Electrostatic shock properties inferred from AKR fine structure

The auroral kilometric radiation (AKR) consists of a large number of fast drifting elementary radiation events that have been interpreted as travelling electron holes resulting from the nonlinear evolution of electron-acoustic waves. The elementary radiation structures sometimes become reflected...

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Main Authors: R. Pottelette, R. A. Treumann, M. Berthomier, J. Jasperse
Format: Article
Language:English
Published: Copernicus Publications 2003-01-01
Series:Nonlinear Processes in Geophysics
Online Access:http://www.nonlin-processes-geophys.net/10/87/2003/npg-10-87-2003.pdf
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author R. Pottelette
R. A. Treumann
M. Berthomier
J. Jasperse
author_facet R. Pottelette
R. A. Treumann
M. Berthomier
J. Jasperse
author_sort R. Pottelette
collection DOAJ
description The auroral kilometric radiation (AKR) consists of a large number of fast drifting elementary radiation events that have been interpreted as travelling electron holes resulting from the nonlinear evolution of electron-acoustic waves. The elementary radiation structures sometimes become reflected or trapped in slowly drifting larger structures where the parallel electric fields are located. These latter features have spectral frequency drifts which can be interpreted in terms of the propagation of shock-like disturbances along the auroral field line at velocities near the ion-acoustic speed. The amplitude, speed, and shock width of such localized ion-acoustic shocks are determined here in the fluid approximation from the Sagdeev potential, assuming realistic plasma parameters. It is emphasized that the electrostatic potentials of such nonlinear structures contribute to auroral acceleration.
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spelling doaj.art-6b6614f66bde41dd9061357371ca67d72022-12-21T21:52:38ZengCopernicus PublicationsNonlinear Processes in Geophysics1023-58091607-79462003-01-01101/28792Electrostatic shock properties inferred from AKR fine structureR. PotteletteR. A. TreumannM. BerthomierJ. JasperseThe auroral kilometric radiation (AKR) consists of a large number of fast drifting elementary radiation events that have been interpreted as travelling electron holes resulting from the nonlinear evolution of electron-acoustic waves. The elementary radiation structures sometimes become reflected or trapped in slowly drifting larger structures where the parallel electric fields are located. These latter features have spectral frequency drifts which can be interpreted in terms of the propagation of shock-like disturbances along the auroral field line at velocities near the ion-acoustic speed. The amplitude, speed, and shock width of such localized ion-acoustic shocks are determined here in the fluid approximation from the Sagdeev potential, assuming realistic plasma parameters. It is emphasized that the electrostatic potentials of such nonlinear structures contribute to auroral acceleration.http://www.nonlin-processes-geophys.net/10/87/2003/npg-10-87-2003.pdf
spellingShingle R. Pottelette
R. A. Treumann
M. Berthomier
J. Jasperse
Electrostatic shock properties inferred from AKR fine structure
Nonlinear Processes in Geophysics
title Electrostatic shock properties inferred from AKR fine structure
title_full Electrostatic shock properties inferred from AKR fine structure
title_fullStr Electrostatic shock properties inferred from AKR fine structure
title_full_unstemmed Electrostatic shock properties inferred from AKR fine structure
title_short Electrostatic shock properties inferred from AKR fine structure
title_sort electrostatic shock properties inferred from akr fine structure
url http://www.nonlin-processes-geophys.net/10/87/2003/npg-10-87-2003.pdf
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AT ratreumann electrostaticshockpropertiesinferredfromakrfinestructure
AT mberthomier electrostaticshockpropertiesinferredfromakrfinestructure
AT jjasperse electrostaticshockpropertiesinferredfromakrfinestructure