Articles | Volume 40, issue 1
Ann. Geophys., 40, 121–150, 2022
https://doi.org/10.5194/angeo-40-121-2022
Ann. Geophys., 40, 121–150, 2022
https://doi.org/10.5194/angeo-40-121-2022
Review paper
 | Highlight paper
28 Feb 2022
Review paper  | Highlight paper | 28 Feb 2022

Magnetospheric response to solar wind forcing: ultra-low-frequency wave–particle interaction perspective

Qiugang Zong

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Cited articles

Alfvén, H.: Existence of electromagnetic-hydrodynamic waves, Nature, 150, 405–406, 1942. 
Alfvén, H. and Arrhenius, G.: Evolution of the solar system (Vol. 10), Scientific and Technical Information Office, National Aeronautics and Space Administration, https://ntrs.nasa.gov/api/citations/19770006016/downloads/19770006016.pdf (last access: 24 February 2022), 1976. 
Alfvén, H. and Fälthammar, C. G.: Cosmical Electrodynamics, Clarendon, 1963. 
Arnoldy, R. L., Moore, T. E., and Akasofu, S. I.: Plasma injection events at synchronous orbit related to positive Dst, J. Geophys. Res., 87, 77–84, 1982. 
Bellan, P. M.: Fundamentals of plasma physics, Cambridge, Cambridge University Press, https://doi.org/10.1017/CBO9780511807183, 2008. 
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Short summary
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.