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dc.contributor.author Simon, S.
dc.contributor.author Motschmann, U.
dc.contributor.author Kleindienst, G.
dc.contributor.author Glassmeier, K. H.
dc.contributor.author Bertucci, Cesar
dc.contributor.author Dougherty, M. K.
dc.date.available 2017-07-17T15:54:54Z
dc.date.issued 2008-12
dc.identifier.citation Simon, S.; Motschmann, U.; Kleindienst, G.; Glassmeier, K. H.; Bertucci, Cesar; et al.; Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data; American Geophysical Union; Geophysical Research Letters; 35; 4; 12-2008; 1-4
dc.identifier.issn 0094-8276
dc.identifier.uri http://hdl.handle.net/11336/20680
dc.description.abstract During the T34 flyby on 19 July 2007, the Cassini spacecraft passed through the magnetic pile-up region at Titan's ramside. The magnetic environment of Titan during this flyby is studied using a three-dimensional hybrid simulation model. This approach treats the electrons of the plasma as a massless, charge-neutralizing fluid, whereas the effects of finite ion gyroradii are taken into account by modeling the ions as individual particles. The simulation results are compared to data collected by the Cassini Magnetometer Instrument. The key features of the measured magnetic field signature have shown to be fully reproducible in the framework of the simulation model. Several signatures in the observed magnetic field can be ascribed to the passage of the Cassini spacecraft through the magnetic barrier upstream of Titan.
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's magnetic field
dc.subject.classification Astronomía
dc.subject.classification Ciencias Físicas
dc.subject.classification CIENCIAS NATURALES Y EXACTAS
dc.title Titan's magnetic field signature during the Cassini T34 flyby: Comparison between hybrid simulations and MAG data
dc.type info:eu-repo/semantics/article
dc.type info:ar-repo/semantics/artículo
dc.type info:eu-repo/semantics/publishedVersion
dc.date.updated 2017-07-17T13:33:20Z
dc.journal.volume 35
dc.journal.number 4
dc.journal.pagination 1-4
dc.journal.pais Estados Unidos
dc.journal.ciudad Nueva York
dc.description.fil Fil: Simon, S.. Technische Universitat Braunschweig; Alemania
dc.description.fil Fil: Motschmann, U.. Technische Universitat Braunschweig; Alemania
dc.description.fil Fil: Kleindienst, G.. Technische Universitat Braunschweig; Alemania
dc.description.fil Fil: Glassmeier, K. H.. Technische Universitat Braunschweig; Alemania
dc.description.fil 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/10.1029/2007GL033056
dc.relation.alternativeid info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1029/2007GL033056/abstract


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    Articulos de INST.DE ASTRONOMIA Y FISICA DEL ESPACIO(I)

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info:eu-repo/semantics/openAccess Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción: Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Unported (CC BY-NC-SA 2.5)