Quantifying the effect of magnetopause shadowing on electron radiation belt dropouts

Energetic radiation belt electron fluxes can undergo sudden dropouts in response to different solar wind drivers. Many physical processes contribute to the electron flux dropout, but their respective roles in the net electron depletion remain a fundamental puzzle. Some previous studies have qual...

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Main Authors: Y. Yu, J. Koller, S. K. Morley
Format: Article
Language:English
Published: Copernicus Publications 2013-11-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/31/1929/2013/angeo-31-1929-2013.pdf
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spelling doaj-a557f310fbe840edbeee6402079a70c82020-11-25T00:06:41ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762013-11-01311929193910.5194/angeo-31-1929-2013Quantifying the effect of magnetopause shadowing on electron radiation belt dropoutsY. Yu0J. Koller1S. K. Morley2Space Science and Application, Los Alamos National Laboratory, Los Alamos, NM, USASpace Science and Application, Los Alamos National Laboratory, Los Alamos, NM, USASpace Science and Application, Los Alamos National Laboratory, Los Alamos, NM, USAEnergetic radiation belt electron fluxes can undergo sudden dropouts in response to different solar wind drivers. Many physical processes contribute to the electron flux dropout, but their respective roles in the net electron depletion remain a fundamental puzzle. Some previous studies have qualitatively examined the importance of magnetopause shadowing in the sudden dropouts either from observations or from simulations. While it is difficult to directly measure the electron flux loss into the solar wind, radial diffusion codes with a fixed boundary location (commonly utilized in the literature) are not able to explicitly account for magnetopause shadowing. The exact percentage of its contribution has therefore not yet been resolved. To overcome these limitations and to determine the exact contribution in percentage, we carry out radial diffusion simulations with the magnetopause shadowing effect explicitly accounted for during a superposed solar wind stream interface passage, and quantify the relative contribution of the magnetopause shadowing coupled with outward radial diffusion by comparing with GPS-observed total flux dropout. Results indicate that during high-speed solar wind stream events, which are typically preceded by enhanced dynamic pressure and hence a compressed magnetosphere, magnetopause shadowing coupled with the outward radial diffusion can explain about 60–99% of the main-phase radiation belt electron depletion near the geosynchronous orbit. While the outer region (<i>L</i><sup>*</sup> > 5) can nearly be explained by the above coupled mechanism, additional loss mechanisms are needed to fully explain the energetic electron loss for the inner region (<i>L</i><sup>*</sup> &leq; 5). While this conclusion confirms earlier studies, our quantification study demonstrates its relative importance with respect to other mechanisms at different locations.https://www.ann-geophys.net/31/1929/2013/angeo-31-1929-2013.pdf
collection DOAJ
language English
format Article
sources DOAJ
author Y. Yu
J. Koller
S. K. Morley
spellingShingle Y. Yu
J. Koller
S. K. Morley
Quantifying the effect of magnetopause shadowing on electron radiation belt dropouts
Annales Geophysicae
author_facet Y. Yu
J. Koller
S. K. Morley
author_sort Y. Yu
title Quantifying the effect of magnetopause shadowing on electron radiation belt dropouts
title_short Quantifying the effect of magnetopause shadowing on electron radiation belt dropouts
title_full Quantifying the effect of magnetopause shadowing on electron radiation belt dropouts
title_fullStr Quantifying the effect of magnetopause shadowing on electron radiation belt dropouts
title_full_unstemmed Quantifying the effect of magnetopause shadowing on electron radiation belt dropouts
title_sort quantifying the effect of magnetopause shadowing on electron radiation belt dropouts
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2013-11-01
description Energetic radiation belt electron fluxes can undergo sudden dropouts in response to different solar wind drivers. Many physical processes contribute to the electron flux dropout, but their respective roles in the net electron depletion remain a fundamental puzzle. Some previous studies have qualitatively examined the importance of magnetopause shadowing in the sudden dropouts either from observations or from simulations. While it is difficult to directly measure the electron flux loss into the solar wind, radial diffusion codes with a fixed boundary location (commonly utilized in the literature) are not able to explicitly account for magnetopause shadowing. The exact percentage of its contribution has therefore not yet been resolved. To overcome these limitations and to determine the exact contribution in percentage, we carry out radial diffusion simulations with the magnetopause shadowing effect explicitly accounted for during a superposed solar wind stream interface passage, and quantify the relative contribution of the magnetopause shadowing coupled with outward radial diffusion by comparing with GPS-observed total flux dropout. Results indicate that during high-speed solar wind stream events, which are typically preceded by enhanced dynamic pressure and hence a compressed magnetosphere, magnetopause shadowing coupled with the outward radial diffusion can explain about 60–99% of the main-phase radiation belt electron depletion near the geosynchronous orbit. While the outer region (<i>L</i><sup>*</sup> > 5) can nearly be explained by the above coupled mechanism, additional loss mechanisms are needed to fully explain the energetic electron loss for the inner region (<i>L</i><sup>*</sup> &leq; 5). While this conclusion confirms earlier studies, our quantification study demonstrates its relative importance with respect to other mechanisms at different locations.
url https://www.ann-geophys.net/31/1929/2013/angeo-31-1929-2013.pdf
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