Physics – Plasma Physics
Scientific paper
May 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusm.p41a..06l&link_type=abstract
American Geophysical Union, Spring Meeting 2008, abstract #P41A-06
Physics
Plasma Physics
1
2700 Magnetospheric Physics (6939), 6000 Planetary Sciences: Comets And Small Bodies, 7800 Space Plasma Physics
Scientific paper
We discuss the results of the hybrid simulation of Titan's environment in case of T9 encounter. The simulations are based on recent analysis of the Cassini Plasma Spectrometer (CAPS) ion measurements during the T9 flyby through the induced magnetic tail of Titan [Sittler et al, 2008]. This new result changes our previous model of the interaction of Saturn's rotating magnetosphere with Titan from one that was discussed in the recent publications. The current simulation shows that mass loading by pickup ions H+, H_2+, CH4+ and N2+ is stronger than in the previous simulations. In our hybrid simulations we use Chamberlain profiles for the exosphere's components. We also include a simple ionosphere model. Special attention will be paid to comparing our numerical results with Cassini T-9 observations. We shall estimate the mass loading rate and the energy input to the upper atmosphere from ambient and pickup ions for the T9 encounter. E C Sittler et al., Spring AGU Meeting, 2008.
Hartle Richard E.
Lipatov Alexander S.
Sittler Edward C.
No associations
LandOfFree
Titan's plasma environment for T9 encounter: 3D hybrid simulation and comparison with observations 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 Titan's plasma environment for T9 encounter: 3D hybrid simulation and comparison with observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Titan's plasma environment for T9 encounter: 3D hybrid simulation and comparison with observations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1397652