GSTDTAP  > 气候变化
DOI10.1002/2017GL072831
Plasma environment at the dawn flank of Jupiter's magnetosphere: Juno arrives at Jupiter
McComas, D. J.1,2,3; Szalay, J. R.3; Allegrini, F.3,4; Bagenal, F.5; Connerney, J.6; Ebert, R. W.3; Kurth, W. S.7; Louarn, P.8; Mauk, B.9; Reno, M.10; Thomsen, M. F.11; Valek, P.3,4; Weidner, S.2; Wilson, R. J.; Bolton, S.3
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USA; France
英文摘要

This study examines the first observations from the Jovian Auroral Distributions Experiment (JADE) as the Juno spacecraft arrived at Jupiter. JADE observations show that Juno crossed the bow shock at 08:16 UT on 2016 day of year (DOY) 176 and magnetopause at 21:20 on DOY 177, with additional magnetopause encounters until 23:39 on DOY 181. JADE made the first detailed observations of the plasma environment just inside the dawn flank of the magnetopause. We find subcorotational ions and variable electron beaming, with multiple flux tubes of varying plasma properties. Ion composition shows a dearth of heavy ions; protons dominate the plasma, with only intermittent, low fluxes of O+/S++, along with traces of O++ and S+++. We also find very little H-3(+) or He+, which are expected for an ionospheric plasma source. A few heavy ion bursts occur when the radial field nears reversal, but many other such reversals are not accompanied by heavy ions.


领域气候变化
收录类别SCI-E
WOS记录号WOS:000404131900007
WOS关键词BOW SHOCK ; SATURN
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/26596
专题气候变化
作者单位1.Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA;
2.Princeton Univ, Princeton Plasma Phys Lab, POB 451, Princeton, NJ 08543 USA;
3.Southwest Res Inst, Space Sci & Engn Div, San Antonio, TX USA;
4.Univ Texas San Antonio, Dept Phys & Astron, San Antonio, TX USA;
5.Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80309 USA;
6.Goddard Space Flight Ctr, Greenbelt, MD USA;
7.Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA;
8.Inst Rech Astrophys & Planetol, Toulouse, France;
9.Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA;
10.Austin Mission Consulting, Austin, TX USA;
11.Planetary Sci Inst, Tucson, AZ USA
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GB/T 7714
McComas, D. J.,Szalay, J. R.,Allegrini, F.,et al. Plasma environment at the dawn flank of Jupiter's magnetosphere: Juno arrives at Jupiter[J]. GEOPHYSICAL RESEARCH LETTERS,2017,44(10).
APA McComas, D. J..,Szalay, J. R..,Allegrini, F..,Bagenal, F..,Connerney, J..,...&Bolton, S..(2017).Plasma environment at the dawn flank of Jupiter's magnetosphere: Juno arrives at Jupiter.GEOPHYSICAL RESEARCH LETTERS,44(10).
MLA McComas, D. J.,et al."Plasma environment at the dawn flank of Jupiter's magnetosphere: Juno arrives at Jupiter".GEOPHYSICAL RESEARCH LETTERS 44.10(2017).
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