High-latitude dayside ionosphere response to Pc5 field line resonance

International audience We report observations of pulsations due to Field Line Resonance (FLR) in the morning sector of the high-latitude dayside ionosphere on 1 February 1998. The Geotail spacecraft, ideally skimming the dayside magnetopause, monitored the magnetopause motion, which is seen to induc...

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Main Authors: Pitout, F., Eglitis, P., Blelly, P.-L.
Other Authors: Agence Spatiale Européenne = European Space Agency (ESA), Swedish Institute of Space Physics Kiruna (IRF), Centre d'étude spatiale des rayonnements (CESR), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 2003
Subjects:
Online Access:https://hal.science/hal-00329268
https://hal.science/hal-00329268/document
https://hal.science/hal-00329268/file/angeo-21-1509-2003.pdf
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spelling ftmeteofrance:oai:HAL:hal-00329268v1 2023-12-17T10:29:36+01:00 High-latitude dayside ionosphere response to Pc5 field line resonance Pitout, F. Eglitis, P. Blelly, P.-L. Agence Spatiale Européenne = European Space Agency (ESA) Swedish Institute of Space Physics Kiruna (IRF) Centre d'étude spatiale des rayonnements (CESR) Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS) 2003 https://hal.science/hal-00329268 https://hal.science/hal-00329268/document https://hal.science/hal-00329268/file/angeo-21-1509-2003.pdf en eng HAL CCSD European Geosciences Union hal-00329268 https://hal.science/hal-00329268 https://hal.science/hal-00329268/document https://hal.science/hal-00329268/file/angeo-21-1509-2003.pdf info:eu-repo/semantics/OpenAccess ISSN: 0992-7689 EISSN: 1432-0576 Annales Geophysicae https://hal.science/hal-00329268 Annales Geophysicae, 2003, 21 (7), pp.1509-1520 [SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere [SDU.STU]Sciences of the Universe [physics]/Earth Sciences info:eu-repo/semantics/article Journal articles 2003 ftmeteofrance 2023-11-21T23:42:17Z International audience We report observations of pulsations due to Field Line Resonance (FLR) in the morning sector of the high-latitude dayside ionosphere on 1 February 1998. The Geotail spacecraft, ideally skimming the dayside magnetopause, monitored the magnetopause motion, which is seen to induce a modulated response of the ionosphere by means of ULF waves. Pulsations in the Pc5 frequency range were observed in the ground magnetic field measured by the IMAGE array, as well as in the electron and ion temperatures measured by the EISCAT Svalbard Radar. The ion temperature oscillations are an indicator of a modulated convection electric field while field-aligned currents (FAC) associated with the FLR control the electron temperature. We have performed a simulation of the ionosphere experiencing sinusoidal FAC and electric field in order to confirm our hypothesis. In addition to the ionospheric response, the possible cause of the FLR and processes involved are also discussed. Article in Journal/Newspaper EISCAT Svalbard Météo-France: HAL Svalbard
institution Open Polar
collection Météo-France: HAL
op_collection_id ftmeteofrance
language English
topic [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
spellingShingle [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
Pitout, F.
Eglitis, P.
Blelly, P.-L.
High-latitude dayside ionosphere response to Pc5 field line resonance
topic_facet [SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
[SDU.STU]Sciences of the Universe [physics]/Earth Sciences
description International audience We report observations of pulsations due to Field Line Resonance (FLR) in the morning sector of the high-latitude dayside ionosphere on 1 February 1998. The Geotail spacecraft, ideally skimming the dayside magnetopause, monitored the magnetopause motion, which is seen to induce a modulated response of the ionosphere by means of ULF waves. Pulsations in the Pc5 frequency range were observed in the ground magnetic field measured by the IMAGE array, as well as in the electron and ion temperatures measured by the EISCAT Svalbard Radar. The ion temperature oscillations are an indicator of a modulated convection electric field while field-aligned currents (FAC) associated with the FLR control the electron temperature. We have performed a simulation of the ionosphere experiencing sinusoidal FAC and electric field in order to confirm our hypothesis. In addition to the ionospheric response, the possible cause of the FLR and processes involved are also discussed.
author2 Agence Spatiale Européenne = European Space Agency (ESA)
Swedish Institute of Space Physics Kiruna (IRF)
Centre d'étude spatiale des rayonnements (CESR)
Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP)
Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)
format Article in Journal/Newspaper
author Pitout, F.
Eglitis, P.
Blelly, P.-L.
author_facet Pitout, F.
Eglitis, P.
Blelly, P.-L.
author_sort Pitout, F.
title High-latitude dayside ionosphere response to Pc5 field line resonance
title_short High-latitude dayside ionosphere response to Pc5 field line resonance
title_full High-latitude dayside ionosphere response to Pc5 field line resonance
title_fullStr High-latitude dayside ionosphere response to Pc5 field line resonance
title_full_unstemmed High-latitude dayside ionosphere response to Pc5 field line resonance
title_sort high-latitude dayside ionosphere response to pc5 field line resonance
publisher HAL CCSD
publishDate 2003
url https://hal.science/hal-00329268
https://hal.science/hal-00329268/document
https://hal.science/hal-00329268/file/angeo-21-1509-2003.pdf
geographic Svalbard
geographic_facet Svalbard
genre EISCAT
Svalbard
genre_facet EISCAT
Svalbard
op_source ISSN: 0992-7689
EISSN: 1432-0576
Annales Geophysicae
https://hal.science/hal-00329268
Annales Geophysicae, 2003, 21 (7), pp.1509-1520
op_relation hal-00329268
https://hal.science/hal-00329268
https://hal.science/hal-00329268/document
https://hal.science/hal-00329268/file/angeo-21-1509-2003.pdf
op_rights info:eu-repo/semantics/OpenAccess
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