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Article: Electron Energization and Energy Dissipation in Microscale Electromagnetic Environments

TitleElectron Energization and Energy Dissipation in Microscale Electromagnetic Environments
Authors
Issue Date2020
Citation
Astrophysical Journal Letters, 2020, v. 899, n. 2, article no. L31 How to Cite?
AbstractParticle energization and energy dissipation in electromagnetic environments are longstanding topics of intensive research in space, laboratory, and astrophysical plasmas. One challenge is to understand these conversion processes at smaller and smaller spatial/temporal scales. In this Letter, with very high cadence measurements of particle distributions from the Magnetospheric Multiscale spacecraft, we report evidence of evolution of an identified microscale (i.e., electron gyro-scale) magnetic cavity structure and reveal within it a unique energization process that does not adhere to prevailing adiabatic invariance theory. Our finding indicates that this process is largely energy dependent, and can accelerate/decelerate charged particles inside the trapping region during their gyromotion, clearly altering the particle distribution.
Persistent Identifierhttp://hdl.handle.net/10722/334686
ISSN
2021 Impact Factor: 8.811
2020 SCImago Journal Rankings: 3.639
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorLiu, J.-
dc.contributor.authorYao, S. T.-
dc.contributor.authorShi, Q. Q.-
dc.contributor.authorWang, X. G.-
dc.contributor.authorZong, Q. G.-
dc.contributor.authorFeng, Y. Y.-
dc.contributor.authorLiu, H.-
dc.contributor.authorGuo, R. L.-
dc.contributor.authorYao, Z. H.-
dc.contributor.authorRae, I. J.-
dc.contributor.authorDegeling, A. W.-
dc.contributor.authorTian, A. M.-
dc.contributor.authorRussell, C. T.-
dc.contributor.authorZhang, Y. T.-
dc.contributor.authorWang, Y. X.-
dc.contributor.authorWoodham, L. D.-
dc.contributor.authorPu, Z. Y.-
dc.contributor.authorXiao, C. J.-
dc.contributor.authorFu, S. Y.-
dc.contributor.authorGiles, B. L.-
dc.date.accessioned2023-10-20T06:49:55Z-
dc.date.available2023-10-20T06:49:55Z-
dc.date.issued2020-
dc.identifier.citationAstrophysical Journal Letters, 2020, v. 899, n. 2, article no. L31-
dc.identifier.issn2041-8205-
dc.identifier.urihttp://hdl.handle.net/10722/334686-
dc.description.abstractParticle energization and energy dissipation in electromagnetic environments are longstanding topics of intensive research in space, laboratory, and astrophysical plasmas. One challenge is to understand these conversion processes at smaller and smaller spatial/temporal scales. In this Letter, with very high cadence measurements of particle distributions from the Magnetospheric Multiscale spacecraft, we report evidence of evolution of an identified microscale (i.e., electron gyro-scale) magnetic cavity structure and reveal within it a unique energization process that does not adhere to prevailing adiabatic invariance theory. Our finding indicates that this process is largely energy dependent, and can accelerate/decelerate charged particles inside the trapping region during their gyromotion, clearly altering the particle distribution.-
dc.languageeng-
dc.relation.ispartofAstrophysical Journal Letters-
dc.titleElectron Energization and Energy Dissipation in Microscale Electromagnetic Environments-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.3847/2041-8213/abab92-
dc.identifier.scopuseid_2-s2.0-85090446530-
dc.identifier.volume899-
dc.identifier.issue2-
dc.identifier.spagearticle no. L31-
dc.identifier.epagearticle no. L31-
dc.identifier.eissn2041-8213-
dc.identifier.isiWOS:000566179400001-

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