Generation of resonant Alfvén waves in the auroral oval

Many independent observations have shown that resonant field line Pc5 pulsations (typical periods of about several minutes) are preferably excited inside the auroral oval. Consideration of the most evident interpretation schemes shows that there is no simple explanation of this effect. Here we con...

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Main Authors: V. A. Pilipenko, D. Yu. Klimushkin, P. N. Mager, M. J. Engebretson, O. V. Kozyreva
Format: Article
Language:English
Published: Copernicus Publications 2016-02-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/34/241/2016/angeo-34-241-2016.pdf
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author V. A. Pilipenko
V. A. Pilipenko
D. Yu. Klimushkin
P. N. Mager
M. J. Engebretson
O. V. Kozyreva
O. V. Kozyreva
author_facet V. A. Pilipenko
V. A. Pilipenko
D. Yu. Klimushkin
P. N. Mager
M. J. Engebretson
O. V. Kozyreva
O. V. Kozyreva
author_sort V. A. Pilipenko
collection DOAJ
description Many independent observations have shown that resonant field line Pc5 pulsations (typical periods of about several minutes) are preferably excited inside the auroral oval. Consideration of the most evident interpretation schemes shows that there is no simple explanation of this effect. Here we consider theoretically the generation of toroidal Pc5 Alfvén waves by fluctuating magnetospheric field-aligned currents. It is shown that the Alfvén wave latitudinal structure has the same features as in the case of the classical field line resonance driven by external sources: a peak localized in latitude and a 180° phase shift across the resonant magnetic shell. This model suggests an additional mechanism of ultra-low-frequency (ULF) wave excitation which can operate at auroral latitudes.
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spelling doaj.art-4d275f45ff1a4da9be204532770fba242022-12-21T23:20:57ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762016-02-013424124810.5194/angeo-34-241-2016Generation of resonant Alfvén waves in the auroral ovalV. A. Pilipenko0V. A. Pilipenko1D. Yu. Klimushkin2P. N. Mager3M. J. Engebretson4O. V. Kozyreva5O. V. Kozyreva6Institute of Physics of the Earth, 123242 Moscow, RussiaSpace Research Institute, 117997 Moscow, RussiaInstitute of Solar-Terrestrial Physics, 664033 Irkutsk, RussiaInstitute of Solar-Terrestrial Physics, 664033 Irkutsk, RussiaAugsburg College, Minneapolis, MN 55454, USAInstitute of Physics of the Earth, 123242 Moscow, RussiaSpace Research Institute, 117997 Moscow, RussiaMany independent observations have shown that resonant field line Pc5 pulsations (typical periods of about several minutes) are preferably excited inside the auroral oval. Consideration of the most evident interpretation schemes shows that there is no simple explanation of this effect. Here we consider theoretically the generation of toroidal Pc5 Alfvén waves by fluctuating magnetospheric field-aligned currents. It is shown that the Alfvén wave latitudinal structure has the same features as in the case of the classical field line resonance driven by external sources: a peak localized in latitude and a 180° phase shift across the resonant magnetic shell. This model suggests an additional mechanism of ultra-low-frequency (ULF) wave excitation which can operate at auroral latitudes.https://www.ann-geophys.net/34/241/2016/angeo-34-241-2016.pdf
spellingShingle V. A. Pilipenko
V. A. Pilipenko
D. Yu. Klimushkin
P. N. Mager
M. J. Engebretson
O. V. Kozyreva
O. V. Kozyreva
Generation of resonant Alfvén waves in the auroral oval
Annales Geophysicae
title Generation of resonant Alfvén waves in the auroral oval
title_full Generation of resonant Alfvén waves in the auroral oval
title_fullStr Generation of resonant Alfvén waves in the auroral oval
title_full_unstemmed Generation of resonant Alfvén waves in the auroral oval
title_short Generation of resonant Alfvén waves in the auroral oval
title_sort generation of resonant alfven waves in the auroral oval
url https://www.ann-geophys.net/34/241/2016/angeo-34-241-2016.pdf
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