A study of particle acceleration in the auroral regions of planetary magnetospheres
Particle acceleration is a topic of general astrophysical interest which can be studied in a convenient natural laboratory: the Earth's magnetosphere and, more widely, the magnetospheres of magnetised planets. In particular, numerous physical processes occur in the auroral regions, for example...
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Other Authors: | , , , , , |
Format: | Doctoral or Postdoctoral Thesis |
Language: | French |
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HAL CCSD
1999
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Online Access: | https://tel.archives-ouvertes.fr/tel-00010474 https://tel.archives-ouvertes.fr/tel-00010474/document https://tel.archives-ouvertes.fr/tel-00010474/file/tel-00010474.pdf |
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ftccsdartic:oai:HAL:tel-00010474v1 |
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record_format |
openpolar |
institution |
Open Polar |
collection |
Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
op_collection_id |
ftccsdartic |
language |
French |
topic |
auroral regions Alfvén waves non homogeneous plasma energy dissipation numerical simulations régions aurorales ondes d'Alfvén plasma non homogène accélération dissipation d'énergie simulations numériques [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] |
spellingShingle |
auroral regions Alfvén waves non homogeneous plasma energy dissipation numerical simulations régions aurorales ondes d'Alfvén plasma non homogène accélération dissipation d'énergie simulations numériques [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] Génot, Vincent A study of particle acceleration in the auroral regions of planetary magnetospheres |
topic_facet |
auroral regions Alfvén waves non homogeneous plasma energy dissipation numerical simulations régions aurorales ondes d'Alfvén plasma non homogène accélération dissipation d'énergie simulations numériques [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] |
description |
Particle acceleration is a topic of general astrophysical interest which can be studied in a convenient natural laboratory: the Earth's magnetosphere and, more widely, the magnetospheres of magnetised planets. In particular, numerous physical processes occur in the auroral regions, for example the northern and southern auroras, which are very spectacular but rather imperfectly understood phenomena. Numerous satellite measurements have shown the existence of highly energetic populations of particles flowing towards the Earth, and this implies the existence of a strong electric potential difference which most of the proposed models fail to predict. Generally speaking, an understanding of this acceleration is necessary to explain the dynamic coupling between the magnetosphere, where the energy is released during substorms, and ionosphere where the energy is dissipated. The study of the dissipation, which takes place on short spatial and temporal scales, constitutes the main theme of the present work. We consider as electromagnetic perturbation an Alfvén wave propagating along the geomagnetic field lines. Its interaction, in the auroral zones, with the highly inhomogeneous structures known as plasma cavities, leads to the formation of parallel electric fields able to accelerate particles, as well as to a significant energy transfer from the waves to the electrons. Finally, this study enables us to suggest a new scenario for the formation of auroral arcs. This work was conducted both analytically and numerically using a "particles in cell" code. L'accélération de particules est une thématique d'astrophysique générale qui peut être étudiée dans un laboratoire naturel : les régions aurorales de la Terre, et plus globalement, celles des planètes magnétisées. Ces régions sont en effet le siège de nombreux processus qui donnent, entre autres, naissance aux aurores boréales et australes, phénomènes spectaculaires mais dont de nombreux aspects restent incompris. En particulier, de multiples mesures de satellites ont ... |
author2 |
Centre d'étude spatiale des rayonnements (CESR) Observatoire Midi-Pyrénées (OMP) Météo France-Centre National d'Études Spatiales Toulouse (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales Toulouse (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3) Université Fédérale Toulouse Midi-Pyrénées Université de Versailles-Saint Quentin en Yvelines Le Quéau Dominique |
format |
Doctoral or Postdoctoral Thesis |
author |
Génot, Vincent |
author_facet |
Génot, Vincent |
author_sort |
Génot, Vincent |
title |
A study of particle acceleration in the auroral regions of planetary magnetospheres |
title_short |
A study of particle acceleration in the auroral regions of planetary magnetospheres |
