Pi 2 waves simultaneously observed by Cluster and CPMN ground-based magnetometers near the plasmapause

We have analyzed an event on 14 February 2003 in which Cluster satellites and the CPMN ground magnetometer chain made simultaneous observations of a Pi 2 pulsation along the same meridian. Three of the four Cluster satellites were located outside the plasmasphere, while the other one was located...

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Main Authors: H. Kawano, S. Ohtani, T. Uozumi, T. Tokunaga, A. Yoshikawa, K. Yumoto, E. A. Lucek, M. André, the CPMN group
Format: Article
Language:English
Published: Copernicus Publications 2011-09-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/29/1663/2011/angeo-29-1663-2011.pdf
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author H. Kawano
H. Kawano
S. Ohtani
T. Uozumi
T. Tokunaga
T. Tokunaga
A. Yoshikawa
A. Yoshikawa
K. Yumoto
K. Yumoto
E. A. Lucek
M. André
the CPMN group
author_facet H. Kawano
H. Kawano
S. Ohtani
T. Uozumi
T. Tokunaga
T. Tokunaga
A. Yoshikawa
A. Yoshikawa
K. Yumoto
K. Yumoto
E. A. Lucek
M. André
the CPMN group
author_sort H. Kawano
collection DOAJ
description We have analyzed an event on 14 February 2003 in which Cluster satellites and the CPMN ground magnetometer chain made simultaneous observations of a Pi 2 pulsation along the same meridian. Three of the four Cluster satellites were located outside the plasmasphere, while the other one was located within the plasmasphere. By combining the multipoint observations in space and the multipoint observations on the ground, we have obtained a detailed <i>L</i>-profile of the Pi 2 signatures, which has not been done in the past. In addition, we have used a method called Independent Component Analysis (ICA) to separate out other superposed waves with similar spectral components. The result shows that the wave phase of the Pi 2 was the same up to <i>L</i> &sim; 3.9 (corresponding to the plasmasphere), became earlier up to <i>L</i> &sim; 4.1 (corresponding to the plasmapause boundary layer), and showed a delaying tendency up to <i>L</i> &sim; 5.9 (corresponding to the plasmatrough). This systematic phase pattern, obtained for the first time by a combination of a ground magnetometer chain and multisatellites along a magnetic meridian with the aid of ICA, supports the interpretation that a Pi 2 signal propagated from a farther source and reached the plasmasphere.
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spelling doaj.art-ad54402186ad4e04a272882fac81ac762022-12-22T00:50:03ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762011-09-01291663167210.5194/angeo-29-1663-2011Pi 2 waves simultaneously observed by Cluster and CPMN ground-based magnetometers near the plasmapauseH. Kawano0H. Kawano1S. Ohtani2T. Uozumi3T. Tokunaga4T. Tokunaga5A. Yoshikawa6A. Yoshikawa7K. Yumoto8K. Yumoto9E. A. Lucek10M. André11the CPMN group12Department of Earth and Planetary Sciences, Kyushu University, Fukuoka, JapanSpace Environment Research Center, Kyushu University, Fukuoka, JapanJohns Hopkins University, Applied Physics Laboratory, Laurel, USASpace Environment Research Center, Kyushu University, Fukuoka, JapanDepartment of Earth and Planetary Sciences, Kyushu University, Fukuoka, Japannow at: Meiji Institute for Advanced Study of Mathematical Sciences, Kawasaki, JapanDepartment of Earth and Planetary Sciences, Kyushu University, Fukuoka, JapanSpace Environment Research Center, Kyushu University, Fukuoka, JapanDepartment of Earth and Planetary Sciences, Kyushu University, Fukuoka, JapanSpace Environment Research Center, Kyushu University, Fukuoka, JapanSpace and Atmospheric Physics Group, Blackett Laboratory, Imperial College, London, UKSwedish Institute of Space Physics, Uppsala, Sweden<a href="http://denji102.geo.kyushu-u.ac.jp/denji/obs/cpmn/cpmn_obs_e.html" target="_blank">http://denji102.geo.kyushu-u.ac.jp/denji/obs/cpmn/cpmn_obs_e.html</a>We have analyzed an event on 14 February 2003 in which Cluster satellites and the CPMN ground magnetometer chain made simultaneous observations of a Pi 2 pulsation along the same meridian. Three of the four Cluster satellites were located outside the plasmasphere, while the other one was located within the plasmasphere. By combining the multipoint observations in space and the multipoint observations on the ground, we have obtained a detailed <i>L</i>-profile of the Pi 2 signatures, which has not been done in the past. In addition, we have used a method called Independent Component Analysis (ICA) to separate out other superposed waves with similar spectral components. The result shows that the wave phase of the Pi 2 was the same up to <i>L</i> &sim; 3.9 (corresponding to the plasmasphere), became earlier up to <i>L</i> &sim; 4.1 (corresponding to the plasmapause boundary layer), and showed a delaying tendency up to <i>L</i> &sim; 5.9 (corresponding to the plasmatrough). This systematic phase pattern, obtained for the first time by a combination of a ground magnetometer chain and multisatellites along a magnetic meridian with the aid of ICA, supports the interpretation that a Pi 2 signal propagated from a farther source and reached the plasmasphere.https://www.ann-geophys.net/29/1663/2011/angeo-29-1663-2011.pdf
spellingShingle H. Kawano
H. Kawano
S. Ohtani
T. Uozumi
T. Tokunaga
T. Tokunaga
A. Yoshikawa
A. Yoshikawa
K. Yumoto
K. Yumoto
E. A. Lucek
M. André
the CPMN group
Pi 2 waves simultaneously observed by Cluster and CPMN ground-based magnetometers near the plasmapause
Annales Geophysicae
title Pi 2 waves simultaneously observed by Cluster and CPMN ground-based magnetometers near the plasmapause
title_full Pi 2 waves simultaneously observed by Cluster and CPMN ground-based magnetometers near the plasmapause
title_fullStr Pi 2 waves simultaneously observed by Cluster and CPMN ground-based magnetometers near the plasmapause
title_full_unstemmed Pi 2 waves simultaneously observed by Cluster and CPMN ground-based magnetometers near the plasmapause
title_short Pi 2 waves simultaneously observed by Cluster and CPMN ground-based magnetometers near the plasmapause
title_sort pi 2 waves simultaneously observed by cluster and cpmn ground based magnetometers near the plasmapause
url https://www.ann-geophys.net/29/1663/2011/angeo-29-1663-2011.pdf
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