INVESTIGADORES
BERTUCCI Cesar
congresos y reuniones científicas
Título:
Advanced Hybrid Simulation on the Magnetic Interaction at Titan
Autor/es:
SILLANPÄÄ, I.; KALLIO, E.; JARVINEN, R.; JANHUNEN, P.; VILPPOLA, J.; MURSULA, K.; BERTUCCI, C.; DOUGHERTY, M. K.; NEUBAUER, F. M.
Reunión:
Congreso; AGU Fall Meeting 2006; 2006
Resumen:
Titan, the largest moon of Saturn, has a unique plasma interaction with
the rotating plasma of Saturn's magnetosphere. Titan's dense and
nitrogen rich atmosphere is a major plasma source in the Kronian system
as it interacts with the subsonic and super-Alfvénic
magnetospheric plasma flow. Important aspects of this interaction
include ion outflow, forming of a magnetotail and draping of magnetic
field lines. Titan is a major research target for the current Cassini
mission with over 40 close flybys. To provide tools for analysis of
these new measurements we use a global hybrid simulation model to study
Titan's plasma interaction. Hybrid simulations are important at Titan in
order to reproduce the three-dimensional structures and the high
asymmetry in the behavior of ions around Titan that are results of
strong gyroradius effects. In this study we have focused on the
intriguing magnetic morphology at Titan based on our recent simulation
results. We use methods such as field line tracing to present and
analyze the magnetic connections between different parts in Titan's
interaction region. We discuss also effects that varying plasma
parameters and solar cycle dependence have on this plasma interaction.