@article{1eb67bd3ca70404ea8956bc7cc991a3e,
title = "Differentiating Between Simultaneous Loss Drivers in Earth's Outer Radiation Belt: Multi‐Dimensional Phase Space Density Analysis",
abstract = "We analyzed the contribution of electromagnetic ion cyclotron (EMIC) wave driven electron loss to a flux dropout event in September 2017. The evolution of electron phase space density (PSD) through the dropout showed the formation of a radially peaked PSD profile as electrons were lost at high L*, resembling distributions created by magnetopause shadowing. By comparing 2D Fokker Planck simulations of pitch angle diffusion to the observed change in PSD, we found that the μ and K of electron loss aligned with maximum scattering rates at dropout onset. We conclude that, during this dropout event, EMIC waves produced substantial electron loss. Because pitch angle diffusion occurred on closed drift paths near the last closed drift shell, no radial PSD minimum was observed. Therefore, the radial PSD gradients resembled solely magnetopause shadowing loss, even though the local pitch angle scattering produced electron losses of several orders of magnitude of the PSD.",
keywords = "electron flux dropout, geomagnetic storm, Van Allen probes, magnetopause shadowing, EMIC wave, radiation belt",
author = "Staples, {F. A.} and Qianli Ma and Adam Kellerman and Rae, {I. J.} and Colin Forsyth and Sandhu, {J. K.} and Jacob Bortnik",
note = "Funding information: We acknowledge the developers of the IRBEM library, which was used to compute adiabatic invariant coordinates (Boscher et al., 2013). The computations employed computational and storage services associated with the Hoffman2 Shared Cluster provided by UCLA Institute for Digital Research and Education's Research Technology Group. ACK acknowledges high-performance computing support from Cheyenne (https://doi.org/10.5065/D6RX99HX) provided by NCAR's Computational and Information Systems Laboratory, sponsored by the National Science Foundation. FS was supported by NASA Grant 80NSSC20K1402 and NSF Grant 2149782. ACK acknowledges support from NASA Grants 80NSSC20K1402 and 80NSSC20K1281, and NSF Grant 2149782. QM acknowledges the NASA Grant 80NSSC20K0196, and NSF Grant AGS-2225445. IJR and JKS acknowledge support from NERC Grants NE/P017185/2, NE/V002554/2, and STFC Grant ST/V006320/1. CF was supported by NERC IRF NE/N014480/1 and NERC Grants NE/P017185/1 and NE/V002554/2.",
year = "2023",
month = dec,
day = "16",
doi = "10.1029/2023gl106162",
language = "English",
volume = "50",
journal = "Geophysical Research Letters",
issn = "0094-8276",
publisher = "American Geophysical Union",
number = "23",
}