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Review of modeling of losses and sources of relativistic electrons in the outer radiation belt I: Radial transport

Shprits Y. Y., S. R. Elkington, N. P. Meredith, D. A. Subbotin, (2008), Review of modeling of losses and sources of relativistic electrons in the outer radiation belt I: Radial transport, Journal Of Atmospheric And Solar-terrestrial Physics, 70, 1679 – 1693, doi:10.1016/j.jastp.2008.06.008, Dynamic Variability of Earth’s Radiation Belts

Abstract

In this paper, we focus on the modeling of radial transport in the Earth's outer radiation belt. A historical overview of the first observations of the radiation belts is presented, followed by a brief description of radial diffusion. We describe how resonant interactions with poloidal and toroidal components of the ULF waves can change the electron's energy and provide radial displacements. We also present radial diffusion and guiding center simulations that show the importance of radial transport in redistributing relativistic electron fluxes and also in accelerating and decelerating radiation belt electrons. We conclude by presenting guiding center simulations of the coupled particle tracing and magnetohydrodynamic (MHD) codes and by discussing the origin of relativistic electrons at geosynchronous orbit. Local acceleration and losses and 3D simulations of the dynamics of the radiation belt fluxes are discussed in the companion paper [Shprits, Y.Y., Subbotin, D.A., Meredith, N.P., Elkington, S.R., 2008. Review of modeling of losses and sources of relativistic electrons in the outer radiation belt II: Local acceleration and loss. Journal of Atmospheric and Solar-Terrestrial Physics, this issue. doi:10.1016/j.jastp.2008.06.014].

Authors (sorted by name)

Elkington Meredith Shprits Subbotin

Journal / Conference

Journal Of Atmospheric And Solar-terrestrial Physics

Acknowledgments

This research was supported by NSF GEM grants ATM-0603191 and NASA LWS grant NNX06AB84G. The authors would like to thank Richard M. Thorne and Michael Schulz for stimulating discussions.

Grants

ATM‐0603191 NNX06AB84G

Bibtex

@article{SHPRITS20081679,
title = "Review of modeling of losses and sources of relativistic electrons in the outer radiation belt I: Radial transport",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
volume = "70",
number = "14",
pages = "1679 - 1693",
year = "2008",
note = "Dynamic Variability of Earth's Radiation Belts",
issn = "1364-6826",
doi = "10.1016/j.jastp.2008.06.008",
url = "http://www.sciencedirect.com/science/article/pii/S1364682608001648",
author = "Yuri Y. Shprits and Scot R. Elkington and Nigel P. Meredith and Dmitriy A. Subbotin",
keywords = "Radiation belt, Modeling, Radial diffusion",
abstract = "In this paper, we focus on the modeling of radial transport in the Earth's outer radiation belt. A historical overview of the first observations of the radiation belts is presented, followed by a brief description of radial diffusion. We describe how resonant interactions with poloidal and toroidal components of the ULF waves can change the electron's energy and provide radial displacements. We also present radial diffusion and guiding center simulations that show the importance of radial transport in redistributing relativistic electron fluxes and also in accelerating and decelerating radiation belt electrons. We conclude by presenting guiding center simulations of the coupled particle tracing and magnetohydrodynamic (MHD) codes and by discussing the origin of relativistic electrons at geosynchronous orbit. Local acceleration and losses and 3D simulations of the dynamics of the radiation belt fluxes are discussed in the companion paper [Shprits, Y.Y., Subbotin, D.A., Meredith, N.P., Elkington, S.R., 2008. Review of modeling of losses and sources of relativistic electrons in the outer radiation belt II: Local acceleration and loss. Journal of Atmospheric and Solar-Terrestrial Physics, this issue. doi:10.1016/j.jastp.2008.06.014]."
}