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--- mist_regular_meetings [2020/04/30 15:48]
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+++ mist_regular_meetings [2020/04/30 15:55] (current)
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 Paris-Durham (PD) 50 km/s shock into WNM.
-To initialise PD we run a time evolution of a parcel of gas irradiated with an ISRF G0=1, cosmic ray rate zeta=10^-16 s-1.
+To initialise PD we run a time evolution of a parcel of gas at density n=0.1 cm-3, irradiated with an ISRF G0=1, and cosmic ray rate zeta=10^-16 s-1.
 This is the chemical evolution of that parcel, showing the electron fraction reaching ~10^-2.
 {{:00_slab.png?650|}}
 This is the temperature evolution of that parcel, reaching T~10^4 K.
 {{:01_slabtemp.png?650|}}
+Using the result of the above runs as the input (chemical abundances, temperature) for PD, here is a 50 km/s shock. This is the temperature and hydrogen density profile.
 {{:02_parisdurham.png?650|}}
-{{:03_comparisont.png?650|}}
+For comparison with mappings (Sutherland and Dopita 2017), several models were run. This is the temperature profiles of the PD shock (black), mappings with most basic settings (blue), basic + cosmic ray rate zeta=10^-17 s-1 (orange), basic + UV field (Mathis field, 9.50918E+09 phots/cm^2/s), basic + dust calculation.
+{{:03_comparisont.png?800|}}
+Here are the electron density profiles.
+{{:04_comparison_ne.png?800|}}
-{{:04_comparison_ne.png?650|}}
+Here are the hydrogen density profiles.
-{{:05_comparison_nH.png?650|}}
+{{:05_comparison_nH.png?800|}}