Fig. 11.From: The orientation of Titan’s dayside ionosphere and its effects on Titan’s plasma interactionThe final H1+ densities for case 1 (A), case 2 (B) and case 3 (C) at 1300 km altitude are shown. The densities are lower than the initial densities shown in Fig. 10 indicating that the ionosphere is no longer in photochemical equilibrium at this altitude. Dynamical processes are not important.Back to article page