Chapmann Layer

This simulation calculate the ion production rate calculated by Chapman. This follows the verison in Chapter 5 of "Theory of Planetary Atmospheres" by Chamberlain and Hunten, Academic Press (1978).

The simulation allows the user to adjust parameters that enter into the scale height and the EUV  flux. Based on these inputs it plots the (single species) Neutral Density and the ion production rate against the altitude.