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Article: Observations of the Beam-Driven Whistler Mode Waves in the Magnetic Reconnection Region at the Dayside Magnetopause

TitleObservations of the Beam-Driven Whistler Mode Waves in the Magnetic Reconnection Region at the Dayside Magnetopause
Authors
Issue Date2021
Citation
Journal of Geophysical Research: Space Physics, 2021, v. 126, n. 2, article no. e2020JA028525 How to Cite?
AbstractWe report observations of the whistler mode waves in the magnetic reconnection region at the dayside magnetopause using the magnetospheric multiscale (MMS) mission on January 11, 2016. In this event, whistlers mostly occur on the magnetospheric side of the reconnection central plane and are closely related to counter-streaming electron beams in the medium energy range (200–300 eV). These counter-streaming electron beams can be attributed to the accelerated magnetosheath electrons by the reconnection. Through quantitatively testing the Landau resonance condition and solving the kinetic dispersion relations, we present the evidence for whistler excitation by electron beams in the medium energy range. Additionally, the whistlers are observed simultaneously with the pitch-angle scattering of electrons in the high-energy range (300–3,000 eV). The calculation results show that this scattering is likely to occur through electron cyclotron wave-particle interactions, which can isotropize electrons and exchange energy between plasmas and waves.
Persistent Identifierhttp://hdl.handle.net/10722/346992
ISSN
2023 Impact Factor: 2.6
2023 SCImago Journal Rankings: 0.845

 

DC FieldValueLanguage
dc.contributor.authorZhao, S. Q.-
dc.contributor.authorXiao, C. J.-
dc.contributor.authorLiu, Terry Z.-
dc.contributor.authorChen, Huayue-
dc.contributor.authorZhang, H.-
dc.contributor.authorShi, M. J.-
dc.contributor.authorTeng, Shangchun-
dc.contributor.authorZhang, H. S.-
dc.contributor.authorWang, X. G.-
dc.contributor.authorPu, Z. Y.-
dc.contributor.authorLiu, M. Z.-
dc.date.accessioned2024-09-17T04:14:38Z-
dc.date.available2024-09-17T04:14:38Z-
dc.date.issued2021-
dc.identifier.citationJournal of Geophysical Research: Space Physics, 2021, v. 126, n. 2, article no. e2020JA028525-
dc.identifier.issn2169-9380-
dc.identifier.urihttp://hdl.handle.net/10722/346992-
dc.description.abstractWe report observations of the whistler mode waves in the magnetic reconnection region at the dayside magnetopause using the magnetospheric multiscale (MMS) mission on January 11, 2016. In this event, whistlers mostly occur on the magnetospheric side of the reconnection central plane and are closely related to counter-streaming electron beams in the medium energy range (200–300 eV). These counter-streaming electron beams can be attributed to the accelerated magnetosheath electrons by the reconnection. Through quantitatively testing the Landau resonance condition and solving the kinetic dispersion relations, we present the evidence for whistler excitation by electron beams in the medium energy range. Additionally, the whistlers are observed simultaneously with the pitch-angle scattering of electrons in the high-energy range (300–3,000 eV). The calculation results show that this scattering is likely to occur through electron cyclotron wave-particle interactions, which can isotropize electrons and exchange energy between plasmas and waves.-
dc.languageeng-
dc.relation.ispartofJournal of Geophysical Research: Space Physics-
dc.titleObservations of the Beam-Driven Whistler Mode Waves in the Magnetic Reconnection Region at the Dayside Magnetopause-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1029/2020JA028525-
dc.identifier.scopuseid_2-s2.0-85102100890-
dc.identifier.volume126-
dc.identifier.issue2-
dc.identifier.spagearticle no. e2020JA028525-
dc.identifier.epagearticle no. e2020JA028525-
dc.identifier.eissn2169-9402-

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