Subir material

Suba sus trabajos a SEDICI, para mejorar notoriamente su visibilidad e impacto

 

Mostrar el registro sencillo del ítem

dc.date.accessioned 2019-10-01T17:28:50Z
dc.date.available 2019-10-01T17:28:50Z
dc.date.issued 2010
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/82425
dc.description.abstract The main purpose of this investigation is to study the ionospheric F region response induced by the intense geomagnetic storm that occurred on 7-8 September 2002. The geomagnetic index Dst reached a minimum of -181 nT at 0100 UT on 8 September. In this study, we used observations from a chain of 12 GPS stations and another chain of 6 digital ionosonde stations. It should be mentioned that, soon after the sudden commencement (SC) at 1637 UT on 7 September, the TEC variations at midlatitude stations in both hemispheres showed an F region positive storm phase. However, during the recovery phase, a strong hemispheric asymmetry was observed in the ionospheric response. While a TID type soliton was observed to propagate in the Southern American sector, no TID activity was seen in the Northern American sector. Also, in the Southern Hemisphere, the TEC variations were less affected by the geomagnetic storm. The Northern Hemisphere observations showed a strong and long-lasting negative F region storm phase starting at about 1000 UT on 8 September (lasting for about 24 h). A perusal of TEC phase fluctuations and equatorial spread-F (ESF) ionospheric sounding data indicates that, on the disturbed night of 7-8 September, some stations showed the occurrence of ESF starting at about 0000 UT (2000 LT) on 8 September, whereas other stations showed that the ESF occurrence started much later, at about 0800 UT (0500 LT). This hemispheric asymmetric response of the ionospheric F region possibly indicates the presence of different mechanisms for the generation of ESF along the various latitudinal regions during the disturbed period. en
dc.language en es
dc.subject Geomagnetic storm es
dc.subject Ionosphere es
dc.title Hemispheric asymmetries in the ionospheric response observed in the American sector during an intense geomagnetic storm en
dc.type Articulo es
sedici.identifier.other eid:2-s2.0-78650297291 es
sedici.identifier.other doi:10.1029/2010JA015661 es
sedici.identifier.other art. ID A12312 es
sedici.identifier.issn 2169-9402 es
sedici.creator.person Abreu, A. J. de es
sedici.creator.person Fagundes, P. R. es
sedici.creator.person Sahai, Y. es
sedici.creator.person Jesus, R. de es
sedici.creator.person Bittencourt, J. A. es
sedici.creator.person Brunini, Claudio Antonio es
sedici.creator.person Gende, Mauricio es
sedici.creator.person Pillat, V. G. es
sedici.creator.person Lima, W. L. C. es
sedici.creator.person Abalde, J. R. es
sedici.creator.person Pimenta, A. A. es
sedici.subject.materias Astronomía es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Journal of Geophysical Research: Space Physics es
sedici.relation.journalVolumeAndIssue vol. 115, no. 12 es


Descargar archivos

Este ítem aparece en la(s) siguiente(s) colección(ones)

Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)