Solar cycle 22 control on daily geomagnetic variation at Terra Nova Bay (Antarctica)
Nine summer geomagnetic observatory data (1986-1995) from Terra Nova Bay Base, Antarctica (Lat.74.690S, Long. 164.120E, 80.040S magnetic latitude) are used to investigate the behaviour of the daily variation of the geomagnetic field at polar latitude. The instrumentation includes a proton precession...
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Istituto Nazionale di Geofisica e Vulcanologia, INGV
1998
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ftjaog:oai:ojs.annalsofgeophysics.eu:article/3820 2023-05-15T13:54:52+02:00 Solar cycle 22 control on daily geomagnetic variation at Terra Nova Bay (Antarctica) Cafarella, L. Meloni, A. Palangio, P. 1998-11-25 application/pdf https://www.annalsofgeophysics.eu/index.php/annals/article/view/3820 https://doi.org/10.4401/ag-3820 eng eng Istituto Nazionale di Geofisica e Vulcanologia, INGV https://www.annalsofgeophysics.eu/index.php/annals/article/view/3820/3884 https://www.annalsofgeophysics.eu/index.php/annals/article/view/3820 doi:10.4401/ag-3820 Annals of Geophysics; V. 41 N. 5-6 (1998) Annals of Geophysics; Vol. 41 No. 5-6 (1998) 2037-416X 1593-5213 magnetic variations daily variation Antartica 01.03.05. Solar variability and solar wind info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion 1998 ftjaog https://doi.org/10.4401/ag-3820 2022-03-27T06:36:36Z Nine summer geomagnetic observatory data (1986-1995) from Terra Nova Bay Base, Antarctica (Lat.74.690S, Long. 164.120E, 80.040S magnetic latitude) are used to investigate the behaviour of the daily variation of the geomagnetic field at polar latitude. The instrumentation includes a proton precession magnetometer for total intensity |F| digital recordings; DI magnetometers for absolute measuring of the angular elements D and I and a three axis flux-gate system for acquiring H,D Z time variation data. We find that the magnetic time variation amplitude follows the solar cycle evolution and that the ratio between minimum solar median and maximum solar median is between 2-3 for intensive elements (H and Z) and 1.7 for declination(D). The solar cycle effect on geomagnetic daily variation elements amplitude in Antarctica, in comparison with previous studies, is then probably larger than expected. As a consequence, the electric current system that causes the daily magnetic field variation reveals a quite large solar cycle effect at Terra Nova Bay. Article in Journal/Newspaper Antarc* Antarctica antartic* Annals of Geophysics (INGV, Istituto Nazionale di Geofisica e Vulcanologia) Terra Nova Bay Annals of Geophysics 41 5-6 |
institution |
Open Polar |
collection |
Annals of Geophysics (INGV, Istituto Nazionale di Geofisica e Vulcanologia) |
op_collection_id |
ftjaog |
language |
English |
topic |
magnetic variations daily variation Antartica 01.03.05. Solar variability and solar wind |
spellingShingle |
magnetic variations daily variation Antartica 01.03.05. Solar variability and solar wind Cafarella, L. Meloni, A. Palangio, P. Solar cycle 22 control on daily geomagnetic variation at Terra Nova Bay (Antarctica) |
topic_facet |
magnetic variations daily variation Antartica 01.03.05. Solar variability and solar wind |
description |
Nine summer geomagnetic observatory data (1986-1995) from Terra Nova Bay Base, Antarctica (Lat.74.690S, Long. 164.120E, 80.040S magnetic latitude) are used to investigate the behaviour of the daily variation of the geomagnetic field at polar latitude. The instrumentation includes a proton precession magnetometer for total intensity |F| digital recordings; DI magnetometers for absolute measuring of the angular elements D and I and a three axis flux-gate system for acquiring H,D Z time variation data. We find that the magnetic time variation amplitude follows the solar cycle evolution and that the ratio between minimum solar median and maximum solar median is between 2-3 for intensive elements (H and Z) and 1.7 for declination(D). The solar cycle effect on geomagnetic daily variation elements amplitude in Antarctica, in comparison with previous studies, is then probably larger than expected. As a consequence, the electric current system that causes the daily magnetic field variation reveals a quite large solar cycle effect at Terra Nova Bay. |
format |
Article in Journal/Newspaper |
author |
Cafarella, L. Meloni, A. Palangio, P. |
author_facet |
Cafarella, L. Meloni, A. Palangio, P. |
author_sort |
Cafarella, L. |
title |
Solar cycle 22 control on daily geomagnetic variation at Terra Nova Bay (Antarctica) |
title_short |
Solar cycle 22 control on daily geomagnetic variation at Terra Nova Bay (Antarctica) |
title_full |
Solar cycle 22 control on daily geomagnetic variation at Terra Nova Bay (Antarctica) |
title_fullStr |
Solar cycle 22 control on daily geomagnetic variation at Terra Nova Bay (Antarctica) |
title_full_unstemmed |
Solar cycle 22 control on daily geomagnetic variation at Terra Nova Bay (Antarctica) |
title_sort |
solar cycle 22 control on daily geomagnetic variation at terra nova bay (antarctica) |
publisher |
Istituto Nazionale di Geofisica e Vulcanologia, INGV |
publishDate |
1998 |
url |
https://www.annalsofgeophysics.eu/index.php/annals/article/view/3820 https://doi.org/10.4401/ag-3820 |
geographic |
Terra Nova Bay |
geographic_facet |
Terra Nova Bay |
genre |
Antarc* Antarctica antartic* |
genre_facet |
Antarc* Antarctica antartic* |
op_source |
Annals of Geophysics; V. 41 N. 5-6 (1998) Annals of Geophysics; Vol. 41 No. 5-6 (1998) 2037-416X 1593-5213 |
op_relation |
https://www.annalsofgeophysics.eu/index.php/annals/article/view/3820/3884 https://www.annalsofgeophysics.eu/index.php/annals/article/view/3820 doi:10.4401/ag-3820 |
op_doi |
https://doi.org/10.4401/ag-3820 |
container_title |
Annals of Geophysics |
container_volume |
41 |
container_issue |
5-6 |
_version_ |
1766261010409193472 |