The Formation of Saturn's and Jupiter's Electron Radiation Belts by Magnetospheric Electric Fields

被引:37
作者
Hao, Yi-Xin [1 ,2 ]
Sun, Yi-Xin [1 ,2 ]
Roussos, Elias [2 ]
Liu, Ying [1 ]
Kollmann, Peter [3 ]
Yuan, Chong-Jing [4 ]
Krupp, Norbert [2 ]
Paranicas, Chris [3 ]
Zhou, Xu-Zhi [1 ]
Murakami, Go [5 ]
Kita, Hajime [5 ]
Zong, Qiu-Gang [1 ]
机构
[1] Peking Univ, Inst Space Phys & Appl Technol, Beijing 100871, Peoples R China
[2] Max Planck Inst Solar Syst Res, D-37077 Gottingen, Germany
[3] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
[4] Chinese Acad Sci, Inst Geol & Geophys, Beijing 100029, Peoples R China
[5] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Chofu, Tokyo, Japan
基金
中国国家自然科学基金;
关键词
Van Allen radiation belt; Planetary magnetosphere; Outer planets; Jupiter; Saturn; EXTREME-ULTRAVIOLET SPECTROSCOPE; MAGNETIC-FIELD; ZEBRA STRIPES; ACCELERATION; INTERCHANGE; INJECTIONS; ASYMMETRY; MOTION;
D O I
10.3847/2041-8213/abca3f
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The existence of planetary radiation belts with relativistic electron components means that powerful acceleration mechanisms are operating within their volume. Mechanisms that bring charged particles planetward toward stronger magnetic fields can cause their heating. On the basis that electron fluxes in Saturn's radiation belts are enhanced over discrete energy intervals, previous studies have suggested that rapid inward plasma flows may be controlling the production of their most energetic electrons. However, rapid plasma inflows languish in the planet's inner magnetosphere, and they are not spatially appealing as a mechanism to form the belts. Here we show that slow, global-scale flows resulting from transient noon-to-midnight electric fields successfully explain the discretized flux spectra at quasi- and fully relativistic energies, and that they are ultimately responsible for the bulk of the highest energy electrons trapped at Saturn. This finding is surprising, given that plasma flows at Saturn are dominated by the planetary rotation; these weak electric field perturbations were previously considered impactful only over a very narrow electron energy range where the magnetic drifts of electrons cancel out with corotation. We also find quantitative evidence that ultrarelativistic electrons in Jupiter's radiation belts are accelerated by the same mechanism. Given that similar processes at Earth drive a less efficient electron transport compared to Saturn and Jupiter, the conclusion is emerging that global-scale electric fields can provide powerful relativistic electron acceleration, especially at strongly magnetized and fast-rotating astrophysical objects.
引用
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页数:13
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