2019
DOI: 10.3847/1538-4357/aaf970
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On the Contribution of EMIC Waves to the Reconfiguration of the Relativistic Electron Butterfly Pitch Angle Distribution Shape on 2014 September 12—A Case Study*

Abstract: Following the arrival of two interplanetary coronal mass ejections on 2014 September 12, the Relativistic Electron-Proton Telescope instrument on board the twin Van Allen Probes observed a long-term dropout in the outer belt electron fluxes. The interplanetary shocks compressed the magnetopause, thereby enabling the loss of relativistic electrons in the outer radiation belt to the magnetosheath region via the magnetopause shadowing. Previous studies have invoked enhanced radial transport associated with ultra-… Show more

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Cited by 9 publications
(18 citation statements)
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“…The spacecraft potential provides the electron number density and the minimum resonance energy calculated is 1.2 MeV, which indicates that the EMIC wave packets observed in this event can resonantly interact with electrons ≥1.2 MeV. Consequently, EMIC waves may have scattered electrons to the loss cone (see e.g., Medeiros et al, 2019) during the high-energy electron flux dropout in the outer radiation belt under the influence of the ICME's sheath.…”
Section: 1029/2020ja028492mentioning
confidence: 85%
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“…The spacecraft potential provides the electron number density and the minimum resonance energy calculated is 1.2 MeV, which indicates that the EMIC wave packets observed in this event can resonantly interact with electrons ≥1.2 MeV. Consequently, EMIC waves may have scattered electrons to the loss cone (see e.g., Medeiros et al, 2019) during the high-energy electron flux dropout in the outer radiation belt under the influence of the ICME's sheath.…”
Section: 1029/2020ja028492mentioning
confidence: 85%
“…During the maximum magnetosphere compression (panel e and f), the modeled magnetopause boundary intercepts the 100 nT isocontour line, which would correspond to the drift paths of equatorially mirroring electrons near geosynchronous orbit. Thus, such electrons would be lost to the adjacent magnetosheath region upon interception with the magnetopause (see also Medeiros et al., 2019), therefore strongly suggesting that magnetopause shadowing significantly contributed to remove relativistic electrons from the outermost region of the outer Van Allen belt. We thus identify magnetopause shadowing as the first dynamical mechanism contributing to the high‐energy electron loss during the turbulent ICME's sheath region.…”
Section: Dynamic Mechanisms Associated With the High‐energy Electron mentioning
confidence: 97%
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