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mist_regular_meetings [2020/04/30 15:54] al |
mist_regular_meetings [2020/04/30 15:55] (current) al |
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| 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. | 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?650|}} | + | {{:03_comparisont.png?800|}} |
| - | {{:04_comparison_ne.png?650|}} | + | Here are the electron density profiles. |
| - | {{:05_comparison_nH.png?650|}} | + | {{:04_comparison_ne.png?800|}} |
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| + | Here are the hydrogen density profiles. | ||
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| + | {{:05_comparison_nH.png?800|}} | ||