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dc.contributor.author
Edberg, N. J. T.  
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Andrews, D. J.  
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Shebanits, O.  
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Agren, K.  
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Wahlund, J. E.  
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Opgenoorth, H. J.  
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Roussos, E.  
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Garnier, P.  
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Cravens, T. E.  
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Badman, S. V.  
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Modolo, R.  
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Bertucci, Cesar  
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Dougherty, M. K.  
dc.date.available
2017-05-29T19:18:38Z  
dc.date.issued
2013-06  
dc.identifier.citation
Edberg, N. J. T.; Andrews, D. J.; Shebanits, O.; Agren, K.; Wahlund, J. E.; et al.; Extreme densities in Titan's ionosphere during the T85 magnetosheath encounter; American Geophysical Union; Geophysical Research Letters; 40; 12; 6-2013; 2879-2883  
dc.identifier.issn
0094-8276  
dc.identifier.uri
http://hdl.handle.net/11336/17089  
dc.description.abstract
We present Cassini Langmuir probe measurements of the highest electron number densities ever reported from the ionosphere of Titan. The measured density reached 4310 cm−3 during the T85 Titan flyby. This is at least 500 cm−3 higher than ever observed before and at least 50% above the average density for similar solar zenith angles. The peak of the ionospheric density is not reached on this flyby, making the maximum measured density a lower limit. During this flyby, we also report that an impacting coronal mass ejection (CME) leaves Titan in the magnetosheath of Saturn, where it is exposed to shocked solar wind plasma for at least 2 h 45 min. We suggest that the solar wind plasma in the magnetosheath during the CME conditions significantly modifies Titan's ionosphere by an addition of particle impact ionization by precipitating protons.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
American Geophysical Union  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Titan  
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Cassini  
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Ionosphere  
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Magnetosheath  
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Astronomía  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
Extreme densities in Titan's ionosphere during the T85 magnetosheath encounter  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2017-05-23T19:16:50Z  
dc.journal.volume
40  
dc.journal.number
12  
dc.journal.pagination
2879-2883  
dc.journal.pais
Estados Unidos  
dc.description.fil
Fil: Edberg, N. J. T.. Swedish Institute of Space Physics; Suecia  
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Fil: Andrews, D. J.. Swedish Institute of Space Physics; Suecia  
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Fil: Shebanits, O.. Swedish Institute of Space Physics; Suecia  
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Fil: Agren, K.. Swedish Institute of Space Physics; Suecia  
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Fil: Wahlund, J. E.. Swedish Institute of Space Physics; Suecia  
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Fil: Opgenoorth, H. J.. Swedish Institute of Space Physics; Suecia  
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Fil: Roussos, E.. Max Planck Institute for Solar System Research; Alemania  
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Fil: Garnier, P.. University of Toulouse; Francia  
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Fil: Cravens, T. E.. University of Kansas; Estados Unidos  
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Fil: Badman, S. V.. University of Leicester; Reino Unido  
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Fil: Modolo, R.. UVSQ/LATMOS-IPSL/CNRS-INSU; Francia  
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Fil: Bertucci, Cesar. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina  
dc.description.fil
Fil: Dougherty, M. K.. Imperial College London; Reino Unido  
dc.journal.title
Geophysical Research Letters  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1002/grl.50579  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1002/grl.50579/full