...continuing...

Text:
Results
-Ion production and direct heating - needs results
-Chemistry (further)? - needs coding
-Heating (further - Joule heating etc)? - needs coding
-Photons - needs results
-Sensitivities - needs results
Discussion - needs results
Conclusions - needs results

Figures:
4.6 - Validation monoruns - runs ongoing
4.13 - Uranus North ion production - ongoing
4.14 - Uranus South ion production - ongoing
4.16 - Uranus heating - ongoing
4.19 - Peak rate altitudes, Uranus - needs runs
4.24 - H3+ densities for three cases Saturn(?) - needs coding, runs
4.25 - H3+ densities for three cases Uranus(?) - needs coding, runs
4.26-8 - Sensitivity graphs for Saturn, three whole 3D graphs - runs ongoing

Tables:
4.2 - Ion production Uranus - runs ongoing
4.4 - Heating Uranus - runs ongoing
4.5 - H3+ Saturn(?) - needs coding, runs
4.6 - H3+ Uranus(?) - needs coding, runs

Modelling required:
Validation runs (three cases - highly intensive due to powerful aurora) - ongoing
Uranus runs (two cases - very low intensity aurora) - ongoing
Chemistry module - coding to update for certain Steve based things, then runs using model atmospheres and ion production
Sensitivities - you can't miss these runs, they've been going for a year now... - ongoing

First of the alpha runs has been completed - the one on rimmer. How long will the others take? It is mere days until they run out of time... The results for the first one are as hopeless as could be hoped for (this is the run with the small increments code completely turned off to show how essential it is to have the code).

After some problems with the code, the chemistry thing is slowly coming back to life. Helium is still a bit dodgy, but will see.

Garden Party Time