Solar quiet geomagnetic variations and E-region neutral winds at equatorial latitudes

A model of the ionospheric current system valid at zones close to the geomagnetic equator, taking into account the contribution of neutral winds, is proposed. From this, the external magnetic field at ground is calculated. Also, ground records of the geomagnetic field variations at the Peruvian equa...

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Autores principales: de la Vega, M., Favetto, A., Osella, A.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00219169_v57_n10_p1129_delaVega
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spelling todo:paper_00219169_v57_n10_p1129_delaVega2023-10-03T14:22:41Z Solar quiet geomagnetic variations and E-region neutral winds at equatorial latitudes de la Vega, M. Favetto, A. Osella, A. A model of the ionospheric current system valid at zones close to the geomagnetic equator, taking into account the contribution of neutral winds, is proposed. From this, the external magnetic field at ground is calculated. Also, ground records of the geomagnetic field variations at the Peruvian equatorial zone were separated into their external and internal contributions. Using an iterative process a local particular fitting was found by comparing the separated external field to the one calculated with the proposed model. © 1995. Fil:de la Vega, M. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Favetto, A. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Osella, A. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_00219169_v57_n10_p1129_delaVega
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description A model of the ionospheric current system valid at zones close to the geomagnetic equator, taking into account the contribution of neutral winds, is proposed. From this, the external magnetic field at ground is calculated. Also, ground records of the geomagnetic field variations at the Peruvian equatorial zone were separated into their external and internal contributions. Using an iterative process a local particular fitting was found by comparing the separated external field to the one calculated with the proposed model. © 1995.
format JOUR
author de la Vega, M.
Favetto, A.
Osella, A.
spellingShingle de la Vega, M.
Favetto, A.
Osella, A.
Solar quiet geomagnetic variations and E-region neutral winds at equatorial latitudes
author_facet de la Vega, M.
Favetto, A.
Osella, A.
author_sort de la Vega, M.
title Solar quiet geomagnetic variations and E-region neutral winds at equatorial latitudes
title_short Solar quiet geomagnetic variations and E-region neutral winds at equatorial latitudes
title_full Solar quiet geomagnetic variations and E-region neutral winds at equatorial latitudes
title_fullStr Solar quiet geomagnetic variations and E-region neutral winds at equatorial latitudes
title_full_unstemmed Solar quiet geomagnetic variations and E-region neutral winds at equatorial latitudes
title_sort solar quiet geomagnetic variations and e-region neutral winds at equatorial latitudes
url http://hdl.handle.net/20.500.12110/paper_00219169_v57_n10_p1129_delaVega
work_keys_str_mv AT delavegam solarquietgeomagneticvariationsanderegionneutralwindsatequatoriallatitudes
AT favettoa solarquietgeomagneticvariationsanderegionneutralwindsatequatoriallatitudes
AT osellaa solarquietgeomagneticvariationsanderegionneutralwindsatequatoriallatitudes
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