Transport and Loss of Ring Current Electrons Inside Geosynchronous Orbit During the 17 March 2013 Storm

Aseev, N. A.; Shprits, Y. Y.; Wang, D.; Wygant, J.; Drozdov, A. Y.; Kellerman, A. C.; Reeves, G. D.

doi:10.1029/2018JA026031

Title: Transport and Loss of Ring Current Electrons Inside Geosynchronous Orbit During the 17 March 2013 Storm

Journal Article · Mon Jan 21 00:00:00 EST 2019 · Journal of Geophysical Research. Space Physics

DOI:https://doi.org/10.1029/2018JA026031· OSTI ID:1630876

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GFZ German Research Centre for Geosciences, Potsdam (Germany); Univ. of Potsdam (Germany)
GFZ German Research Centre for Geosciences, Potsdam (Germany); Univ. of Potsdam (Germany); Univ. of California, Los Angeles, CA (United States)
GFZ German Research Centre for Geosciences, Potsdam (Germany)
Univ. of Minnesota, Minneapolis, MN (United States)
Univ. of California, Los Angeles, CA (United States)
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

Ring current electrons (1–100 keV) have received significant attention in recent decades, but many questions regarding their major transport and loss mechanisms remain open. In this study, we use the four-dimensional Versatile Electron Radiation Belt code to model the enhancement of phase space density that occurred during the 17 March 2013 storm. Our model includes global convection, radial diffusion, and scattering into the Earth's atmosphere driven by whistler-mode hiss and chorus waves. We study the sensitivity of the model to the boundary conditions, global electric field, the electric field associated with subauroral polarization streams, electron loss rates, and radial diffusion coefficients. The results of the code are almost insensitive to the model parameters above 4.5 R _E R _E , which indicates that the general dynamics of the electrons between 4.5 R _E and the geostationary orbit can be explained by global convection. We found that the major discrepancies between the model and data can stem from the inaccurate electric field model and uncertainties in lifetimes. We show that additional mechanisms that are responsible for radial transport are required to explain the dynamics of ≥40-keV electrons, and the inclusion of the radial diffusion rates that are typically assumed in radiation belt studies leads to a better agreement with the data. The overall effect of subauroral polarization streams on the electron phase space density profiles seems to be smaller than the uncertainties in other input parameters. This study is an initial step toward understanding the dynamics of these particles inside the geostationary orbit.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: USDOE; National Aeronautics and Space Administration (NASA); Helmholtz-Gemeinschaft (HFG); National Science Foundation (NSF); German Research Foundation (DFG)

Grant/Contract Number:: 89233218CNA000001; NNX15AI94G; NNX16AG78G; AGS-1552321; NAS5-01072; 922613; CRC 1294

OSTI ID:: 1630876

Report Number(s):: LA-UR-19-32274; TRN: US2200709

Journal Information:: Journal of Geophysical Research. Space Physics, Vol. 124, Issue 2; ISSN 2169-9380

Publisher:: American Geophysical UnionCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 9 works

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Title: Transport and Loss of Ring Current Electrons Inside Geosynchronous Orbit During the 17 March 2013 Storm

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