Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study

An energetic ion (<i>E</i>&le;40) event observed by the CLUSTER/CIS experiment upstream of the Earth's bow shock is studied in detail. The ion event is observed in association with quasi-monochromatic ULF MHD-like waves, which we show modulate the ion fluxes. According to th...

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Main Authors: K. Meziane, C. Mazelle, M. Wilber, D. LeQuéau, J. P. Eastwood, H. Rème, I. Dandouras, J. A. Sauvaud, J. M. Bosqued, G. K. Parks, L. M. Kistler, M. McCarthy, B. Klecker, A. Korth, M.-B. Bavassano-Cattaneo, R. Lundin, A. Balogh
Format: Article
Language:English
Published: Copernicus Publications 2004-07-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/22/2325/2004/angeo-22-2325-2004.pdf
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spelling doaj-16399d111e1746b3b8a14d922cb64a552020-11-24T21:46:44ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762004-07-01222325233510.5194/angeo-22-2325-2004Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case studyK. Meziane0C. Mazelle1M. Wilber2D. LeQuéau3J. P. Eastwood4H. Rème5I. Dandouras6J. A. Sauvaud7J. M. Bosqued8G. K. Parks9L. M. Kistler10M. McCarthy11B. Klecker12A. Korth13M.-B. Bavassano-Cattaneo14R. Lundin15A. Balogh16Physics Department, University of New Brunswick, CanadaCentre d’Etudes Spatiales des Rayonnements, 9 Avenue du Colonel Roche, Toulouse, 31028, FranceSpace Sciences Laboratory, University of California, Berkeley 94720, USACentre d’Etudes Spatiales des Rayonnements, 9 Avenue du Colonel Roche, Toulouse, 31028, FranceSpace and Atmospheric Physics, The Blackett Laboratory, Imperial College, London, SW7 2BW, UKCentre d’Etudes Spatiales des Rayonnements, 9 Avenue du Colonel Roche, Toulouse, 31028, FranceCentre d’Etudes Spatiales des Rayonnements, 9 Avenue du Colonel Roche, Toulouse, 31028, FranceCentre d’Etudes Spatiales des Rayonnements, 9 Avenue du Colonel Roche, Toulouse, 31028, FranceCentre d’Etudes Spatiales des Rayonnements, 9 Avenue du Colonel Roche, Toulouse, 31028, FranceSpace Sciences Laboratory, University of California, Berkeley 94720, USASpace Science Center, University of New Hamshire, Durham, 03824, USAEarth and Space Sciences, University of Washington, Seattle, 98195, USAMPI für Extraterrestrische Physik, Garching, 85741, GermanyMPI für Aeronomie, Katlenburg-Lindau, 37191, GermanyCNR-IFSI, Roma, 00133, ItalySwedish Institute of Space Physics, Kiruna, 98128, SwedenSpace and Atmospheric Physics, The Blackett Laboratory, Imperial College, London, SW7 2BW, UKAn energetic ion (<i>E</i>&le;40) event observed by the CLUSTER/CIS experiment upstream of the Earth's bow shock is studied in detail. The ion event is observed in association with quasi-monochromatic ULF MHD-like waves, which we show modulate the ion fluxes. According to three statistical bow shock position models, the Cluster spacecrafts are located at ~0.5 <i>R<sub>e</sub></i> from the shock and the averaged bow shock &theta;<sub><i>Bn0</i></sub> is about ~30&deg;. The analysis of the three-dimensional angular distribution indicates that ions propagating roughly along the magnetic field direction are observed at the onset of the event. Later on, the angular distribution is gyrophase-bunched and the pitch-angle distribution is peaked at &alpha;<sub>0</sub>~&theta;<sub><i>Bn0</i></sub>, consistent with the specular reflection production mechanism. The analysis of the waves shows that they are left-handed in the spacecraft frame of reference (right-handed in the solar wind frame) and propagate roughly along the ambient magnetic field; we have found that they are in cyclotron-resonance with the field-aligned beam observed just upstream. Using properties of the waves and particles, we explain the observed particle flux-modulation in the context of &theta;<sub><i>Bn</i></sub> changes at the shock caused by the convected ULF waves. We have found that the high count rates coincide with particles leaving the shock when &theta;<sub><i>Bn</i></sub> angles are less than ~40&deg;, consistent with the specular reflection hypothesis as the production mechanism of ions.https://www.ann-geophys.net/22/2325/2004/angeo-22-2325-2004.pdf
collection DOAJ
language English
format Article
sources DOAJ
author K. Meziane
C. Mazelle
M. Wilber
D. LeQuéau
J. P. Eastwood
H. Rème
I. Dandouras
J. A. Sauvaud
J. M. Bosqued
G. K. Parks
L. M. Kistler
M. McCarthy
B. Klecker
A. Korth
M.-B. Bavassano-Cattaneo
R. Lundin
A. Balogh
spellingShingle K. Meziane
C. Mazelle
M. Wilber
D. LeQuéau
J. P. Eastwood
H. Rème
I. Dandouras
J. A. Sauvaud
J. M. Bosqued
G. K. Parks
L. M. Kistler
M. McCarthy
B. Klecker
A. Korth
M.-B. Bavassano-Cattaneo
R. Lundin
A. Balogh
Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study
Annales Geophysicae
author_facet K. Meziane
C. Mazelle
M. Wilber
D. LeQuéau
J. P. Eastwood
H. Rème
I. Dandouras
J. A. Sauvaud
J. M. Bosqued
G. K. Parks
L. M. Kistler
M. McCarthy
B. Klecker
A. Korth
M.-B. Bavassano-Cattaneo
R. Lundin
A. Balogh
author_sort K. Meziane
title Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study
title_short Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study
title_full Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study
title_fullStr Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study
title_full_unstemmed Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study
title_sort bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
publishDate 2004-07-01
description An energetic ion (<i>E</i>&le;40) event observed by the CLUSTER/CIS experiment upstream of the Earth's bow shock is studied in detail. The ion event is observed in association with quasi-monochromatic ULF MHD-like waves, which we show modulate the ion fluxes. According to three statistical bow shock position models, the Cluster spacecrafts are located at ~0.5 <i>R<sub>e</sub></i> from the shock and the averaged bow shock &theta;<sub><i>Bn0</i></sub> is about ~30&deg;. The analysis of the three-dimensional angular distribution indicates that ions propagating roughly along the magnetic field direction are observed at the onset of the event. Later on, the angular distribution is gyrophase-bunched and the pitch-angle distribution is peaked at &alpha;<sub>0</sub>~&theta;<sub><i>Bn0</i></sub>, consistent with the specular reflection production mechanism. The analysis of the waves shows that they are left-handed in the spacecraft frame of reference (right-handed in the solar wind frame) and propagate roughly along the ambient magnetic field; we have found that they are in cyclotron-resonance with the field-aligned beam observed just upstream. Using properties of the waves and particles, we explain the observed particle flux-modulation in the context of &theta;<sub><i>Bn</i></sub> changes at the shock caused by the convected ULF waves. We have found that the high count rates coincide with particles leaving the shock when &theta;<sub><i>Bn</i></sub> angles are less than ~40&deg;, consistent with the specular reflection hypothesis as the production mechanism of ions.
url https://www.ann-geophys.net/22/2325/2004/angeo-22-2325-2004.pdf
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