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Formation of energetic electron butterfly distributions by magnetosonic waves via Landau resonance
Journal article   Open access   Peer reviewed

Formation of energetic electron butterfly distributions by magnetosonic waves via Landau resonance

Craig A Kletzing, Jinxing Li, Lunjin Chen, Binbin Ni, William S Kurth, Qianli Ma, George B Hospodarsky, Lun Xie, Zuyin Pu, Suiyan Fu, …
Geophysical research letters, Vol.43(7), pp.3009-3016
04/16/2016
DOI: 10.1002/2016GL067853
url
https://doi.org/10.1002/2016GL067853View
Published (Version of record) Open Access

Abstract

Radiation belt electrons can exhibit different types of pitch angle distributions in response to various magnetospheric processes. Butterfly distributions, characterized by flux minima at pitch angles around 90°, are broadly observed in both the outer and inner belts and the slot region. Butterfly distributions close to the outer magnetospheric boundary have been attributed to drift shell splitting and losses to the magnetopause. However, their occurrence in the inner belt and the slot region has hitherto not been resolved. By analyzing the particle and wave data collected by the Van Allen Probes during a geomagnetic storm, we combine test particle calculations and Fokker-Planck simulations to reveal that scattering by equatorial magnetosonic waves is a significant cause for the formation of energetic electron butterfly distributions in the inner magnetosphere. Another event shows that a large-amplitude magnetosonic wave in the outer belt can create electron butterfly distributions in just a few minutes.

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