Continuing

Ok, on with the checks:

1.38 KeV
100k

2.03 KeV
1M+ (Hurray!)

2.98 KeV
1M

4.4 KeV
1M+ (Hurray!)

6.4 KeV
10,000ok

9.4 KeV
1000ok

14 KeV
1000ok

20.8 KeV
1000ok

30.5 KeV
1000ok

...where 'ok' is listed it means the energy has been checked at that flux, but no higher yet. Higher energy electrons take longer to deal with as they pass through a larger slab of atmosphere, they penetrate into the small increments area requiring extra calculations, they last longer and they produce more secondaries that require thermalisation. Fortunately, above a certain energy, they're also able to fly through the atmosphere with few interactions. Unfortunately, we're not dealing with those energies...

There is a problem to be resolved to do with excitation recording, which mismatches altitudes and array size. This will be sorted. It is done. I'll compile at a later date - the program will, that is, not me myself.

Have grabbed even more profiles off Makenzie.