Low and mid-frequency pulsations in the polar cap: polarization pattern and MLT dependence of the spectral power during the descending phase of the solar cycle
We present a statistical analysis of ULF (1-100 mHz) geomagnetic measurements conducted during years 2003-2006 at the Italian/French base of Concordia at Dome C, close to the geomagnetic pole, and at the Italian base«Mario Zucchelli» at Terra Nova Bay, also located in the polar cap, but at lower lat...
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ftopenaccessrep:oai:zenodo.org:130195 2023-10-29T02:36:27+01:00 Low and mid-frequency pulsations in the polar cap: polarization pattern and MLT dependence of the spectral power during the descending phase of the solar cycle Umberto Villante Massimo Vellante Marcello De Lauretis A. Piancatelli Patrizia Francia 2010-03-03 https://www.openaccessrepository.it/record/130195 https://doi.org/10.4401/ag-4570 und unknown url:https://www.openaccessrepository.it/communities/itmirror https://www.openaccessrepository.it/record/130195 doi:10.4401/ag-4570 info:eu-repo/semantics/openAccess Geophysics info:eu-repo/semantics/article publication-article 2010 ftopenaccessrep https://doi.org/10.4401/ag-4570 2023-10-03T22:20:41Z We present a statistical analysis of ULF (1-100 mHz) geomagnetic measurements conducted during years 2003-2006 at the Italian/French base of Concordia at Dome C, close to the geomagnetic pole, and at the Italian base«Mario Zucchelli» at Terra Nova Bay, also located in the polar cap, but at lower latitude. Our analysis shows thathigh latitude ULF pulsation power is largely controlled by the solar wind speed. At Terra Nova Bay the powershows a maximum at local noon, clearly related to cusp and closed field lines phenomena. At few mHz, the polarizationpattern indicates field line resonances driven, just equatorward with respect to the station, by wavespropagating tailward; the polarization of higher frequency pulsations, mostly originated from interplanetary upstreamwaves, suggests waves propagating sunward from the night sector. At Dome C the wave power shows asmall enhancement in the local morning, more pronounced for mid-frequency pulsations; the polarization pattern,at all frequencies, appears to indicate waves propagating sunward from the night sector, suggesting a propagationchannel to the ground via the magnetotail lobes. Article in Journal/Newspaper Geomagnetic Pole Istituto Nazionale di Fisica Nucleare (INFN): Open Access Repository Annals of Geophysics 52 1 |
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Open Polar |
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Istituto Nazionale di Fisica Nucleare (INFN): Open Access Repository |
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ftopenaccessrep |
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unknown |
topic |
Geophysics |
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Geophysics Umberto Villante Massimo Vellante Marcello De Lauretis A. Piancatelli Patrizia Francia Low and mid-frequency pulsations in the polar cap: polarization pattern and MLT dependence of the spectral power during the descending phase of the solar cycle |
topic_facet |
Geophysics |
description |
We present a statistical analysis of ULF (1-100 mHz) geomagnetic measurements conducted during years 2003-2006 at the Italian/French base of Concordia at Dome C, close to the geomagnetic pole, and at the Italian base«Mario Zucchelli» at Terra Nova Bay, also located in the polar cap, but at lower latitude. Our analysis shows thathigh latitude ULF pulsation power is largely controlled by the solar wind speed. At Terra Nova Bay the powershows a maximum at local noon, clearly related to cusp and closed field lines phenomena. At few mHz, the polarizationpattern indicates field line resonances driven, just equatorward with respect to the station, by wavespropagating tailward; the polarization of higher frequency pulsations, mostly originated from interplanetary upstreamwaves, suggests waves propagating sunward from the night sector. At Dome C the wave power shows asmall enhancement in the local morning, more pronounced for mid-frequency pulsations; the polarization pattern,at all frequencies, appears to indicate waves propagating sunward from the night sector, suggesting a propagationchannel to the ground via the magnetotail lobes. |
format |
Article in Journal/Newspaper |
author |
Umberto Villante Massimo Vellante Marcello De Lauretis A. Piancatelli Patrizia Francia |
author_facet |
Umberto Villante Massimo Vellante Marcello De Lauretis A. Piancatelli Patrizia Francia |
author_sort |
Umberto Villante |
title |
Low and mid-frequency pulsations in the polar cap: polarization pattern and MLT dependence of the spectral power during the descending phase of the solar cycle |
title_short |
Low and mid-frequency pulsations in the polar cap: polarization pattern and MLT dependence of the spectral power during the descending phase of the solar cycle |
title_full |
Low and mid-frequency pulsations in the polar cap: polarization pattern and MLT dependence of the spectral power during the descending phase of the solar cycle |
title_fullStr |
Low and mid-frequency pulsations in the polar cap: polarization pattern and MLT dependence of the spectral power during the descending phase of the solar cycle |
title_full_unstemmed |
Low and mid-frequency pulsations in the polar cap: polarization pattern and MLT dependence of the spectral power during the descending phase of the solar cycle |
title_sort |
low and mid-frequency pulsations in the polar cap: polarization pattern and mlt dependence of the spectral power during the descending phase of the solar cycle |
publishDate |
2010 |
url |
https://www.openaccessrepository.it/record/130195 https://doi.org/10.4401/ag-4570 |
genre |
Geomagnetic Pole |
genre_facet |
Geomagnetic Pole |
op_relation |
url:https://www.openaccessrepository.it/communities/itmirror https://www.openaccessrepository.it/record/130195 doi:10.4401/ag-4570 |
op_rights |
info:eu-repo/semantics/openAccess |
op_doi |
https://doi.org/10.4401/ag-4570 |
container_title |
Annals of Geophysics |
container_volume |
52 |
container_issue |
1 |
_version_ |
1781060396272058368 |