...and again...

Remaining figures to deal with:
3.2 - change in alpha in the small increments code - runs going on the c3
3.11 - dispersion at each altitude for 10keV protons - Jupiter - done!
3.12 - integrated dispersion for 10keV protons - Jupiter - done!
3.13 - gyroradius with altitude - Jupiter - done!
3.14 - product of scale height and collisions - Jupiter - done!

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

This really is dragging on...

Have calculated pressure change range as well as the other dispersion ranges - ie if the Jovian atmosphere had the same constituents as the terrestrial atmosphere, what would the range be. It seems the actual Jovian range is one and a half that range, which is interesting as it shows the Jovian atmosphere to be inherently more dispersing as well as happening to be more dispersing due to its different gyroradii and depth.

Gyroradii done. The openning volley of an evenning of graphs and tables, I hope...
Dispersion done. The graph, not the subject, oh, if only...
Integrated dispersion done. This leaves one doable graph and four tables, plus associated conclusions, and I have a big one to include now...
Collisions over a scale height also now done, leaving just the alpha runs, which are out of my control.

Tables are to be done tomorrow, however, conclusions were done today.