INVESTIGADORES
BERTUCCI Cesar
congresos y reuniones científicas
Título:
Dynamical and Magnetic Field Time Constants for Titan's Ionosphere - Empirical Estimates
Autor/es:
CRAVENS, T. E.; RICHARD, M. S.; MA, Y.; BERTUCCI, C.; LUHMANN, J. G.; LEDVINA, S. A.; ROBERTSON, I. P.; WAHLUND, J.; AGREN, K.; CUI, J.; MUELLER-WODARG, I. C.; WAITE, J. H.; DOUGHERTY, M. K.; BELL, J. M.; ULUSEN, D.
Reunión:
Congreso; AGU Fall Meeting 2009; 2009
Resumen:
Plasma in Titan's ionosphere flows in response to forcing from
thermal pressure gradients, magnetic forces, gravity, and ion-neutral
collisions. Analysis of the coupled ionosphere-magnetosphere dynamics is
difficult due to the complex mix of solar and magnetospheric geometries
that can exist (i.e., the angle of the ram direction of the external
flow relative to the subsolar point), due to the spherical nature of
Titan's neutral atmosphere, and due to the complex ion-neutral
chemistry. We will present an empirical approach to the ionospheric
dynamics by using data from several Cassini instruments to estimate
pressures, flow speeds, and time constants for both the dayside and
nightside. The coupling of the ionospheric plasma to the neutrals should
dominate the plasma transport below an altitude of roughly 1300 km.
Vertical or horizontal transport becomes more important than chemistry
in controlling ionospheric densities for altitudes above about 1400 -
1500 km, depending on the ion species. The structure of the ionospheric
magnetic field should be determined by plasma transport (including any
neutral wind effects) for altitude above about 1000 km and by magnetic
diffusion at lower altitudes. It is possible that sometimes a velocity
shear layer near 1300 km could exist and would affect the magnetic
field. Both Hall and polarization electric field terms in the magnetic
induction equation can be locally important in determining Titan's
ionospheric magnetic field. The dynamics associated with the
magnetospheric interaction with Titan's ionosphere is linked with
possible loss in the tail.