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      Dynamic Properties of Particle Injections Inside Geosynchronous Orbit: A Multisatellite Case Study

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          Abstract

          Four closely located satellites at and inside geosynchronous orbit (GEO) provided a great opportunity to study the dynamical evolution and spatial scale of premidnight energetic particle injections inside GEO during a moderate substorm on 23 December 2016. Just following the substorm onset, the four spacecraft, a LANL satellite at GEO, the two Van Allen Probes (also called “RBSP”) at ~5.8 R E, and a THEMIS satellite at ~5.3 R E, observed substorm‐related particle injections and local dipolarizations near the central meridian (~22 MLT) of a wedge‐like current system. The large‐scale evolution of the electron and ion (H, He, and O) injections was almost identical at the two RBSP spacecraft with ~0.5 R E apart. However, the initial short‐timescale particle injections exhibited a striking difference between RBSP‐A and ‐B: RBSP‐B observed an energy dispersionless injection which occurred concurrently with a transient, strong dipolarization front (DF) with a peak‐to‐peak amplitude of ~25 nT over ~25 s; RBSP‐A measured a dispersed/weaker injection with no corresponding DF. The spatiotemporally localized DF was accompanied by an impulsive, westward electric field (~20 mV m −1). The fast, impulsive E ×  B drift caused the radial transport of the electron and ion injection regions from GEO to ~5.8 R E. The penetrating DF fields significantly altered the rapid energy‐ and pitch angle‐dependent flux changes of the electrons and the H and He ions inside GEO. Such flux distributions could reflect the transient DF‐related particle acceleration and/or transport processes occurring inside GEO. In contrast, O ions were little affected by the DF fields.

          Key Points

          • Four spacecraft observations at and inside GEO reveal the dynamical nature of particle injections and their related local field changes

          • The dispersionless injections inside GEO are highly localized in azimuth and accompanied by a sharp dipolarization front (DF)

          • The DF‐related fields have a much greater impact on electron and light ion injections, but little affect heavy ion injections

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          Most cited references58

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          A magnetospheric magnetic field model with a warped tail current sheet

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            Satellite studies of magnetospheric substorms on August 15, 1968: 9. Phenomenological model for substorms

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              The THEMIS Fluxgate Magnetometer

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                Author and article information

                Contributors
                tetsuo.motoba@gmail.com
                Journal
                J Geophys Res Space Phys
                J Geophys Res Space Phys
                10.1002/(ISSN)2169-9402
                JGRA
                Journal of Geophysical Research. Space Physics
                John Wiley and Sons Inc. (Hoboken )
                2169-9380
                2169-9402
                17 September 2020
                September 2020
                : 125
                : 9 ( doiID: 10.1002/jgra.v125.9 )
                : e2020JA028215
                Affiliations
                [ 1 ] The Johns Hopkins University Applied Physics Laboratory Laurel MD USA
                [ 2 ] Space Sciences Department Aerospace Corporation Los Angeles CA USA
                [ 3 ] Department of Atmospheric and Oceanic Sciences University of California Los Angeles CA USA
                [ 4 ] Los Alamos National Laboratory Los Alamos NM USA
                [ 5 ] Center for Solar‐Terrestrial Research New Jersey Institute of Technology Newark NJ USA
                Author notes
                [*] [* ] Correspondence to:

                T. Motoba,

                tetsuo.motoba@ 123456gmail.com

                Author information
                https://orcid.org/0000-0002-8138-7897
                https://orcid.org/0000-0002-9565-6840
                https://orcid.org/0000-0001-5513-5947
                https://orcid.org/0000-0002-7985-8098
                https://orcid.org/0000-0002-3326-4024
                https://orcid.org/0000-0002-7347-0252
                Article
                JGRA55979 2020JA028215
                10.1029/2020JA028215
                7685150
                e590c0a5-f9d1-4b02-898a-ade9cc44fcec
                ©2020. The Authors.

                This is an open access article under the terms of the http://creativecommons.org/licenses/by-nc-nd/4.0/ License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made.

                History
                : 13 May 2020
                : 28 July 2020
                : 29 August 2020
                Page count
                Figures: 10, Tables: 0, Pages: 18, Words: 8905
                Funding
                Funded by: National Aeronautics and Space Administration (NASA) , open-funder-registry 10.13039/100000104;
                Award ID: 80NSSC19K0847
                Award ID: 80NSSC20K0699
                Award ID: NNX16AF74G
                Award ID: NAS5‐01072 NAS5‐02099
                Funded by: NSF | GEO | Division of Atmospheric and Geospace Sciences (AGS) , open-funder-registry 10.13039/100000159;
                Award ID: 1603028
                Categories
                Magnetospheric Physics
                Geospace Multi‐Point Observations in Van Allen Probes and Arase Era
                Magnetospheric Physics
                Substorms
                Magnetosphere: Inner
                Magnetospheric Configuration and Dynamics
                Research Article
                Research Articles
                Magnetospheric Physics
                Custom metadata
                2.0
                September 2020
                Converter:WILEY_ML3GV2_TO_JATSPMC version:5.9.4 mode:remove_FC converted:24.11.2020

                deep particle injections,dipolarizations,substorms,localized df

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