Bow shock specularly reflected ions in the presence of low-frequency electromagnetic waves: a case study
An energetic ion (<i>E</i>≤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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Copernicus Publications
2004-07-01
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Series: | Annales Geophysicae |
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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>≤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 θ<sub><i>Bn0</i></sub> is about ~30°. 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 α<sub>0</sub>~θ<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 θ<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 θ<sub><i>Bn</i></sub> angles are less than ~40°, 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>≤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 θ<sub><i>Bn0</i></sub> is about
~30°.
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 α<sub>0</sub>~θ<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 θ<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 θ<sub><i>Bn</i></sub> angles are less than ~40°, 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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