Modulation of Energetic Electron Precipitation Driven by Three Types of Whistler Mode Waves

Author:

Shen Xiao‐Chen1ORCID,Li Wen1ORCID,Capannolo Luisa1ORCID,Ma Qianli12ORCID,Qin Murong13ORCID,Artemyev Anton V.4ORCID,Angelopoulos Vassilis4ORCID,Zhang Xiao‐Jia45ORCID,Huang Sheng1ORCID

Affiliation:

1. Center for Space Physics Boston University Boston MA USA

2. Department of Atmospheric and Oceanic Sciences University of California Los Angeles CA USA

3. Cooperative Programs for the Advancement of Earth System Science UCAR Boulder CO USA

4. Department of Earth, Planetary, and Space Sciences University of California Los Angeles CA USA

5. Department of Physics University of Texas at Dallas Richardson TX USA

Abstract

AbstractPrecipitation into the Earth's atmosphere due to pitch angle scattering by plasma waves has been recognized as one of the major loss mechanisms for energetic electrons. In this study, we quantitatively evaluate their roles in precipitating electrons during a conjunction event with modulated electron precipitation observed at low altitudes by Electron Loss and Fields INvestigation and three types of whistler mode waves (hiss, plume hiss, and chorus) measured near the equator by Time History of Events and Macroscale Interactions during Substorms. Electron precipitation was observed from ∼50 keV to <1 MeV with a spatial modulation, suggested by a good correlation between L shell‐sorted precipitation fluxes and wave intensities. A quasi‐linear analysis supports the observed energy range of precipitation and the ratio of precipitating‐to‐trapped flux. Our findings reveal that the modulated energetic electron precipitation is driven by hiss, plume hiss, and chorus waves.

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

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