Institute of Space Physics and Applied Technology, Peking University, Beijing 100871, China
Polar Research Institute of China, Shanghai 200136, China
Invited contribution by Qiugang Zong, recipient of the EGU Hannes Alfvén Medal 2020.
Editorial note: during the submission and review process, the author failed to credit and cite the original paper for Fig. 5. The article has been corrected on 9 August 2024 accordingly.
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6,814
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Cumulative views and downloads
(calculated since 23 Nov 2021)
Total article views: 5,554 (including HTML, PDF, and XML)
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4,328
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5,554
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Cumulative views and downloads
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Total article views: 1,260 (including HTML, PDF, and XML)
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871
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Cumulative views and downloads
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Viewed (geographical distribution)
Total article views: 6,814 (including HTML, PDF, and XML)
Thereof 6,618 with geography defined
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Total article views: 5,554 (including HTML, PDF, and XML)
Thereof 5,430 with geography defined
and 124 with unknown origin.
Total article views: 1,260 (including HTML, PDF, and XML)
Thereof 1,188 with geography defined
and 72 with unknown origin.
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Latest update: 11 Mar 2026
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Please read the editorial note first before accessing the article.
Magnetospheric physics is in an extremely vibrant phase, with a number of ongoing and highly successful missions, e.g., Cluster, THEMIS, Van Allen Probes, and the MMS spacecraft, providing the most amazing observations and data sets. Since there are many fundamental and unsolved problems, in this paper I have addressed selected topics of ULF wave–charged particle interactions which encompass many special fields of radiation belt, ring current and plasmaspheric physics.
Magnetospheric physics is in an extremely vibrant phase, with a number of ongoing and highly...
