Review of Mercury’s dynamic magnetosphere: Post-MESSENGER era and comparative magnetospheres

• Published in: Science China. Earth sciences Vol. 65; no. 1; pp. 25 - 74
• Main Authors: Sun, Weijie, Dewey, Ryan M., Aizawa, Sae, Huang, Jia, Slavin, James A., Fu, Suiyan, Wei, Yong, Bowers, Charles F.
• Format: Journal Article
• Language: English
• Published: Beijing Science China Press 01.01.2022; Springer Nature B.V
• Subjects: Current sheets; Dynamics; Earth and Environmental Science; Earth magnetosphere; Earth Sciences; Electric fields; Exosphere; Kelvin-Helmholtz waves; Magnetic properties; Magnetic reconnection; Magnetopause; Magnetosheath; Mercury; Mercury (planet); MESSENGER Mission; Planetary magnetospheres; Review; Reviews; Space missions; Spacecraft; Core induction; Dawn-dusk asymmetry; Kelvin-Helmholtz wave; Flux transfer event shower; Extreme solar events; Substorm current wedge; Mercury’s magnetosphere; Reconnection erosion; Particle energization
• ISSN: 1674-7313; 1869-1897
• DOI: 10.1007/s11430-021-9828-0

This review paper summarizes the research of Mercury’s magnetosphere in the Post-MESSENGER era and compares its dynamics to those in other planetary magnetospheres, especially to those in Earth’s magnetosphere. This review starts by introducing the planet Mercury, including its interplanetary environment, magnetosphere, exosphere, and conducting core. The frequent and intense magnetic reconnection on the dayside magnetopause, which is represented by the flux transfer event “shower”, is reviewed on how they depend on magnetosheath plasma β and magnetic shear angle across the magnetopause, following by how it contributes to the flux circulation and magnetosphere-surface-exosphere coupling. In the next, Mercury’s magnetosphere under extreme solar events, including the core induction and the reconnection erosion on the dayside magnetosphere, the responses of the nightside magnetosphere, are reviewed. Then, the dawn-dusk properties of the plasma sheet, including the features of the ions, the structure of the current sheet, and the dynamics of magnetic reconnection, are summarized. The last topic is devoted to the particle energization in Mercury’s magnetosphere, which includes the energization of the Kelvin-Helmholtz waves on the magnetopause boundaries, reconnection-generated magnetic structures, and the cross-tail electric field. In each chapter, the last section discusses the open questions related to each topic, which can be considered by the simulations and the future spacecraft mission. We end this paper by summarizing the future BepiColombo opportunities, which is a joint mission of ESA and JAXA and is en route to Mercury.