Registro completo de metadatos
| Campo DC | Valor | Lengua/Idioma |
|---|---|---|
| dc.creator | Bertucci, Cesar | - |
| dc.date | 2017-07-17T17:48:47Z | - |
| dc.date | 2017-07-17T17:48:47Z | - |
| dc.date | 2009-02-28 | - |
| dc.date | 2017-07-17T13:33:46Z | - |
| dc.date.accessioned | 2019-04-29T15:48:54Z | - |
| dc.date.available | 2019-04-29T15:48:54Z | - |
| dc.date.issued | 2009-02-28 | - |
| dc.identifier | Bertucci, Cesar; Characteristics and variability of Titan's magnetic environment; The Royal Society; Philosophical Transactions of The Royal Society A; 367; 1889; 28-2-2009; 789-798 | - |
| dc.identifier | 1471-2962 | - |
| dc.identifier | http://hdl.handle.net/11336/20702 | - |
| dc.identifier | CONICET Digital | - |
| dc.identifier | CONICET | - |
| dc.identifier.uri | http://rodna.bn.gov.ar:8080/jspui/handle/bnmm/302769 | - |
| dc.description | The structure and variability of Saturn's magnetic field in the vicinity of Titan's orbit is studied. In the dawn magnetosphere, the magnetic field presents a significant radial component directed towards Saturn, suggesting that Titan is usually located below the planet's warped and dynamic magnetodisc. Also, a non-negligible component along the co-rotation direction suggests that Saturn's magnetic field lines close to the magnetodisc are being swept back from their respective magnetic meridians. In the noon sector, Titan seems to be closer to the magnetodisc central current sheet, as the field lines in this region seem to be more dipolar. The distance between the central current sheet and Titan depends mainly on the solar wind pressure. Also, δ|B|/|B|∼0.5 amplitude waveforms at periods close to Saturn's kilometric radiation period are present in the background magnetic field. This modulation in the field is ubiquitous in Saturn's magnetosphere and associated with the presence of a rotating asymmetry in the planet's magnetic field. | - |
| 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.format | application/pdf | - |
| dc.format | application/pdf | - |
| dc.language | eng | - |
| dc.publisher | The Royal Society | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/url/http://rsta.royalsocietypublishing.org/content/367/1889/789.abstract | - |
| dc.relation | info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1098/rsta.2008.0250 | - |
| 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.source.uri | http://hdl.handle.net/11336/30240 | - |
| dc.subject | Titan | - |
| dc.subject | Plasma interactions | - |
| dc.subject | Planetary magnetospheres | - |
| dc.subject | Saturn | - |
| dc.subject | Astronomía | - |
| dc.subject | Ciencias Físicas | - |
| dc.subject | CIENCIAS NATURALES Y EXACTAS | - |
| dc.title | Characteristics and 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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