Weekend runs

Few more runs dun over the weekend. Saturn50 completed as expected, with no problems, also as expected, so another good reason to suspect the runs will be successful. Now just need to put Saturn50 back on for a full run.

Dun. Along with a clutch of Grodents, some phenomalogical work on Uranus and a few other bits and pieces.

Ok, present suggested system for Chapter Five:

Text:
Introduction
Modelling
-Tiros
--explanation of tiros
--Critique of Tiros
-RIDE ovation
--Introduction/RIDE validation
--Parameterisation validation and examples
Results
-CTIP runs with Tiros and with RIDE-O
Discussion
Conclusions

Figures:
5.1 - TIROS original schematic
5.2 - TIROS with Hi_tir and Hi_tir_max as well as DMSP included
5.3 - example standard ionisation output (per unit mass etc)
5.4 - example adjusted standard profile (ionisation rates)
5.5 - cross-sections over the energy range
5.6 - Validation of terrestrial RIDE
5.7 - Schematic of RIDE Ovation
5.8 - validation of parameterisartion
5.9 - example standard plot
5.10 - examples of output plots
...and so on

Tables:
5.1 - energy bands of TIROS
5.2 - energy bands of DMSP
...and so on (probably including later results)

Should put a bit about Richard Horne's stuff in there too, as it suggests further uses for the technique - must also qualify the use of this; normally CTIP is run during storm conditions (hence TIROS producing full oval coverage), but is limited by its pressure levels as to how high activity to go. For projects such as Alex's where lots of data is compared to CTIP, as the data is real data over a real timescale, it is mostly in the quiet time, so needs a quiet-time oval for a proper comparison.

Also done phenomalogical stuff for the final results chapter - after wondering how to fit the proton comparison to data in with the general theme of statistical patterns of electrons into a GCM, simple answer - high precision measuring of the characteristics of particle beams for later, better statistics and resultant models.

It makes sense to me...