INVESTIGADORES
BERTUCCI Cesar
congresos y reuniones científicas
Título:
Titan in Saturn's Magnetosheath: Cassini MAG Observations During the T32 Encounter
Autor/es:
BERTUCCI, C.; SZEGO, K.; WAHLUND, J.; COATES, A. J.; NEUBAUER, F. M.; ACHILLEOS, N.; ARRIDGE, C. S.; DOUGHERTY, M. K.; MODOLO, R.
Reunión:
Congreso; AGU Fall Meeting 2007; 2007
Resumen:
With a magnetopause average stand-off distance of at least 21 Kronian
radii, Titan spends most of its time in Saturn's rotating magnetosphere.
However, for Saturn local times near noon and during periods of high
solar wind pressure, Titan is expected to be found within the
magnetosheath. An analysis of Cassini magnetometer data obtained during
the T32 flyby suggests that Titan was found in Saturn magnetosheath at
the time of the encounter, in the middle of a series of strong
magnetopause compressions and expansions. However, the topology of the
heavily massloaded, draped field lines observed in Titan's magnetic
pileup region suggest that a few minutes before the encounter, the
satellite was within the magnetosphere. This interpretation is supported
by Cassini plasma data. This is the first time that Saturn's major
satellite is found in the shocked solar wind.