Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | Feyerabend, Moritz | - |
| dc.creator | Simon, Sven | - |
| dc.creator | Neubauer, Fritz M. | - |
| dc.creator | Motschmann, Uwe | - |
| dc.creator | Bertucci, Cesar | - |
| dc.creator | Edberg, Niklas J. T. | - |
| dc.creator | Hospodarsky, George B. | - |
| dc.creator | Kurth, William S. | - |
| dc.date | 2017-06-16T15:02:51Z | - |
| dc.date | 2017-06-16T15:02:51Z | - |
| dc.date | 2016-01 | - |
| dc.date | 2017-06-13T14:15:20Z | - |
| dc.date.accessioned | 2019-04-29T15:27:44Z | - |
| dc.date.available | 2019-04-29T15:27:44Z | - |
| dc.date.issued | 2017-06-16T15:02:51Z | - |
| dc.date.issued | 2017-06-16T15:02:51Z | - |
| dc.date.issued | 2016-01 | - |
| dc.date.issued | 2017-06-13T14:15:20Z | - |
| dc.identifier | Feyerabend, Moritz; Simon, Sven; Neubauer, Fritz M.; Motschmann, Uwe; Bertucci, Cesar; et al.; Hybrid simulation of Titan's interaction with the supersonic solar wind during Cassini's T96 flyby; American Geophysical Union; Geophysical Research Letters; 43; 1; 1-2016; 35-42 | - |
| dc.identifier | 0094-8276 | - |
| dc.identifier | http://hdl.handle.net/11336/18301 | - |
| dc.identifier | CONICET Digital | - |
| dc.identifier | CONICET | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/294585 | - |
| dc.description | By applying a hybrid (kinetic ions and fluid electrons) simulation code, we study the plasma environment of Saturn´s largest moon Titan during Cassini´s T96 flyby on 1 December 2013. The T96 encounter marks the only observed event of the entire Cassini mission where Titan was located in the supersonic solar wind in front of Saturn´s bow shock. Our simulations can quantitatively reproduce the key features of Cassini magnetic field and electron density observations during this encounter. We demonstrate that the large-scale features of Titan´s induced magnetosphere during T96 can be described in terms of a steady state interaction with a high-pressure solar wind flow. About 40 min before the encounter, Cassini observed a rotation of the incident solar wind magnetic field by almost 90°. We provide strong evidence that this rotation left a bundle of fossilized magnetic field lines in Titan´s ionosphere that was subsequently detected by the spacecraft. | - |
| dc.description | Fil: Feyerabend, Moritz. Georgia Institute Of Techology; Estados Unidos | - |
| dc.description | Fil: Simon, Sven. Georgia Institute Of Techology; Estados Unidos | - |
| dc.description | Fil: Neubauer, Fritz M.. Universitat Zu Köln; Alemania | - |
| dc.description | Fil: Motschmann, Uwe. Deutsches Zentrum Fur Luft- Und Raumfahrt; Alemania. Technische Universitat Braunschweig; Alemania | - |
| dc.description | 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: Edberg, Niklas J. T.. Instiutet For Rymdfysik; Suecia | - |
| dc.description | Fil: Hospodarsky, George B.. University Of Iowa; Estados Unidos | - |
| dc.description | Fil: Kurth, William S.. University Of Iowa; Estados Unidos | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | American Geophysical Union | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1002/2015GL066848 | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/ark/http://onlinelibrary.wiley.com/doi/10.1002/2015GL066848/abstract | - |
| dc.rights | info:eu-repo/semantics/openAccess | - |
| dc.rights | https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ | - |
| dc.source | reponame:CONICET Digital (CONICET) | - |
| dc.source | instname:Consejo Nacional de Investigaciones Científicas y Técnicas | - |
| dc.source | instacron:CONICET | - |
| dc.subject | CASSINI | - |
| dc.subject | MOON-PLASMA INTERACTION | - |
| dc.subject | T96 FLYBY | - |
| dc.subject | TITAN | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | Hybrid simulation of Titan's interaction with the supersonic solar wind during Cassini's T96 flyby | - |
| dc.type | info:eu-repo/semantics/article | - |
| dc.type | info:eu-repo/semantics/publishedVersion | - |
| dc.type | info:ar-repo/semantics/articulo | - |
| Aparece en las colecciones: | CONICET | |
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