Physics
Scientific paper
Jul 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005georl..3220s06h&link_type=abstract
Geophysical Research Letters, Volume 32, Issue 20, CiteID L20S06
Physics
17
Magnetospheric Physics: Magnetospheric Configuration And Dynamics, Magnetospheric Physics: Numerical Modeling, Magnetospheric Physics: Planetary Magnetospheres (5443, 5737, 6033), Planetary Sciences: Fluid Planets: Magnetospheres (2756)
Scientific paper
We present the results of a 3D global magnetohydrodynamic simulation of the magnetosphere of Saturn for the period of Cassini's initial approach and entry into the magnetosphere. We compare calculated bow shock and magnetopause locations with the Cassini measurements. In order to match the measured locations we use a substantial mass source due to the icy satellites (~1 × 1028 s-1 of water product ions). We find that the location of bow shock and magnetopause crossings are consistent with previous spacecraft measurements, although Cassini encountered the surfaces further from Saturn than the previously determined average location. In addition, we find that the shape of the model bow shock and magnetopause have smaller flaring angles than previous models and are asymmetric dawn-to-dusk. Finally, we find that tilt of Saturn's dipole and rotation axes results in asymmetries in the bow shock and magnetopause and in the magnetotail being hinged near Titan's orbit (~20 RS).
Achilleos Nicholas
Dougherty K. M. K. M.
Gombosi Tamas I.
Hansen Kenneth Calvin
Hospodarsky George B.
No associations
LandOfFree
Global MHD simulations of Saturn's magnetosphere at the time of Cassini approach does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Global MHD simulations of Saturn's magnetosphere at the time of Cassini approach, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Global MHD simulations of Saturn's magnetosphere at the time of Cassini approach will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1250094