The Earth’s passage of coronal mass ejecta on October 29-31, 2003: ULF geomagnetic field fluttuations at very high latitude
We study ULF geomagnetic field fluctuations detected on October 29-31, 2003, when the Earth’s arrival of solar wind CMEs produced major geomagnetic storms; these solar wind structures are characterized by extremely high plasma speed and long-duration intervals with northward interplanetary magnetic...
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Società Astronomica Italiana
2005
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| Online Access: | http://hdl.handle.net/2122/9775 |
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ftingv:oai:www.earth-prints.org:2122/9775 |
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ftingv:oai:www.earth-prints.org:2122/9775 2023-05-15T14:01:37+02:00 The Earth’s passage of coronal mass ejecta on October 29-31, 2003: ULF geomagnetic field fluttuations at very high latitude Lepidi, S. Cafarella, L. Palangio, P. Santarelli, L. Lepidi, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Cafarella, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Palangio, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Santarelli, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia 2005-06-27 http://hdl.handle.net/2122/9775 en eng Società Astronomica Italiana Solar variability and Earth's climate http://hdl.handle.net/2122/9775 open Magnetosphere: MHD waves – Magnetosphere: polar cap 01. Atmosphere::01.03. Magnetosphere::01.03.05. Solar variability and solar wind Conference paper 2005 ftingv 2022-07-29T06:06:52Z We study ULF geomagnetic field fluctuations detected on October 29-31, 2003, when the Earth’s arrival of solar wind CMEs produced major geomagnetic storms; these solar wind structures are characterized by extremely high plasma speed and long-duration intervals with northward interplanetary magnetic field. The analyzed geomagnetic field data are from four high latitude stations (three in Antarctica), located deep in the polar cap. The analysis is extended also to low latitude European stations, in order to discriminate between local and global magnetospheric phenomena. Published Monte Porzio Catone 1A. Geomagnetismo e Paleomagnetismo open Conference Object Antarc* Antarctica Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) |
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Open Polar |
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Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) |
| op_collection_id |
ftingv |
| language |
English |
| topic |
Magnetosphere: MHD waves – Magnetosphere: polar cap 01. Atmosphere::01.03. Magnetosphere::01.03.05. Solar variability and solar wind |
| spellingShingle |
Magnetosphere: MHD waves – Magnetosphere: polar cap 01. Atmosphere::01.03. Magnetosphere::01.03.05. Solar variability and solar wind Lepidi, S. Cafarella, L. Palangio, P. Santarelli, L. The Earth’s passage of coronal mass ejecta on October 29-31, 2003: ULF geomagnetic field fluttuations at very high latitude |
| topic_facet |
Magnetosphere: MHD waves – Magnetosphere: polar cap 01. Atmosphere::01.03. Magnetosphere::01.03.05. Solar variability and solar wind |
| description |
We study ULF geomagnetic field fluctuations detected on October 29-31, 2003, when the Earth’s arrival of solar wind CMEs produced major geomagnetic storms; these solar wind structures are characterized by extremely high plasma speed and long-duration intervals with northward interplanetary magnetic field. The analyzed geomagnetic field data are from four high latitude stations (three in Antarctica), located deep in the polar cap. The analysis is extended also to low latitude European stations, in order to discriminate between local and global magnetospheric phenomena. Published Monte Porzio Catone 1A. Geomagnetismo e Paleomagnetismo open |
| author2 |
Lepidi, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Cafarella, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Palangio, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Santarelli, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia |
| format |
Conference Object |
| author |
Lepidi, S. Cafarella, L. Palangio, P. Santarelli, L. |
| author_facet |
Lepidi, S. Cafarella, L. Palangio, P. Santarelli, L. |
| author_sort |
Lepidi, S. |
| title |
The Earth’s passage of coronal mass ejecta on October 29-31, 2003: ULF geomagnetic field fluttuations at very high latitude |
| title_short |
The Earth’s passage of coronal mass ejecta on October 29-31, 2003: ULF geomagnetic field fluttuations at very high latitude |
| title_full |
The Earth’s passage of coronal mass ejecta on October 29-31, 2003: ULF geomagnetic field fluttuations at very high latitude |
| title_fullStr |
The Earth’s passage of coronal mass ejecta on October 29-31, 2003: ULF geomagnetic field fluttuations at very high latitude |
| title_full_unstemmed |
The Earth’s passage of coronal mass ejecta on October 29-31, 2003: ULF geomagnetic field fluttuations at very high latitude |
| title_sort |
earth’s passage of coronal mass ejecta on october 29-31, 2003: ulf geomagnetic field fluttuations at very high latitude |
| publisher |
Società Astronomica Italiana |
| publishDate |
2005 |
| url |
http://hdl.handle.net/2122/9775 |
| genre |
Antarc* Antarctica |
| genre_facet |
Antarc* Antarctica |
| op_relation |
Solar variability and Earth's climate http://hdl.handle.net/2122/9775 |
| op_rights |
open |
| _version_ |
1766271562187538432 |