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行星环电流的基本图像与动态变化过程

傅昊博 乐超

世界地震译丛2026,Vol.57Issue(4):371-382,12.
世界地震译丛2026,Vol.57Issue(4):371-382,12.DOI:10.19975/j.dqyxx.2025-034

行星环电流的基本图像与动态变化过程

Basic image and dynamic variation processes of planetary ring currents

傅昊博 1乐超2

作者信息

  • 1. 北京大学 地球与空间科学学院,北京 100871
  • 2. 北京大学 地球与空间科学学院,北京 100871||中国科学院国家空间科学中心 太阳活动与空间天气全国重点实验室,北京 100190
  • 折叠

摘要

Abstract

Ring currents,an important current system formed by the azimuthal drift of charged particles in planetary magnetospheres,play a key role in disturbing planetary magnetic fields and driving magnetospheric dy-namics.This paper systematically reviews recent research progress on the basic features and dynamic processes of ring currents around Earth,Mercury,Jupiter,and Saturn.For Earth's ring current,the contribution ratio of oxygen ions to the plasma pressure and energy density during geomagnetic storms significantly increases,and their loss mechanisms(such as charge exchange)have also been further discussed.In addition,the impact of geomagnetic substorms on the overall intensity,time variations,and spatial distributions of ring currents(such as enhancing dusk side ring currents via particle injections)has also been extensively studied.Further analysis confirms that the im-pacts of these two factors are not independent,but have positive relations:the energy density ratio of oxygen ions also increases during geomagnetic substorms.The existence of a ring current around Mercury had not been con-firmed before.However,using observations from the MESSENGER spacecraft and test particle simulations,recent studies have,for the first time,both observationally and theoretically discovered and confirmed the existence of ring currents that are formed by energetic protons orbiting along the Shabansky orbits.The basic characteristics of Mercury magnetic storms during strong solar activity periods are further studied.Research on the ring currents of Jupiter and Saturn relies highly on the datasets.Thanks to the rich data information provided by the Juno and Cas-sini spacecraft,recent research has,on the basis of previous results,obtained further conclusions on the giants'ring current.For Jupiter,the co-rotation characteristics,the dominant plasma component and their proportions,the spa-tial distributions,as well as the overall structure of the current sheet from the Io orbit to near the dawn side mag-netopause have been established.For Saturn,studies have revealed its bowl-shaped ring current structure,ENA fea-tures,and the 11-year variation cycles.Despite these significant advances,many questions about planetary ring cur-rents remain unresolved,including:(1)the causal relationship between a high ratio of oxygen ions and ring current intensification during intense geomagnetic storms;(2)the response of Mercury's ring current to solar wind vari-ations and the specific processes during Mercury's magnetic storms;and(3)the differences in the structure and dy-namics of ring currents among giant planets.Future satellite missions will provide novel observational data for ring current research,driving new breakthroughs in the discovery of planetary ring currents.

关键词

行星磁层/环电流/水星/木星/土星

Key words

planetary magnetosphere/ring current/Mercury/Jupiter/Saturn

分类

天文与地球科学

引用本文复制引用

傅昊博,乐超..行星环电流的基本图像与动态变化过程[J].世界地震译丛,2026,57(4):371-382,12.

基金项目

国家自然科学基金资助项目(42274200,42441809) (42274200,42441809)

国家重点研发计划资助项目(2023YFC2808900) Supported by the National Natural Science Foundation of China(Grant Nos.42274200,42441809)and the National Key R&D Pro-gram of China(Grant No.2023YFC2808900) (2023YFC2808900)

世界地震译丛

2097-1893

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