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Comments to species results.
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_tutorials/incompressible_flow/Inc_Species_Transport/Inc_Species_Transport.md

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@@ -65,7 +65,7 @@ For `CONV_NUM_METHOD_SPECIES= SCALAR_UPWIND` a second order MUSCL reconstruction
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The `TIME_DISCRE_SPECIES` can be either an implicit or explicit euler and a CFL reduction coefficient `CFL_REDUCTION_SPECIES` compared to the regular `CFL_NUMBER` is available.
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The iniital species mass fractions are given by the list `SPECIES_INIT= 1.0, ...`.
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The inital species mass fractions are given by the list `SPECIES_INIT= 1.0, ...`.
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`SPECIES_CLIPPING= YES` with the respective lists for min and max enforces a strict lower and upper limit for the mass fraction solution used by the solver.
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@@ -149,11 +149,17 @@ $ mpirun -n <#cores> SU2_CFD species3_primitiveVenturi.cfg
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## Results
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The case converges nicely as expected on such a simple case and mesh.
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![Residual plot](../../tutorials_files/incompressible_flow/Inc_Species_Transport/images/residuals_specMix.png)
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Figure (2): Residual plot (Incompressible mean flow, SST turbulence model, species transport).
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Note that there is still some unphysical mass fraction fluctuation for Species_0 at the junction corner. This becomes much less apparent by using `MUSCL_SPECIES = YES` but does not fully disappear.
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![Species Mass Fractions](../../tutorials_files/incompressible_flow/Inc_Species_Transport/images/speciesMassFractions.jpg)
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Figure (3): Volume mass fractions for both species. Species_1 is mirrored for better comparison.
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Velocity magnitude field along which the species are transported. For a much less homogenous mixture at the outlet one could decrease the `DIFFUSIVITY_CONSTANT` which makes for a more interesting optimization problem.
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![Velocity Magnitude](../../tutorials_files/incompressible_flow/Inc_Species_Transport/images/VelocityMag.jpg)
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Figure (4): Velocity Magnitude in the domain.

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