Cross-Scale Processes of Magnetic Reconnection

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dc.citation.articleNumber71en_US
dc.citation.journalTitleSpace Science Reviewsen_US
dc.citation.volumeNumber219en_US
dc.contributor.authorHwang, K.-J.en_US
dc.contributor.authorNakamura, R.en_US
dc.contributor.authorEastwood, J. P.en_US
dc.contributor.authorFuselier, S. A.en_US
dc.contributor.authorHasegawa, H.en_US
dc.contributor.authorNakamura, T.en_US
dc.contributor.authorLavraud, B.en_US
dc.contributor.authorDokgo, K.en_US
dc.contributor.authorTurner, D. L.en_US
dc.contributor.authorErgun, R. E.en_US
dc.contributor.authorReiff, P. H.en_US
dc.date.accessioned2024-05-03T15:51:15Zen_US
dc.date.available2024-05-03T15:51:15Zen_US
dc.date.issued2023en_US
dc.description.abstractVarious physical processes in association with magnetic reconnection occur over multiple scales from the microscopic to macroscopic scale lengths. This paper reviews multi-scale and cross-scale aspects of magnetic reconnection revealed in the near-Earth space beyond the general global-scale features and magnetospheric circulation organized by the Dungey Cycle. Significant and novel advancements recently reported, in particular, since the launch of the Magnetospheric Multi-scale mission (MMS), are highlighted being categorized into different locations with different magnetic topologies. These potentially paradigm-shifting findings include shock and foreshock transient driven reconnection, magnetosheath turbulent reconnection, flow shear driven reconnection, multiple X-line structures generated in the dayside/flankside/nightside magnetospheric current sheets, development and evolution of reconnection-driven structures such as flux transfer events, flux ropes, and dipolarization fronts, and their interactions with ambient plasmas. The paper emphasizes key aspects of kinetic processes leading to multi-scale structures and bringing large-scale impacts of magnetic reconnection as discovered in the geospace environment. These key features can be relevant and applicable to understanding other heliospheric and astrophysical systems.en_US
dc.identifier.citationHwang, K.-J., Nakamura, R., Eastwood, J. P., Fuselier, S. A., Hasegawa, H., Nakamura, T., Lavraud, B., Dokgo, K., Turner, D. L., Ergun, R. E., & Reiff, P. H. (2023). Cross-Scale Processes of Magnetic Reconnection. Space Science Reviews, 219(8), 71. https://doi.org/10.1007/s11214-023-01010-9en_US
dc.identifier.digitals11214-023-01010-9en_US
dc.identifier.doihttps://doi.org/10.1007/s11214-023-01010-9en_US
dc.identifier.urihttps://hdl.handle.net/1911/115592en_US
dc.language.isoengen_US
dc.publisherSpringer Natureen_US
dc.rightsExcept where otherwise noted, this work is licensed under a Creative Commons Attribution (CC BY) license. Permission to reuse, publish, or reproduce the work beyond the terms of the license or beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder.en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.titleCross-Scale Processes of Magnetic Reconnectionen_US
dc.typeJournal articleen_US
dc.type.dcmiTexten_US
dc.type.publicationpublisher versionen_US
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