Titan Magnetic Tail: Does its Configuration correspond to the Induced Magnetosphere?

Abstract

Magnetic field structure observed in numerous Cassini flybys in the region of Titan interaction with the corotating flow of Kronian magnetosheric plasma contradicts the classical picture of the ideal induced magnetosphere produced by the magnetic field line draping about the obstacle. Clear draping is observed only upstream the Titan, but not in the Titan magnetic wake. We consider the magnetic field tension downstream the Titan magnetic tail and show that the magnetic field direction is not consistent with the induced magnetosphere produced by magnetic field lines draping. We arrive at the conclusion that the mechanisms alternative to the induced magnetosphere formation should be considered for the Titan magnetic surrounding.