Local time behaviour of low frequency geomagnetic field fluctuation power at low latitude

In this paper we present a statistical study of the local time behaviour of low frequency (0.7-4.0 mHz) geomagnetic field fluctuation power at a low latitude station (corrected geomagnetic latitude 36.2°N). The analysis was conducted for two contiguous years during the ascending phase of the solar c...

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Main Authors: M. De Lauretis, P. Francia, S. Lepidi
Format: Article
Language:English
Published: Istituto Nazionale di Geofisica e Vulcanologia (INGV) 2001-06-01
Series:Annals of Geophysics
Subjects:
Online Access:http://www.annalsofgeophysics.eu/index.php/annals/article/view/3607
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author M. De Lauretis
P. Francia
S. Lepidi
author_facet M. De Lauretis
P. Francia
S. Lepidi
author_sort M. De Lauretis
collection DOAJ
description In this paper we present a statistical study of the local time behaviour of low frequency (0.7-4.0 mHz) geomagnetic field fluctuation power at a low latitude station (corrected geomagnetic latitude 36.2°N). The analysis was conducted for two contiguous years during the ascending phase of the solar cycle. We found that the power of the horizontal east-west geomagnetic field component shows a diurnal and seasonal variation which can be related to variations of the ionospheric current system (Sq) mainly produced by dynamo-action in the ionospheric E region. The power of the horizontal north-south geomagnetic field component is higher in the local afternoon with respect to the morning; this asymmetry is more evident during time intervals characterized by high solar wind dynamic pressure.
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spelling doaj.art-eaad551479ad42578a83a34846f174ba2022-12-22T02:00:03ZengIstituto Nazionale di Geofisica e Vulcanologia (INGV)Annals of Geophysics1593-52132037-416X2001-06-0144110.4401/ag-3607Local time behaviour of low frequency geomagnetic field fluctuation power at low latitudeM. De LauretisP. FranciaS. LepidiIn this paper we present a statistical study of the local time behaviour of low frequency (0.7-4.0 mHz) geomagnetic field fluctuation power at a low latitude station (corrected geomagnetic latitude 36.2°N). The analysis was conducted for two contiguous years during the ascending phase of the solar cycle. We found that the power of the horizontal east-west geomagnetic field component shows a diurnal and seasonal variation which can be related to variations of the ionospheric current system (Sq) mainly produced by dynamo-action in the ionospheric E region. The power of the horizontal north-south geomagnetic field component is higher in the local afternoon with respect to the morning; this asymmetry is more evident during time intervals characterized by high solar wind dynamic pressure.http://www.annalsofgeophysics.eu/index.php/annals/article/view/3607Geomagnetic pulsationMHD waves and instabilities
spellingShingle M. De Lauretis
P. Francia
S. Lepidi
Local time behaviour of low frequency geomagnetic field fluctuation power at low latitude
Annals of Geophysics
Geomagnetic pulsation
MHD waves and instabilities
title Local time behaviour of low frequency geomagnetic field fluctuation power at low latitude
title_full Local time behaviour of low frequency geomagnetic field fluctuation power at low latitude
title_fullStr Local time behaviour of low frequency geomagnetic field fluctuation power at low latitude
title_full_unstemmed Local time behaviour of low frequency geomagnetic field fluctuation power at low latitude
title_short Local time behaviour of low frequency geomagnetic field fluctuation power at low latitude
title_sort local time behaviour of low frequency geomagnetic field fluctuation power at low latitude
topic Geomagnetic pulsation
MHD waves and instabilities
url http://www.annalsofgeophysics.eu/index.php/annals/article/view/3607
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AT pfrancia localtimebehaviouroflowfrequencygeomagneticfieldfluctuationpoweratlowlatitude
AT slepidi localtimebehaviouroflowfrequencygeomagneticfieldfluctuationpoweratlowlatitude