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--- mist_regular_meetings [2020/04/30 15:44]
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+++ mist_regular_meetings [2020/04/30 15:55] (current)
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 **30 April 2020**
+Paris-Durham (PD) 50 km/s shock into WNM.
-{{:00_slab.png?400|}}
+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.
-{{:01_slabtemp.png?600|}}
+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|}}
+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|}}
+Here are the hydrogen density profiles.
+{{:05_comparison_nH.png?800|}}