GSTDTAP  > 气候变化
DOI10.1002/2017GL073730
A heavy ion and proton radiation belt inside of Jupiter's rings
Kollmann, P.1; Paranicas, C.1; Clark, G.1; Mauk, B. H.1; Haggerty, D. K.1; Rymer, A. M.1; Santos-Costa, D.2; Connerney, J. E. P.3; Allegrini, F.2,4; Valek, P.2; Kurth, W. S.5; Gladstone, G. R.2; Levin, S.6; Bolton, S.2
2017-06-16
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2017
卷号44期号:11
文章类型Article
语种英语
国家USA
英文摘要

Energetic charged particle measurements by the Jupiter Energetic Particle Detector Instrument (JEDI) on board Juno have revealed a radiation belt of hundreds of keV ions up to the atomic mass of sulfur, located between Jupiter's rings and atmosphere. Proton energy spectra display an unusual intensity increase above 300keV. We suggest that this is because charge exchange in Jupiter's neutral environment does not efficiently remove ions at such high energies. Since this innermost belt includes heavy ions, it cannot be exclusively supplied by cosmic ray albedo neutron decay, which is an important source at Earth and Saturn but only supplies protons and electrons. We find indications that the stripping of energetic neutral atoms in Jupiter's high atmosphere might be the ion source. Since the stripped off electrons are of low energy, this hypothesis is consistent with observations of the ratio of energetic electrons to ions being much less than 1.


Plain Language Summary Planets with their own a magnetic field, as Earth and Jupiter, are surrounded by "belts" of radiation. In case of Jupiter, most of this radiation extends to relatively large distances to Jupiter ( several times the size of the planet) but is so strong that it is difficult to engineer satellites that can fly through them safely. Juno is the first spacecraft that repeatedly passes close to Jupiter and its Jupiter Energetic Particle Detector Instrument ( JEDI) was now able to measure and quantify a small, separate radiation belt close to Jupiter. The measured population was unknown before and is located between Jupiter's atmosphere and its tenuous rings, inward to the main radiation belt.


英文关键词Juno Jupiter energetic particles energetic neutral atoms ENA CRAND radiation belt
领域气候变化
收录类别SCI-E
WOS记录号WOS:000404382600002
WOS关键词INNER MAGNETOSPHERE ; SYSTEM ; TORUS ; TRANSPORT ; HYDROGEN ; FLUXES
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/26800
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.Univ Texas San Antonio, Dept Phys & Astron, San Antonio, TX USA;
5.Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA;
6.Jet Prop Lab, Pasadena, CA USA
推荐引用方式
GB/T 7714
Kollmann, P.,Paranicas, C.,Clark, G.,et al. A heavy ion and proton radiation belt inside of Jupiter's rings[J]. GEOPHYSICAL RESEARCH LETTERS,2017,44(11).
APA Kollmann, P..,Paranicas, C..,Clark, G..,Mauk, B. H..,Haggerty, D. K..,...&Bolton, S..(2017).A heavy ion and proton radiation belt inside of Jupiter's rings.GEOPHYSICAL RESEARCH LETTERS,44(11).
MLA Kollmann, P.,et al."A heavy ion and proton radiation belt inside of Jupiter's rings".GEOPHYSICAL RESEARCH LETTERS 44.11(2017).
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