I work in the design of ground based optical systems used in Astrophysics. One effect we frequently have to correct for is atmospheric dispersion. This is relatively straightforward, and in many cases the current atmospheric model built into Zemax is sufficient. However, when working at extremely high resolution (for example in Adaptive Optics) the current implementation in Zemax is not good - the data used to calculated atmospheric dispersion is using data which is out of date - the data from Hohenkerk and Sinclair underestimates the dispersion.
Is there any likelihood this will be updated to more recent data?