Fig. 9.From: The orientation of Titan’s dayside ionosphere and its effects on Titan’s plasma interactionThe Log of the final H1+ densities for case 1 (A), case 2 (B) and case 3 (C) at 1200 km altitude are shown. The densities are represented by 10s of thousands of particles in each cell of the chemistry grid. The results show good agreement with the 1-dimensional photochemical results shown in Fig. 2 indicating that the ionosphere is in photochemical equilibrium at this altitude.Back to article page