Strong atmospheric disturbances as a possible origin of inner zone particle diffusion
A new mechanism of the atmosphere-magnetosphere interaction, which might be called "acoustic-magnetospheric cyclotron accelerator", is proposed. The idea of this mechanism stems from the fact that strong acoustical perturbations in the ionosphere (e.g., due to earthquakes, thun...
Main Authors: | , , |
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Format: | Article |
Language: | English |
Published: |
Copernicus Publications
1999-04-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/17/526/1999/angeo-17-526-1999.pdf |
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author | O. A. Pokhotelov V. A. Pilipenko M. Parrot |
author_facet | O. A. Pokhotelov V. A. Pilipenko M. Parrot |
author_sort | O. A. Pokhotelov |
collection | DOAJ |
description | A new mechanism of the
atmosphere-magnetosphere interaction, which might be called
"acoustic-magnetospheric cyclotron accelerator", is proposed. The idea
of this mechanism stems from the fact that strong acoustical perturbations in
the ionosphere (e.g., due to earthquakes, thunderstorms, etc.) may generate
magnetic disturbances in the magnetosphere. Then, the latter will induce local
resonant acceleration and subsequent inward diffusion of trapped particles. This
idea may be fruitful in the interpretation of some occasional increases in inner
zone particle fluxes which do not correlate with the solar or magnetospheric
activities.<br><br><b>Key words.</b> Ionosphere (active experiments;
ionosphere-atmosphere interactions; particle acceleration) |
first_indexed | 2024-12-10T14:07:52Z |
format | Article |
id | doaj.art-be0d501ec6a0401599f97382d9d4dcfd |
institution | Directory Open Access Journal |
issn | 0992-7689 1432-0576 |
language | English |
last_indexed | 2024-12-10T14:07:52Z |
publishDate | 1999-04-01 |
publisher | Copernicus Publications |
record_format | Article |
series | Annales Geophysicae |
spelling | doaj.art-be0d501ec6a0401599f97382d9d4dcfd2022-12-22T01:45:35ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05761999-04-011752653210.1007/s00585-999-0526-2Strong atmospheric disturbances as a possible origin of inner zone particle diffusionO. A. Pokhotelov0V. A. Pilipenko1M. Parrot2Institute of the Physics of the Earth, Moscow 123810, RussiaInstitute of the Physics of the Earth, Moscow 123810, RussiaLaboratoire de Physique et Chimie de l'Environnement, CNRS, 3A av. de la Recherche Scientifique, F-45071 Orléans, France, e-mail: mparrot@cnrs-orleans.frA new mechanism of the atmosphere-magnetosphere interaction, which might be called "acoustic-magnetospheric cyclotron accelerator", is proposed. The idea of this mechanism stems from the fact that strong acoustical perturbations in the ionosphere (e.g., due to earthquakes, thunderstorms, etc.) may generate magnetic disturbances in the magnetosphere. Then, the latter will induce local resonant acceleration and subsequent inward diffusion of trapped particles. This idea may be fruitful in the interpretation of some occasional increases in inner zone particle fluxes which do not correlate with the solar or magnetospheric activities.<br><br><b>Key words.</b> Ionosphere (active experiments; ionosphere-atmosphere interactions; particle acceleration)https://www.ann-geophys.net/17/526/1999/angeo-17-526-1999.pdf |
spellingShingle | O. A. Pokhotelov V. A. Pilipenko M. Parrot Strong atmospheric disturbances as a possible origin of inner zone particle diffusion Annales Geophysicae |
title | Strong atmospheric disturbances as a possible origin of inner zone particle diffusion |
title_full | Strong atmospheric disturbances as a possible origin of inner zone particle diffusion |
title_fullStr | Strong atmospheric disturbances as a possible origin of inner zone particle diffusion |
title_full_unstemmed | Strong atmospheric disturbances as a possible origin of inner zone particle diffusion |
title_short | Strong atmospheric disturbances as a possible origin of inner zone particle diffusion |
title_sort | strong atmospheric disturbances as a possible origin of inner zone particle diffusion |
url | https://www.ann-geophys.net/17/526/1999/angeo-17-526-1999.pdf |
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