Dynamics of geomagnetic field secular variations at the Antarctic continent

The changes of the geomagnetic field secular variations at the Antarctic magnetic observatories for 1956—2010 years were investigated. Comparison between the secular variations at the Antarctica continent and at the north polar cap and adjacent observatories in the middle latitudes of south hemisphe...

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Date:2016
Main Authors: Sumaruk, Yu. P., Sumaruk, T. P.
Format: Article
Language:Ukrainian
Published: S. Subbotin Institute of Geophysics of the NAS of Ukraine 2016
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Online Access:https://journals.uran.ua/geofizicheskiy/article/view/107771
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Journal Title:Geofizicheskiy Zhurnal

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Geofizicheskiy Zhurnal
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author Sumaruk, Yu. P.
Sumaruk, T. P.
author_facet Sumaruk, Yu. P.
Sumaruk, T. P.
author_sort Sumaruk, Yu. P.
baseUrl_str
collection OJS
datestamp_date 2020-10-07T11:34:21Z
description The changes of the geomagnetic field secular variations at the Antarctic magnetic observatories for 1956—2010 years were investigated. Comparison between the secular variations at the Antarctica continent and at the north polar cap and adjacent observatories in the middle latitudes of south hemisphere was performed.   The conclusion was drawn that secular variations at the high latitudes of the Earth have three sources: changes of the position of the central magnetic dipole and also changes of the value of its magnetic momentum, changes of sources in tectonosphere and changes of geomadnetic activity. depending on the sign of general magnetic field of the Sun, and, correspondingly, on the sign of the vertical component of the interplanetary magnetic field.
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spelling journalsuranua-geofizicheskiy-article-1077712020-10-07T11:34:21Z Dynamics of geomagnetic field secular variations at the Antarctic continent Sumaruk, Yu. P. Sumaruk, T. P. secular variations magnetic anomalies geomagnetic activity general magnetic field of the Sun The changes of the geomagnetic field secular variations at the Antarctic magnetic observatories for 1956—2010 years were investigated. Comparison between the secular variations at the Antarctica continent and at the north polar cap and adjacent observatories in the middle latitudes of south hemisphere was performed.   The conclusion was drawn that secular variations at the high latitudes of the Earth have three sources: changes of the position of the central magnetic dipole and also changes of the value of its magnetic momentum, changes of sources in tectonosphere and changes of geomadnetic activity. depending on the sign of general magnetic field of the Sun, and, correspondingly, on the sign of the vertical component of the interplanetary magnetic field. S. Subbotin Institute of Geophysics of the NAS of Ukraine 2016-07-01 Article Article application/pdf https://journals.uran.ua/geofizicheskiy/article/view/107771 10.24028/gzh.0203-3100.v38i2.2016.107771 Geofizicheskiy Zhurnal; Vol. 38 No. 2 (2016); 120-138 Геофизический журнал; Том 38 № 2 (2016); 120-138 Геофізичний журнал; Том 38 № 2 (2016); 120-138 2524-1052 0203-3100 uk https://journals.uran.ua/geofizicheskiy/article/view/107771/102725 Copyright (c) 2020 Geofizicheskiy Zhurnal https://creativecommons.org/licenses/by/4.0
spellingShingle secular variations
magnetic anomalies
geomagnetic activity
general magnetic field of the Sun
Sumaruk, Yu. P.
Sumaruk, T. P.
Dynamics of geomagnetic field secular variations at the Antarctic continent
title Dynamics of geomagnetic field secular variations at the Antarctic continent
title_full Dynamics of geomagnetic field secular variations at the Antarctic continent
title_fullStr Dynamics of geomagnetic field secular variations at the Antarctic continent
title_full_unstemmed Dynamics of geomagnetic field secular variations at the Antarctic continent
title_short Dynamics of geomagnetic field secular variations at the Antarctic continent
title_sort dynamics of geomagnetic field secular variations at the antarctic continent
topic secular variations
magnetic anomalies
geomagnetic activity
general magnetic field of the Sun
topic_facet secular variations
magnetic anomalies
geomagnetic activity
general magnetic field of the Sun
url https://journals.uran.ua/geofizicheskiy/article/view/107771
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