author_facet Canu, P.
Décréau, P. M. E.
Trotignon, J. G.
Rauch, J. L.
Seran, H. C.
Fergeau, P.
Lévêque, M.
Martin, Ph.
Sené, F. X.
Le Guirriec, E.
Alleyne, H.
Yearby, K.
Canu, P.
Décréau, P. M. E.
Trotignon, J. G.
Rauch, J. L.
Seran, H. C.
Fergeau, P.
Lévêque, M.
Martin, Ph.
Sené, F. X.
Le Guirriec, E.
Alleyne, H.
Yearby, K.
author Canu, P.
Décréau, P. M. E.
Trotignon, J. G.
Rauch, J. L.
Seran, H. C.
Fergeau, P.
Lévêque, M.
Martin, Ph.
Sené, F. X.
Le Guirriec, E.
Alleyne, H.
Yearby, K.
spellingShingle Canu, P.
Décréau, P. M. E.
Trotignon, J. G.
Rauch, J. L.
Seran, H. C.
Fergeau, P.
Lévêque, M.
Martin, Ph.
Sené, F. X.
Le Guirriec, E.
Alleyne, H.
Yearby, K.
Annales Geophysicae
Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
Space and Planetary Science
Earth and Planetary Sciences (miscellaneous)
Atmospheric Science
Geology
Astronomy and Astrophysics
author_sort canu, p.
spelling Canu, P. Décréau, P. M. E. Trotignon, J. G. Rauch, J. L. Seran, H. C. Fergeau, P. Lévêque, M. Martin, Ph. Sené, F. X. Le Guirriec, E. Alleyne, H. Yearby, K. 1432-0576 Copernicus GmbH Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Geology Astronomy and Astrophysics http://dx.doi.org/10.5194/angeo-19-1697-2001 <jats:p>Abstract. We use the data collected by the Whisper instrument onboard the Cluster spacecraft for a first test of its capabilities in the identification of the natural plasma waves observed in the Earth’s magnetosphere. The main signatures observed at the plasma frequency, upper hybrid frequency, and electron Bernstein modes were often difficult to be reliably recognized on previous missions. We use here the characteristic frequencies provided by the resonances triggered by the relaxation sounder of Whisper to identify with good confidence the various signatures detected in the complex wave spectra collected close to the plasmapause. Coupled with the good sensitivity, frequency and time resolution of Whisper, the resonances detected by the sounder allow one to precisely spot these natural emissions. This first analysis seems to confirm the interpretation of Geos observations: the natural emissions observed in Bernstein modes above the plasma frequency, now widely observed onboard Cluster, are not modeled by a single Maxwellian electrons distribution function. Therefore, multi-temperature electron distribution functions should be considered.Key words. Space plasma physics (active perturbation experiments; waves and instabilities; instrument and techniques) </jats:p> Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder Annales Geophysicae
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series Annales Geophysicae
source_id 49
title Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
title_unstemmed Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
title_full Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
title_fullStr Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
title_full_unstemmed Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
title_short Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
title_sort identification of natural plasma emissions observed close to the plasmapause by the cluster-whisper relaxation sounder
topic Space and Planetary Science
Earth and Planetary Sciences (miscellaneous)
Atmospheric Science
Geology
Astronomy and Astrophysics
url http://dx.doi.org/10.5194/angeo-19-1697-2001
publishDate 2001
physical 1697-1709
description <jats:p>Abstract. We use the data collected by the Whisper instrument onboard the Cluster spacecraft for a first test of its capabilities in the identification of the natural plasma waves observed in the Earth’s magnetosphere. The main signatures observed at the plasma frequency, upper hybrid frequency, and electron Bernstein modes were often difficult to be reliably recognized on previous missions. We use here the characteristic frequencies provided by the resonances triggered by the relaxation sounder of Whisper to identify with good confidence the various signatures detected in the complex wave spectra collected close to the plasmapause. Coupled with the good sensitivity, frequency and time resolution of Whisper, the resonances detected by the sounder allow one to precisely spot these natural emissions. This first analysis seems to confirm the interpretation of Geos observations: the natural emissions observed in Bernstein modes above the plasma frequency, now widely observed onboard Cluster, are not modeled by a single Maxwellian electrons distribution function. Therefore, multi-temperature electron distribution functions should be considered.Key words. Space plasma physics (active perturbation experiments; waves and instabilities; instrument and techniques) </jats:p>
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author Canu, P., Décréau, P. M. E., Trotignon, J. G., Rauch, J. L., Seran, H. C., Fergeau, P., Lévêque, M., Martin, Ph., Sené, F. X., Le Guirriec, E., Alleyne, H., Yearby, K.
