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

Abstract

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 radiationmore » 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.« less

Authors:
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3]; ORCiD logo [4]; ORCiD logo [5]; ORCiD logo [5]; ORCiD logo [6]
+ Show Author Affiliations
  1. GFZ German Research Centre for Geosciences, Potsdam (Germany); Univ. of Potsdam (Germany)
  2. GFZ German Research Centre for Geosciences, Potsdam (Germany); Univ. of Potsdam (Germany); Univ. of California, Los Angeles, CA (United States)
  3. GFZ German Research Centre for Geosciences, Potsdam (Germany)
  4. Univ. of Minnesota, Minneapolis, MN (United States)
  5. Univ. of California, Los Angeles, CA (United States)
  6. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
Publication Date:
Research Org.:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Org.:
USDOE; National Aeronautics and Space Administration (NASA); Helmholtz-Gemeinschaft (HFG); National Science Foundation (NSF); German Research Foundation (DFG)
OSTI Identifier:
1630876
Report Number(s):
LA-UR-19-32274
Journal ID: ISSN 2169-9380; TRN: US2200709
Grant/Contract Number:  
89233218CNA000001; NNX15AI94G; NNX16AG78G; AGS-1552321; NAS5-01072; 922613; CRC 1294
Resource Type:
Accepted Manuscript
Journal Name:
Journal of Geophysical Research. Space Physics
Additional Journal Information:
Journal Volume: 124; Journal Issue: 2; Journal ID: ISSN 2169-9380
Publisher:
American Geophysical Union
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; heliospheric and magnetospheric physics; ring current electrons; magnetospheric convection; ensemble modeling; inner magnetosphere; electron transport; wave-particle interactions

Citation Formats

Aseev, N. A., Shprits, Y. Y., Wang, D., Wygant, J., Drozdov, A. Y., Kellerman, A. C., and Reeves, G. D. Transport and Loss of Ring Current Electrons Inside Geosynchronous Orbit During the 17 March 2013 Storm. United States: N. p., 2019. Web. doi:10.1029/2018JA026031.
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Aseev, N. A., Shprits, Y. Y., Wang, D., Wygant, J., Drozdov, A. Y., Kellerman, A. C., & Reeves, G. D. Transport and Loss of Ring Current Electrons Inside Geosynchronous Orbit During the 17 March 2013 Storm. United States. https://doi.org/10.1029/2018JA026031
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Aseev, N. A., Shprits, Y. Y., Wang, D., Wygant, J., Drozdov, A. Y., Kellerman, A. C., and Reeves, G. D. Mon . "Transport and Loss of Ring Current Electrons Inside Geosynchronous Orbit During the 17 March 2013 Storm". United States. https://doi.org/10.1029/2018JA026031. https://www.osti.gov/servlets/purl/1630876.
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@article{osti_1630876,
title = {Transport and Loss of Ring Current Electrons Inside Geosynchronous Orbit During the 17 March 2013 Storm},
author = {Aseev, N. A. and Shprits, Y. Y. and Wang, D. and Wygant, J. and Drozdov, A. Y. and Kellerman, A. C. and Reeves, G. D.},
abstractNote = {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.},
doi = {10.1029/2018JA026031},
journal = {Journal of Geophysical Research. Space Physics},
number = 2,
volume = 124,
place = {United States},
year = {Mon Jan 21 00:00:00 EST 2019},
month = {Mon Jan 21 00:00:00 EST 2019}
}
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