Complex stuff
Remaining figures to deal with:
3.2 - change in alpha in the small increments code - runs queued on the c3
3.5 - dispersion at each altitude for 10keV protons - ready to do
3.6 - integrated dispersion for 10keV protons - ready to do
3.9 - product of scale height and collisions - ready to do
3.11 - dispersion at each altitude for 10keV protons - Jupiter - ready to do
3.12 - integrated dispersion for 10keV protons - Jupiter - ready to do
3.13 - gyroradius with altitude - Jupiter - needs calculations
3.14 - product of scale height and collisions - Jupiter - ready to do
Tables:
3.2 - integrated dispersion at 10keV for different pitch angles etc (Earth); mine plus lorentzens - ready to do
3.3 - start 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 - needs calculations
3.5 - start and end points of dispersion region for different end points - needs calculations
Ones that don't need cross-sections:
3.2 - change in alpha in the small increments code
3.13 - gyroradius with altitude - Jupiter
Alpha runs reset off due to runscript troubles...
So, back to cross-sections.
Now dealt with H/H+ cross-sections for O, O2, N, N2, H, H2, Ar, He, CH4 and C2H2 (the last two involving some calculations...). This allows me to do all except 3.13, which still requires the VIP model (yep, I did say that would be one of the easier ones, but I decided to tackle the harder ones first anyway...).
Values for tables 3.2 and 3.3 have been calculated. The other two require the gyroradii from 3.13. Magnetic colatitude of Jovian aurora is ~15, will take that for geog. coords too, as there are two places on the North side and two on the South that agree with this - plus its easier to remember.
Have worked through schmidt normalised associated legendre polynomials. It takes as long as it does to pronounce schmidt normalised associated polynomials, but isn't as exciting... I hate schmidt normalised associated legendre polynomials. Snalps?
3.2 - change in alpha in the small increments code - runs queued on the c3
3.5 - dispersion at each altitude for 10keV protons - ready to do
3.6 - integrated dispersion for 10keV protons - ready to do
3.9 - product of scale height and collisions - ready to do
3.11 - dispersion at each altitude for 10keV protons - Jupiter - ready to do
3.12 - integrated dispersion for 10keV protons - Jupiter - ready to do
3.13 - gyroradius with altitude - Jupiter - needs calculations
3.14 - product of scale height and collisions - Jupiter - ready to do
Tables:
3.2 - integrated dispersion at 10keV for different pitch angles etc (Earth); mine plus lorentzens - ready to do
3.3 - start 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 - needs calculations
3.5 - start and end points of dispersion region for different end points - needs calculations
Ones that don't need cross-sections:
3.2 - change in alpha in the small increments code
3.13 - gyroradius with altitude - Jupiter
Alpha runs reset off due to runscript troubles...
So, back to cross-sections.
Now dealt with H/H+ cross-sections for O, O2, N, N2, H, H2, Ar, He, CH4 and C2H2 (the last two involving some calculations...). This allows me to do all except 3.13, which still requires the VIP model (yep, I did say that would be one of the easier ones, but I decided to tackle the harder ones first anyway...).
Values for tables 3.2 and 3.3 have been calculated. The other two require the gyroradii from 3.13. Magnetic colatitude of Jovian aurora is ~15, will take that for geog. coords too, as there are two places on the North side and two on the South that agree with this - plus its easier to remember.
Have worked through schmidt normalised associated legendre polynomials. It takes as long as it does to pronounce schmidt normalised associated polynomials, but isn't as exciting... I hate schmidt normalised associated legendre polynomials. Snalps?
Labels: Chapter Three, latex, Thesis
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