INVESTIGADORES
BERTUCCI Cesar
congresos y reuniones científicas
Título:
Distortion of Saturn's Magnetopause Surface Observed by Cassini
Autor/es:
ACHILLEOS, NICHOLAS A.; ARRIDGE, C. S.; BERTUCCI, C.; MCANDREWS, H. J.; DOUGHERTY, M. K.; COATES, A. J.; CASSINI MAGNETOMETER TEAM
Reunión:
Congreso; American Astronomical Society, DPS meeting #38; 2006
Resumen:
The Cassini spacecraft has now encountered Saturn's magnetopause
boundary over 100 times, during more than 20 orbits of the planet.
During the compilation of minimum variance analyses for the inbound
`Rev 5' orbit (March 2005), we have detected what appears to
be a significantly `distorted' orientation of the
magnetopause for the final pair of crossings on the inbound leg. This
pair of crossings encloses a brief ( 10 minute) excursion into the
planetary magnetosheath (as revealed by the CAPS instrument), which
occurred an unusually long time (>6 hours) and distance (3 RS =
Saturn radii) after the earlier group of at least seven clear
magnetopause encounters. Application of an equilibrium magnetopause
model indicates that the standoff distance changed from 20 to 17 RS
during this time interval and that the model solar wind pressure
correspondingly changed by a factor of nearly two. Therefore, a strong
magnetospheric compression is indicated. Minimum variance analysis (MVA)
reveals that all the crossings correspond to a tangential discontinuity.
Moreover, the angle between the MVA and model normals is in the range
10-35 deg for the early group of encounters, but increases to 50-60 deg
for the pair associated with the compressed configuration. The magnetic
data acquired by the MAG instrument show that the field during the brief
( 10 min) magnetosheath excursion associated with the compression
reached orientations nearly orthogonal to a model of the unperturbed
magnetopause surface. The observations are consistent with a sharp
`depression' in the magnetopause surface with a sunward
component of motion. If an anti-sunward moving disturbance is assumed,
then we require an even more distorted, `folded'
magnetopause in order to explain the observations.