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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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00219169_v57_n10_p1129_delaVega |
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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 |
_version_ |
1782023484865511424 |