Solitary Magnetic Structures at Quasi-Parallel Collisionless Shocks: Formation

dc.contributor.authorChen, Li-Jen
dc.contributor.authorWang, Shan
dc.contributor.authorNg, Jonathan
dc.contributor.authorBessho, Naoki
dc.contributor.authorTang, Jian-Ming
dc.contributor.authorFung, Shing F.
dc.contributor.authorLe, Guan
dc.contributor.authorGershman, Daniel
dc.contributor.authorGiles, Barbara
dc.contributor.authorRussell, Christopher T.
dc.contributor.authorTorbert, Roy
dc.contributor.authorBurch, James
dc.date.accessioned2021-07-28T13:22:44Z
dc.date.available2021-07-28T13:22:44Z
dc.date.issued2020-12-11
dc.description.abstractAbstract Solitary magnetic structures known as SLAMS (short large-amplitude magnetic structures) have been considered as essential elements of collisionless shocks with quasi-parallel geometries. Yet the physics underlying their formation remains an open question. In this paper, we use measurements from the magnetospheric multiscale mission combined with fully kinetic simulations to study the formation of SLAMS. We find that gyro-resonance between solar wind ions and right-hand circularly polarized electromagnetic waves results in magnetic field amplification. Gyro-trapping by the growing magnetic field buildup the plasma density that further enhances the current and field. The solitary nature of SLAMS stems from a beat-like magnetic field envelope where the maximum sets the initial location for nonlinear growth. Our results present a conceptual advance on SLAMS, and may shed new light on the open question of magnetic field amplification at astrophysical shocks. Plain Language Summary We integrate MMS measurements and fully kinetic simulations to investigate the nonlinear processes underlying ultra-low-frequency wave growth and evolution into solitary magnetic structures known as SLAMS. The understanding gained here presents a conceptual advance on the formation of SLAMS at planetary bow shocks, and may serve as new insight into how magnetic fields in the interstellar medium are amplified to create an environment for cosmic ray production at astrophysical shocks.en_US
dc.description.sponsorshipL.-J. Chen acknowledges S. Schwartz, D. Caprioli, C. Haggerty, M. Weidl, D. Ellison, E. Zweibel, and J. Drake for discussions. The research at GSFC and UMCP is supported in part by the MMS mission, DOE grants DESC0016278, DESC0020058, NSF AGS-1619584, AGS-2010231, and NASA 80NSSC18K1369.en_US
dc.description.urihttps://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2020GL090800en_US
dc.format.extent10 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m27afk-qgl8
dc.identifier.citationChen, Li-Jen et al.; Solitary Magnetic Structures at Quasi-Parallel Collisionless Shocks: Formation; Geophhysical Research Letters, 48, 1, 11 December, 2020; https://doi.org/10.1029/2020GL090800en_US
dc.identifier.urihttps://doi.org/10.1029/2020GL090800
dc.identifier.urihttp://hdl.handle.net/11603/22191
dc.language.isoen_USen_US
dc.publisherAmerican Geophysical Unionen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.rightsPublic Domain Mark 1.0*
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleSolitary Magnetic Structures at Quasi-Parallel Collisionless Shocks: Formationen_US
dc.typeTexten_US

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