07-16 | |
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:13 |
文章类型 | Article |
语种 | 英语 |
国家 | USA |
英文摘要 | After a successful orbit insertion, the Juno spacecraft completed its first 53.5 day orbit and entered a very low altitude perijove with the full scientific payload operational for the first time on 27 August 2016. The Jupiter Energetic particle Detector Instrument measured ions and electrons over the auroral regions and through closest approach, with ions measured from similar to 0.01 to > 10 MeV, depending on species. This report focuses on the composition of the energetic ions observed during the first perijove of the Juno mission. Of particular interest are the ions that precipitate from the magnetosphere onto the polar atmosphere and ions that are accelerated locally by Jupiter's powerful auroral processes. We report preliminary findings on the spatial variations, species, including energy and pitch angle distributions throughout the prime science region during the first orbit of the Juno mission. The prime motivation for this work was to examine the heavy ions that are thought to be responsible for the observed polar X-rays. Jupiter Energetic particle Detector Instrument (JEDI) did observe precipitating heavy ions with energies > 10 MeV, but for this perijove the intensities were far below those needed to account for previously observed polar X-ray emissions. During this survey we also found an unusual signal of ions between oxygen and sulfur. We include here a report on what appears to be a transitory observation of magnesium, or possibly sodium, at MeV energies through closest approach. |
领域 | 气候变化 |
收录类别 | SCI-E |
WOS记录号 | WOS:000406257400001 |
WOS关键词 | JUNO SPACECRAFT ; MAGNETOSPHERE ; JUPITER ; ATMOSPHERE ; ELECTRONS ; OXYGEN |
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/29008 |
专题 | 气候变化 |
作者单位 | 1.Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA; 2.Southwest Res Inst, San Antonio, TX USA; 3.NASA, Goddard Space Flight Ctr, Greenbelt, MD USA; 4.Jet Prop Lab, Pasadena, CA USA |
推荐引用方式 GB/T 7714 | Haggerty, D. K.,Mauk, B. H.,Paranicas, C. P.,et al. Juno/JEDI observations of 0.01 to > 10 MeV energetic ions in the Jovian auroral regions: Anticipating a source for polar X-ray emission[J]. GEOPHYSICAL RESEARCH LETTERS,2017,44(13). |
APA | Haggerty, D. K..,Mauk, B. H..,Paranicas, C. P..,Clark, G..,Kollmann, P..,...&Levin, S. M..(2017).Juno/JEDI observations of 0.01 to > 10 MeV energetic ions in the Jovian auroral regions: Anticipating a source for polar X-ray emission.GEOPHYSICAL RESEARCH LETTERS,44(13). |
MLA | Haggerty, D. K.,et al."Juno/JEDI observations of 0.01 to > 10 MeV energetic ions in the Jovian auroral regions: Anticipating a source for polar X-ray emission".GEOPHYSICAL RESEARCH LETTERS 44.13(2017). |
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