EGU26-948, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-948
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Tuesday, 05 May, 08:30–10:15 (CEST), Display time Tuesday, 05 May, 08:30–12:30
 
Hall X4, X4.147
Electron Precipitations from the Flow-Breaking Region: Can Whistler-Mode Waves Nonlinearly Resonate with Plasma Sheet Electrons?
Anton Artemyev1,2, Xiaojia Zhang3, and Vassilis Angelopoulos1
Anton Artemyev et al.
  • 1UCLA, Department of Earth, Planetary, and Space Sciences, Los Angeles, United States of America (aartemyev@igpp.ucla.edu)
  • 2UTA, Department of Physics, Arlington, United States of America
  • 3UTD, Department of Physics, Richardson, United States of America

Energetic electron precipitations from the flow-breaking region—the transition between the outer radiation belt and the plasma sheet—are typically characterized by dispersive signatures consistent with scattering via field-line curvature. However, during intervals of injections and magnetic field dipolarizations, low-altitude spacecraft have observed precipitation patterns more characteristic of whistler-mode scattering. In this study, we analyze examples of such precipitation patterns collected by the ELFIN CubeSat in conjunction with equatorial observations from the THEMIS mission. We show that whistler-mode-driven precipitation can include sub-second bursts, which are usually associated with nonlinear resonant scattering of electrons by chorus waves. Based on ELFIN and THEMIS observations, we discuss the possibility of nonlinear resonant electron scattering occurring in the flow-breaking region.

How to cite: Artemyev, A., Zhang, X., and Angelopoulos, V.: Electron Precipitations from the Flow-Breaking Region: Can Whistler-Mode Waves Nonlinearly Resonate with Plasma Sheet Electrons?, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-948, https://doi.org/10.5194/egusphere-egu26-948, 2026.