Artículo

Achilleos, N.; Arridge, C.S.; Bertucci, C.; Guio, P.; Romanelli, N.; Sergis, N. "A combined model of pressure variations in Titan's plasma environment" (2014) Geophysical Research Letters. 41(24):8730-8735
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Abstract:

In order to analyze varying plasma conditions upstream of Titan, we have combined a physical model of Saturn's plasma disk with a geometrical model of the oscillating current sheet. During modeled oscillation phases where Titan is farthest from the current sheet, the main sources of plasma pressure in the near-Titan space are the magnetic pressure and, for disturbed conditions, the hot plasma pressure. When Titan is at the center of the sheet, the main sources are the dynamic pressure associated with Saturn's cold, subcorotating plasma and the hot plasma pressure under disturbed conditions. Total pressure at Titan (dynamic plus thermal plus magnetic) typically increases by a factor of up to about 3 as the current sheet center is approached. The predicted incident plasma flow direction deviates from the orbital plane of Titan by ≲10°. These results suggest a correlation between the location of magnetic pressure maxima and the oscillation phase of the plasma sheet. Our model may be used to predict near-Titan conditions from "far-field" in situ measurements. Key Points Titan's plasma environment responds to global changes in hot plasma pressureTitan is exposed to highly variable upstream plasma beta and dynamic pressureIncluding hot plasma variability improves agreement between models and data ©2014. The Authors.

Registro:

Documento: Artículo
Título:A combined model of pressure variations in Titan's plasma environment
Autor:Achilleos, N.; Arridge, C.S.; Bertucci, C.; Guio, P.; Romanelli, N.; Sergis, N.
Filiación:Department of Physics and Astronomy, University College London, London, United Kingdom
Centre for Planetary Sciences at UCL/Birkbeck, University College London, London, United Kingdom
Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science, Sagamihara, Japan
Mullard Space Science Laboratory, Dorking, United Kingdom
Department of Physics, Lancaster University, Lancaster, United Kingdom
Instituto de Astronomía y Física Del Espacio, University of Buenos Aires, Buenos Aires, Argentina
Office for Space Research and Technology, Academy of Athens, Athens, Greece
Palabras clave:magnetosphere; plasma sheet; Saturn; Titan; Magnetosphere; Planets; Plasma sheaths; Geometrical modeling; In-situ measurement; Oscillating current; Plasma environments; Plasma sheet; Pressure variations; Saturn; Titan; Magnetoplasma; correlation; in situ measurement; magnetic field; magnetosphere; plasma; pressure gradient; Saturn; Titan
Año:2014
Volumen:41
Número:24
Página de inicio:8730
Página de fin:8735
DOI: http://dx.doi.org/10.1002/2014GL061747
Título revista:Geophysical Research Letters
Título revista abreviado:Geophys. Res. Lett.
ISSN:00948276
CODEN:GPRLA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00948276_v41_n24_p8730_Achilleos

Referencias:

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Citas:

---------- APA ----------
Achilleos, N., Arridge, C.S., Bertucci, C., Guio, P., Romanelli, N. & Sergis, N. (2014) . A combined model of pressure variations in Titan's plasma environment. Geophysical Research Letters, 41(24), 8730-8735.
http://dx.doi.org/10.1002/2014GL061747
---------- CHICAGO ----------
Achilleos, N., Arridge, C.S., Bertucci, C., Guio, P., Romanelli, N., Sergis, N. "A combined model of pressure variations in Titan's plasma environment" . Geophysical Research Letters 41, no. 24 (2014) : 8730-8735.
http://dx.doi.org/10.1002/2014GL061747
---------- MLA ----------
Achilleos, N., Arridge, C.S., Bertucci, C., Guio, P., Romanelli, N., Sergis, N. "A combined model of pressure variations in Titan's plasma environment" . Geophysical Research Letters, vol. 41, no. 24, 2014, pp. 8730-8735.
http://dx.doi.org/10.1002/2014GL061747
---------- VANCOUVER ----------
Achilleos, N., Arridge, C.S., Bertucci, C., Guio, P., Romanelli, N., Sergis, N. A combined model of pressure variations in Titan's plasma environment. Geophys. Res. Lett. 2014;41(24):8730-8735.
http://dx.doi.org/10.1002/2014GL061747