Fig. 25.
From: The orientation of Titan’s dayside ionosphere and its effects on Titan’s plasma interaction
Polar view of the magnitude of the magnetic field around Titan for case 2 is shown. There is a buildup in the field strength to about 12 nT at the sub-flow point. The magnetic field strength is also increased above and below the poles as the field drapes around Titan. The results for the other to cases in this plane are nearly identical.