Mostrar el registro sencillo del ítem
dc.contributor.author
Zossi, Bruno Santiago
![Se ha confirmado la validez de este valor de autoridad por un usuario](/themes/CONICETDigital/images/authority_control/invisible.gif)
dc.contributor.author
Fagre, Mariano
![Se ha confirmado la validez de este valor de autoridad por un usuario](/themes/CONICETDigital/images/authority_control/invisible.gif)
dc.contributor.author
Elias, Ana Georgina
![Se ha confirmado la validez de este valor de autoridad por un usuario](/themes/CONICETDigital/images/authority_control/invisible.gif)
dc.date.available
2019-08-12T17:16:51Z
dc.date.issued
2018-12
dc.identifier.citation
Zossi, Bruno Santiago; Fagre, Mariano; Elias, Ana Georgina; On ionic contributions to Pedersen conductance; Blackwell Publishing Ltd; Journal of Geophysical Research: Space Physics; 123; 12; 12-2018; 10310-10318
dc.identifier.issn
2169-9380
dc.identifier.uri
http://hdl.handle.net/11336/81447
dc.description.abstract
Ionospheric conductivity is a key parameter to understand the upper atmosphere electrodynamics, magnetosphere-ionosphere-thermosphere coupling and several geophysical processes. In the case of Pedersen conductivity, ions and electrons are moving in opposite direction, so that it results from the addition of the separate contributions. In this work, the role of the three main ions, that is, NO+, O2 +, and O+, in the conductivity height profile and in the conductance global pattern is analyzed for different solar activity levels and seasons. NO+ is the is the main contributor for the maximum conductivity in all the cases in the E layer; however, O+ takes relevance with a significant percentage of the conductance at certain regions such as the South Atlantic Anomaly and the crests at the equatorial ionization anomaly, becoming the main conducting ion in these zones when the solar activity is high. Regarding seasonal effects, the role of NO+ in the conductivity is maximum on summer hemisphere, while O+ becomes important in winter and maximum with high solar activity. O2 + has maximum percentage close to magnetic poles, where the magnetic field strength is intense lowering the peak conducting level.
dc.format
application/pdf
dc.language.iso
eng
dc.publisher
Blackwell Publishing Ltd
dc.rights
info:eu-repo/semantics/openAccess
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject
Height Profile Conductivity
dc.subject
Ionic Contribution to Conductance
dc.subject
Ionosphere Conductance
dc.subject
Spatial Structure of Conductance
dc.subject.classification
Geociencias multidisciplinaria
![Se ha confirmado la validez de este valor de autoridad por un usuario](/themes/CONICETDigital/images/authority_control/invisible.gif)
dc.subject.classification
Ciencias de la Tierra y relacionadas con el Medio Ambiente
![Se ha confirmado la validez de este valor de autoridad por un usuario](/themes/CONICETDigital/images/authority_control/invisible.gif)
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS
![Se ha confirmado la validez de este valor de autoridad por un usuario](/themes/CONICETDigital/images/authority_control/invisible.gif)
dc.title
On ionic contributions to Pedersen conductance
dc.type
info:eu-repo/semantics/article
dc.type
info:ar-repo/semantics/artículo
dc.type
info:eu-repo/semantics/publishedVersion
dc.date.updated
2019-08-07T14:13:38Z
dc.journal.volume
123
dc.journal.number
12
dc.journal.pagination
10310-10318
dc.journal.pais
Estados Unidos
![Se ha confirmado la validez de este valor de autoridad por un usuario](/themes/CONICETDigital/images/authority_control/invisible.gif)
dc.journal.ciudad
New York
dc.description.fil
Fil: Zossi, Bruno Santiago. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina. Universidad Nacional de Tucumán; Argentina
dc.description.fil
Fil: Fagre, Mariano. Universidad Nacional de Tucumán; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina
dc.description.fil
Fil: Elias, Ana Georgina. Universidad Nacional de Tucumán; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Tucumán; Argentina
dc.journal.title
Journal of Geophysical Research: Space Physics
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2018JA026011
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1029/ 2018JA026011
Archivos asociados