High resolution geomagnetic field observations at Terra Nova bay, Antarctica

he preliminary results obtained from the analysis in the micropulsation frequency range of high time resolution magnetic field data recorded at the Antarctic Italian geomagnetic observatory at Terra Nova Bay for 11 consecutive days in February 1994 are reported. The spectral index over the whole Pcl...

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Published in:Annals of Geophysics
Main Authors: Lepidi, S., Villante, U., Vellante, M., Palangio, P., Meloni, A.
Format: Article in Journal/Newspaper
Language:English
Published: Istituto Nazionale di Geofisica e Vulcanologia, INGV 1996
Subjects:
Online Access:https://www.annalsofgeophysics.eu/index.php/annals/article/view/3987
https://doi.org/10.4401/ag-3987
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spelling ftjaog:oai:ojs.annalsofgeophysics.eu:article/3987 2023-05-15T13:54:52+02:00 High resolution geomagnetic field observations at Terra Nova bay, Antarctica Lepidi, S. Villante, U. Vellante, M. Palangio, P. Meloni, A. 1996-11-25 application/pdf https://www.annalsofgeophysics.eu/index.php/annals/article/view/3987 https://doi.org/10.4401/ag-3987 eng eng Istituto Nazionale di Geofisica e Vulcanologia, INGV https://www.annalsofgeophysics.eu/index.php/annals/article/view/3987/4052 https://www.annalsofgeophysics.eu/index.php/annals/article/view/3987 doi:10.4401/ag-3987 Annals of Geophysics; V. 39 N. 3 (1996) Annals of Geophysics; Vol. 39 No. 3 (1996) 2037-416X 1593-5213 Geomagnetic pulsations spectral index wave polarization Antartica 04.05.05. Main geomagnetic field info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 1996 ftjaog https://doi.org/10.4401/ag-3987 2022-03-27T06:36:47Z he preliminary results obtained from the analysis in the micropulsation frequency range of high time resolution magnetic field data recorded at the Antarctic Italian geomagnetic observatory at Terra Nova Bay for 11 consecutive days in February 1994 are reported. The spectral index over the whole Pcl-Pc5 frequency range is of the order of 3.5 and its value significantly increases beyond about 50 mHz. Spectral peaks in the Pc3 frequency range are common, especially during the daytime hours, and are probably due to the direct penetration of upstream waves in the cusp region. From the local time distribution of the micro pulsation power, a signifi - cant activity enhancement around the local magnetic noon emerges, in agreement with previous observations. The analysis of the signal polarisation characteristics in the horizontal plane shows a predominant CW polarisation in the Pcl-Pc3 frequency ranges with the major axis of the polarisation ellipse in the first quadrant. Article in Journal/Newspaper Antarc* Antarctic Antarctica antartic* Annals of Geophysics (INGV, Istituto Nazionale di Geofisica e Vulcanologia) Antarctic Terra Nova Bay The Antarctic Annals of Geophysics 39 3
institution Open Polar
collection Annals of Geophysics (INGV, Istituto Nazionale di Geofisica e Vulcanologia)
op_collection_id ftjaog
language English
topic Geomagnetic pulsations
spectral index
wave polarization
Antartica
04.05.05. Main geomagnetic field
spellingShingle Geomagnetic pulsations
spectral index
wave polarization
Antartica
04.05.05. Main geomagnetic field
Lepidi, S.
Villante, U.
Vellante, M.
Palangio, P.
Meloni, A.
High resolution geomagnetic field observations at Terra Nova bay, Antarctica
topic_facet Geomagnetic pulsations
spectral index
wave polarization
Antartica
04.05.05. Main geomagnetic field
description he preliminary results obtained from the analysis in the micropulsation frequency range of high time resolution magnetic field data recorded at the Antarctic Italian geomagnetic observatory at Terra Nova Bay for 11 consecutive days in February 1994 are reported. The spectral index over the whole Pcl-Pc5 frequency range is of the order of 3.5 and its value significantly increases beyond about 50 mHz. Spectral peaks in the Pc3 frequency range are common, especially during the daytime hours, and are probably due to the direct penetration of upstream waves in the cusp region. From the local time distribution of the micro pulsation power, a signifi - cant activity enhancement around the local magnetic noon emerges, in agreement with previous observations. The analysis of the signal polarisation characteristics in the horizontal plane shows a predominant CW polarisation in the Pcl-Pc3 frequency ranges with the major axis of the polarisation ellipse in the first quadrant.
format Article in Journal/Newspaper
author Lepidi, S.
Villante, U.
Vellante, M.
Palangio, P.
Meloni, A.
author_facet Lepidi, S.
Villante, U.
Vellante, M.
Palangio, P.
Meloni, A.
author_sort Lepidi, S.
title High resolution geomagnetic field observations at Terra Nova bay, Antarctica
title_short High resolution geomagnetic field observations at Terra Nova bay, Antarctica
title_full High resolution geomagnetic field observations at Terra Nova bay, Antarctica
title_fullStr High resolution geomagnetic field observations at Terra Nova bay, Antarctica
title_full_unstemmed High resolution geomagnetic field observations at Terra Nova bay, Antarctica
title_sort high resolution geomagnetic field observations at terra nova bay, antarctica
publisher Istituto Nazionale di Geofisica e Vulcanologia, INGV
publishDate 1996
url https://www.annalsofgeophysics.eu/index.php/annals/article/view/3987
https://doi.org/10.4401/ag-3987
geographic Antarctic
Terra Nova Bay
The Antarctic
geographic_facet Antarctic
Terra Nova Bay
The Antarctic
genre Antarc*
Antarctic
Antarctica
antartic*
genre_facet Antarc*
Antarctic
Antarctica
antartic*
op_source Annals of Geophysics; V. 39 N. 3 (1996)
Annals of Geophysics; Vol. 39 No. 3 (1996)
2037-416X
1593-5213
op_relation https://www.annalsofgeophysics.eu/index.php/annals/article/view/3987/4052
https://www.annalsofgeophysics.eu/index.php/annals/article/view/3987
doi:10.4401/ag-3987
op_doi https://doi.org/10.4401/ag-3987
container_title Annals of Geophysics
container_volume 39
container_issue 3
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