GSTDTAP  > 气候变化
DOI10.1002/2017GL072866
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
ISSN0094-8276
EISSN1944-8007
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).
条目包含的文件
条目无相关文件。
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Haggerty, D. K.]的文章
[Mauk, B. H.]的文章
[Paranicas, C. P.]的文章
百度学术
百度学术中相似的文章
[Haggerty, D. K.]的文章
[Mauk, B. H.]的文章
[Paranicas, C. P.]的文章
必应学术
必应学术中相似的文章
[Haggerty, D. K.]的文章
[Mauk, B. H.]的文章
[Paranicas, C. P.]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

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。