author_facet Canu, P., Décréau, P. M. E., Trotignon, J. G., Rauch, J. L., Seran, H. C., Fergeau, P., Lévêque, M., Martin, Ph., Sené, F. X., Le Guirriec, E., Alleyne, H., Yearby, K., Canu, P., Décréau, P. M. E., Trotignon, J. G., Rauch, J. L., Seran, H. C., Fergeau, P., Lévêque, M., Martin, Ph., Sené, F. X., Le Guirriec, E., Alleyne, H., Yearby, K.
author_sort canu, p.
container_issue 10/12
container_start_page 1697
container_title Annales Geophysicae
container_volume 19
description <jats:p>Abstract. We use the data collected by the Whisper instrument onboard the Cluster spacecraft for a first test of its capabilities in the identification of the natural plasma waves observed in the Earth’s magnetosphere. The main signatures observed at the plasma frequency, upper hybrid frequency, and electron Bernstein modes were often difficult to be reliably recognized on previous missions. We use here the characteristic frequencies provided by the resonances triggered by the relaxation sounder of Whisper to identify with good confidence the various signatures detected in the complex wave spectra collected close to the plasmapause. Coupled with the good sensitivity, frequency and time resolution of Whisper, the resonances detected by the sounder allow one to precisely spot these natural emissions. This first analysis seems to confirm the interpretation of Geos observations: the natural emissions observed in Bernstein modes above the plasma frequency, now widely observed onboard Cluster, are not modeled by a single Maxwellian electrons distribution function. Therefore, multi-temperature electron distribution functions should be considered.Key words. Space plasma physics (active perturbation experiments; waves and instabilities; instrument and techniques) </jats:p>
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spelling Canu, P. Décréau, P. M. E. Trotignon, J. G. Rauch, J. L. Seran, H. C. Fergeau, P. Lévêque, M. Martin, Ph. Sené, F. X. Le Guirriec, E. Alleyne, H. Yearby, K. 1432-0576 Copernicus GmbH Space and Planetary Science Earth and Planetary Sciences (miscellaneous) Atmospheric Science Geology Astronomy and Astrophysics http://dx.doi.org/10.5194/angeo-19-1697-2001 <jats:p>Abstract. We use the data collected by the Whisper instrument onboard the Cluster spacecraft for a first test of its capabilities in the identification of the natural plasma waves observed in the Earth’s magnetosphere. The main signatures observed at the plasma frequency, upper hybrid frequency, and electron Bernstein modes were often difficult to be reliably recognized on previous missions. We use here the characteristic frequencies provided by the resonances triggered by the relaxation sounder of Whisper to identify with good confidence the various signatures detected in the complex wave spectra collected close to the plasmapause. Coupled with the good sensitivity, frequency and time resolution of Whisper, the resonances detected by the sounder allow one to precisely spot these natural emissions. This first analysis seems to confirm the interpretation of Geos observations: the natural emissions observed in Bernstein modes above the plasma frequency, now widely observed onboard Cluster, are not modeled by a single Maxwellian electrons distribution function. Therefore, multi-temperature electron distribution functions should be considered.Key words. Space plasma physics (active perturbation experiments; waves and instabilities; instrument and techniques) </jats:p> Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder Annales Geophysicae
spellingShingle Canu, P., Décréau, P. M. E., Trotignon, J. G., Rauch, J. L., Seran, H. C., Fergeau, P., Lévêque, M., Martin, Ph., Sené, F. X., Le Guirriec, E., Alleyne, H., Yearby, K., Annales Geophysicae, Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder, Space and Planetary Science, Earth and Planetary Sciences (miscellaneous), Atmospheric Science, Geology, Astronomy and Astrophysics
title Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
title_full Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
title_fullStr Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
title_full_unstemmed Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
title_short Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
title_sort identification of natural plasma emissions observed close to the plasmapause by the cluster-whisper relaxation sounder
title_unstemmed Identification of natural plasma emissions observed close to the plasmapause by the Cluster-Whisper relaxation sounder
topic Space and Planetary Science, Earth and Planetary Sciences (miscellaneous), Atmospheric Science, Geology, Astronomy and Astrophysics
url http://dx.doi.org/10.5194/angeo-19-1697-2001