...and once more

Remaining figure to deal with:
3.2 - change in alpha in the small increments code - runs going on the c3

Tables:
3.2 - integrated dispersion at 10keV for different pitch angles etc (Earth); mine plus lorentzens - done!
3.3 - start, range and end points of dispersion region for different pitch angles - done!
3.4 - integrated dispersion at 10keV for different pitch angles etc (Jupiter): mine plus Earth ones - done!
3.5 - start, range and end points of dispersion region for different end points - done!

Finally, all tables are done, along with all possible graphs, with the exception of the one still going. When that one finishes, it and its conclusions will go in along with the typesetting of the rest and changing figure X's to actual numbered figures. Then Chapter three can join one and two in the Aylward pit.

Speaking of which, four pages have returned from their so far (one of which had no problems whatsoever, two had minor errors, one was a couple of graphs, which just confused him...).

So, will start corrections.

Done.

Onto chapter four.

The Chapter of Runs

Here is the new structure, worked out a while ago (you haven't forgotten already?):
New Chapter Four (current):
Introduction - done!
Model
-Cross-sections etc, general RIDE stuff
-Model Atmospheres for Jupiter, Saturn and Uranus
-Validation for Jupiter
-Inputs for Saturn
--In Situ
--UV Terrella
--IR
-Inputs for Uranus
--In Situ
--UV
--IR
Results
-Ion production and direct heating
-Chemistry (further)?
-Heating (further - Joule heating etc)?
-Photons?
-Sensitivities
Discussion
Conclusions

Of course, there are currently two versions of this, the converted version of the original paper and the uncoverted corrected paper. These will be slowly melded with the new structure and out will drop the final chapter as well as the paper itself.

Current figure list (suggested inclusions):
Cross-sections (they are the same for J, S and U), plus maybe photoionisation cross-sections and numbers, giving an idea of the scaling, a pair of figures.
Model atmospheres for J, S and U
Validations - Jovian monoruns as well as the Jovian full run
UV Terrella (Saturn oval plus terrella), another pair of figures
Uranus auroral map again, plus IR Uranus?
Ion production - two Saturnian cases, two Uranian cases (from Kim)
Heating, Saturn, Uranus
Energy degradation, Saturn, Uranus
Peak rate altitudes, Saturn and Uranus
Photons Saturn, Uranus?
Sensitivity graphs for Saturn, three whole 3D graphs
=26 figures (for those who can't count - me...)

Loadsa tables too, with heating and ion production for both planets, plus ratios of expected H3+ column densities from photo- and auroral ionisation. Could be fun...

That'll inflate the chapter. Frightening. But necessary.