Relativistic surfatron process for Landau resonant electrons in radiation belts

Recent theoretical studies of the nonlinear wave-particle interactions for relativistic particles have shown that Landau resonant orbits could be efficiently accelerated along the mean background magnetic field for propagation angles θ in close proximity to a critical propagation &theta;<sub&...

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Main Authors: A. Osmane, A. M. Hamza
Format: Article
Language:English
Published: Copernicus Publications 2014-01-01
Series:Nonlinear Processes in Geophysics
Online Access:http://www.nonlin-processes-geophys.net/21/115/2014/npg-21-115-2014.pdf
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author A. Osmane
A. M. Hamza
author_facet A. Osmane
A. M. Hamza
author_sort A. Osmane
collection DOAJ
description Recent theoretical studies of the nonlinear wave-particle interactions for relativistic particles have shown that Landau resonant orbits could be efficiently accelerated along the mean background magnetic field for propagation angles θ in close proximity to a critical propagation &theta;<sub>c</sub> associated with a Hopf–Hopf bifurcation condition. In this report, we extend previous studies to reach greater modeling capacities for the study of electrons in radiation belts by including longitudinal wave effects and inhomogeneous magnetic fields. We find that even though both effects can limit the surfatron acceleration of electrons in radiation belts, gains in energy of the order of 100 keV, taking place on one tenth of a millisecond, are sufficiently strong for the mechanism to be relevant to radiation belt dynamics.
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spelling doaj.art-791fef5efc89430fa82687a8b1539eb32022-12-21T18:43:33ZengCopernicus PublicationsNonlinear Processes in Geophysics1023-58091607-79462014-01-0121111512510.5194/npg-21-115-2014Relativistic surfatron process for Landau resonant electrons in radiation beltsA. Osmane0A. M. Hamza1University of New Brunswick, Physics Department, Fredericton, New Brunswick, CanadaUniversity of New Brunswick, Physics Department, Fredericton, New Brunswick, CanadaRecent theoretical studies of the nonlinear wave-particle interactions for relativistic particles have shown that Landau resonant orbits could be efficiently accelerated along the mean background magnetic field for propagation angles θ in close proximity to a critical propagation &theta;<sub>c</sub> associated with a Hopf–Hopf bifurcation condition. In this report, we extend previous studies to reach greater modeling capacities for the study of electrons in radiation belts by including longitudinal wave effects and inhomogeneous magnetic fields. We find that even though both effects can limit the surfatron acceleration of electrons in radiation belts, gains in energy of the order of 100 keV, taking place on one tenth of a millisecond, are sufficiently strong for the mechanism to be relevant to radiation belt dynamics.http://www.nonlin-processes-geophys.net/21/115/2014/npg-21-115-2014.pdf
spellingShingle A. Osmane
A. M. Hamza
Relativistic surfatron process for Landau resonant electrons in radiation belts
Nonlinear Processes in Geophysics
title Relativistic surfatron process for Landau resonant electrons in radiation belts
title_full Relativistic surfatron process for Landau resonant electrons in radiation belts
title_fullStr Relativistic surfatron process for Landau resonant electrons in radiation belts
title_full_unstemmed Relativistic surfatron process for Landau resonant electrons in radiation belts
title_short Relativistic surfatron process for Landau resonant electrons in radiation belts
title_sort relativistic surfatron process for landau resonant electrons in radiation belts
url http://www.nonlin-processes-geophys.net/21/115/2014/npg-21-115-2014.pdf
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