Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | Bertucci, Cesar | - |
| dc.creator | Sinclair, B. | - |
| dc.creator | Achilleos, N. | - |
| dc.creator | Hunt, P. | - |
| dc.creator | Dougherty, M. K. | - |
| dc.creator | Arridge, C. S. | - |
| dc.date | 2017-07-17T16:20:33Z | - |
| dc.date | 2017-07-17T16:20:33Z | - |
| dc.date | 2009-12 | - |
| dc.date | 2017-07-17T13:33:45Z | - |
| dc.date.accessioned | 2019-04-29T15:55:15Z | - |
| dc.date.available | 2019-04-29T15:55:15Z | - |
| dc.identifier | Bertucci, Cesar; Sinclair, B.; Achilleos, N.; Hunt, P.; Dougherty, M. K.; et al.; The variability of Titan's magnetic environment; Elsevier; Planetary and Space Science; 57; 14-15; 12-2009; 1813-1820 | - |
| dc.identifier | 0032-0633 | - |
| dc.identifier | http://hdl.handle.net/11336/20687 | - |
| dc.identifier | CONICET Digital | - |
| dc.identifier | CONICET | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/305357 | - |
| dc.description | With a mean orbital radius of 20.2 Saturnian radii (1 Saturn radius RS=60,330 km), Titan is usually located within the kronian magnetosphere. 3.5 years of Cassini magnetometer observations in the vicinity of Titan´s orbit reveal that the moon´s magnetic environment is strongly affected by the presence of Saturn´s magnetodisk. As a result of the disk´s solar-wind-induced asymmetry, Titan is exposed to quasi-dipolar fields in the noon sector, and planetward, swept-back fields in the dawn, dusk and midnight sectors. These magnetic properties indicate that the moon is, on average, south of the central current sheet and immersed in Saturn´s rotating magnetospheric plasma for all local times (SLT). At a given SLT, Titan´s distance from the central current sheet associated with the magnetodisk depends on the solar wind pressure and on the phase of the Saturn´s kilometric radiation (SKR). The influence of the solar wind is present at all SLT (although dominant in the noon sector), whereas the SKR modulation seems to affect the magnetic field to first-order at least in the dawn sector. Near dawn local times, Titan tends to be farther from the disk at SKR longitudes around ˜140° and closer to it for longitudes around ˜320°. Depending on these factors, Titan is exposed to either: (i) a ‘magnetodisk lobe’ regime where the plasma beta is low and fields are radially ‘stretched’ and usually stronger or (ii) a ‘current sheet’ regime—characterized by quasi-dipolar, relatively weak fields and a high-beta plasma. | - |
| 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. Imperial College London; Reino Unido | - |
| dc.description | Fil: Sinclair, B.. Imperial College London; Reino Unido | - |
| dc.description | Fil: Achilleos, N.. University College London; Estados Unidos | - |
| dc.description | Fil: Hunt, P.. Imperial College London; Reino Unido | - |
| dc.description | Fil: Dougherty, M. K.. Imperial College London; Reino Unido | - |
| dc.description | Fil: Arridge, C. S.. University College London; Estados Unidos | - |
| dc.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | Elsevier | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1016/j.pss.2009.02.009 | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0032063309000543 | - |
| dc.rights | info:eu-repo/semantics/restrictedAccess | - |
| 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 | Planetary magnetospheres | - |
| dc.subject | Magnetodisk | - |
| dc.subject | Titan | - |
| dc.subject | Plasma interactions with unmagnetized bodies | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | The variability of Titan's magnetic environment | - |
| 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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