title_full |
A study of particle acceleration in the auroral regions of planetary magnetospheres |
title_fullStr |
A study of particle acceleration in the auroral regions of planetary magnetospheres |
title_full_unstemmed |
A study of particle acceleration in the auroral regions of planetary magnetospheres |
title_sort |
study of particle acceleration in the auroral regions of planetary magnetospheres |
publisher |
HAL CCSD |
publishDate |
1999 |
url |
https://tel.archives-ouvertes.fr/tel-00010474 https://tel.archives-ouvertes.fr/tel-00010474/document https://tel.archives-ouvertes.fr/tel-00010474/file/tel-00010474.pdf |
genre |
aurores boréales |
genre_facet |
aurores boréales |
op_source |
https://tel.archives-ouvertes.fr/tel-00010474 Astrophysique [astro-ph]. Université de Versailles-Saint Quentin en Yvelines, 1999. Français |
op_relation |
tel-00010474 https://tel.archives-ouvertes.fr/tel-00010474 https://tel.archives-ouvertes.fr/tel-00010474/document https://tel.archives-ouvertes.fr/tel-00010474/file/tel-00010474.pdf |
op_rights |
info:eu-repo/semantics/OpenAccess |
_version_ |
1766364495867805696 |
spelling |
ftccsdartic:oai:HAL:tel-00010474v1 2023-05-15T15:33:54+02:00 A study of particle acceleration in the auroral regions of planetary magnetospheres Étude des phénomènes d'accélération de particules dans les régions aurorales des magnétosphères Génot, Vincent Centre d'étude spatiale des rayonnements (CESR) Observatoire Midi-Pyrénées (OMP) Météo France-Centre National d'Études Spatiales Toulouse (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales Toulouse (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3) Université Fédérale Toulouse Midi-Pyrénées Université de Versailles-Saint Quentin en Yvelines Le Quéau Dominique 1999-06-30 https://tel.archives-ouvertes.fr/tel-00010474 https://tel.archives-ouvertes.fr/tel-00010474/document https://tel.archives-ouvertes.fr/tel-00010474/file/tel-00010474.pdf fr fre HAL CCSD tel-00010474 https://tel.archives-ouvertes.fr/tel-00010474 https://tel.archives-ouvertes.fr/tel-00010474/document https://tel.archives-ouvertes.fr/tel-00010474/file/tel-00010474.pdf info:eu-repo/semantics/OpenAccess https://tel.archives-ouvertes.fr/tel-00010474 Astrophysique [astro-ph]. Université de Versailles-Saint Quentin en Yvelines, 1999. Français auroral regions Alfvén waves non homogeneous plasma energy dissipation numerical simulations régions aurorales ondes d'Alfvén plasma non homogène accélération dissipation d'énergie simulations numériques [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/doctoralThesis Theses 1999 ftccsdartic 2021-10-24T23:51:34Z Particle acceleration is a topic of general astrophysical interest which can be studied in a convenient natural laboratory: the Earth's magnetosphere and, more widely, the magnetospheres of magnetised planets. In particular, numerous physical processes occur in the auroral regions, for example the northern and southern auroras, which are very spectacular but rather imperfectly understood phenomena. Numerous satellite measurements have shown the existence of highly energetic populations of particles flowing towards the Earth, and this implies the existence of a strong electric potential difference which most of the proposed models fail to predict. Generally speaking, an understanding of this acceleration is necessary to explain the dynamic coupling between the magnetosphere, where the energy is released during substorms, and ionosphere where the energy is dissipated. The study of the dissipation, which takes place on short spatial and temporal scales, constitutes the main theme of the present work. We consider as electromagnetic perturbation an Alfvén wave propagating along the geomagnetic field lines. Its interaction, in the auroral zones, with the highly inhomogeneous structures known as plasma cavities, leads to the formation of parallel electric fields able to accelerate particles, as well as to a significant energy transfer from the waves to the electrons. Finally, this study enables us to suggest a new scenario for the formation of auroral arcs. This work was conducted both analytically and numerically using a "particles in cell" code. L'accélération de particules est une thématique d'astrophysique générale qui peut être étudiée dans un laboratoire naturel : les régions aurorales de la Terre, et plus globalement, celles des planètes magnétisées. Ces régions sont en effet le siège de nombreux processus qui donnent, entre autres, naissance aux aurores boréales et australes, phénomènes spectaculaires mais dont de nombreux aspects restent incompris. En particulier, de multiples mesures de satellites ont ... Doctoral or Postdoctoral Thesis aurores boréales Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |