. We find that on the dayside the solar energy deposition model overestimates the INMS-derived N + 2 production rates by a factor of 2. On the nightside, however, the model driven by suprathermal electron intensities from the Cassini Plasma Spectrometer Electron Spectrometer sometimes agrees and other times underestimates the INMS-derived N + 2 production rates by a factor of up to 2-3. We find that below 1200 km, all ion number densities correlate with the local ionization frequency, although the correlation is significantly stronger for short-lived ions than long-lived ions. Furthermore, we find that, for a given N 2 local ionization frequency, CH + 5 has higher densities on the dayside than on the nightside. We explain that this is due to CH 4 being more efficiently ionized by solar photons than by magnetospheric electrons for a given amount of N 2 ionization.