Investigation of the 3D-Magnetic Field Structure of the Titan Interaction with the Kronian Outer Magnetosphere near ~ 10 SLT Using Magnetic Field Data and Modelling: Draping Boundary and Polarity Reversal Layer

Details Investigation of the 3D-Magnetic Field Structure of the Titan Interaction with the Kronian Outer Magnetosphere near ~ 10 SLT Using Magnetic Field Data and Modelling: Draping Boundary and Polarity Reversal Layer Investigation of the 3D-Magnetic Field Structure of the Titan Interaction with the Kronian Outer Magnetosphere near ~ 10 SLT Using Magnetic Field Data and Modelling: Draping Boundary and Polarity Reversal Layer

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufm.p43a0956n&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #P43A-0956

Physics

2732 Magnetosphere Interactions With Satellites And Rings, 2736 Magnetosphere/Ionosphere Interactions (2431), 2780 Solar Wind Interactions With Unmagnetized Bodies, 6281 Titan

Scientific paper

We shall use magnetic field data from the Titan encounters TA,TB,T3,T8 at 10.6,10.5,10.3 and 9.3 Saturnian Local Time,respectively, and theoretical results from the Advanced 3D-model by Backes et al.[2005]to continue our investigation of the 3D-magnetic field in Titan's induced magnetosphere.In this paper we shall study the draping boundary,which is often seen as a relatively well defined 1.order discontinuity in the magnetic field.Its cross-section is close to an ellipse with the semimajor axis parallel to the initial magnetic field direction and a displacement towards the dayside of Titan away from Saturn.Using flyby T8 we shall try to follow its development forward to the bow of the structure. A suitably defined dynamical draping coordinate system will aid in the structural studies of the polarity reversal layer of the near tail.

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