Dear Jose,
While I have not experimented in detail with the step-35 program, we have done extensive studies on similar problems in https://doi.org/10.1016/j.jcp.2017.09.031 (or https://arxiv.org/abs/1706.09252 for an earlier preprint version of the same manuscript) including the pressure correction scheme. While the spatial discretization is DG where some of the issues are , the experience from our experiments suggests that the pressure correction scheem should not behave too differently from other time discretization schemes with similar ingredients (say BDF-2 on the fully coupled scheme). In other words, I would expect second order convergence in the pressure for Taylor-Hood elements. I should note that there are some subtle issues with boundary conditions in projection schemes, so I cannot exclude some hidden problems with the step-35 implementation or the way you set up the experiments.
Best,
Martin
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'm not entirely clear about what your question is. Are you seeing convergence
rates that are too low or too large? It is not uncommon to have cases where a
scheme converges too fast (the convergence rate is too large); this is
typically the case because the solution has a symmetry.
Best
W.
While I have not experimented in detail with the step-35 program, we have done extensive studies on similar problems in https://doi.org/10.1016/j.jcp.2017.09.031 (or https://arxiv.org/abs/1706.09252 for an earlier preprint version of the same manuscript) including the pressure correction scheme. While the spatial discretization is DG where some of the issues are , the experience from our experiments suggests that the pressure correction scheem should not behave too differently from other time discretization schemes with similar ingredients (say BDF-2 on the fully coupled scheme). In other words, I would expect second order convergence in the pressure for Taylor-Hood elements. I should note that there are some subtle issues with boundary conditions in projection schemes, so I cannot exclude some hidden problems with the step-35 implementation or the way you set up the experiments.
Best,
Martin
Hello Jose,I wish I could help, but I second Wolfgang's question.Is your code available somewhere? I would be glad to take a look at it and compare the solutions for the same problems using different formulations. I would expect that if you fix the issue with boundary conditions (those described in the Guermond paper, that is the "pressure boundary layer") then you would recover exactly what you should get with traditional schemes using Taylor-Hood element (as Martin discussed).
if the velocity error you have is low enough, the somewhat time-independent PPE you solve given that velocity,you might get high enough rates up to a certain point -> and that point might lie below the error you see on those 3 levels.So, try to go for smaller timesteps (keeping the Re the same) and use more spatial refinement levels.In general I would also recommend changing the Reynold's number a bit around and see what happens - maybe it is an effect that is limited to low Re?Anyways, having a bigger convergence rate than expected is a nice problem to have, isn't it? ; )
-I would not think it is caused by a bug given the other rates looking just as expected!All the best,
Richard
I am happy to give further comments, but -- like Wolfgang -- I don't
quite understand what the precise question is. That said:
1. With projection schemes you will need to be careful about pressure
boundary layers. A good starting point might be the Elman, Silvester,
Wathen book.
2. Specific numerical test setups can be more or less sensitive to
this fact (size of pressure error vs velocity error, smoothness of
solutions in time, specific behavior on the boundary, ...)
--
Timo Heister
I don't support this idea. If you take the Taylor-Green vortex for
example, the velocity decays with exp(-2 nu t), while the pressure
decays with the square of that term. Why do you expect error from your
pressure-correction scheme and your error from the time discretization
to converge in the same way? Note that they are not completely
independent of course.
I am not convinced that this completely eliminates all influence of
the pressure-correction scheme. I assume that it still gives an O(dt)
additional error (or maybe something higher order depending on your
scheme).
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Hello Jose,I wish I could help, but I second Wolfgang's question.Is your code available somewhere? I would be glad to take a look at it and compare the solutions for the same problems using different formulations. I would expect that if you fix the issue with boundary conditions (those described in the Guermond paper, that is the "pressure boundary layer") then you would recover exactly what you should get with traditional schemes using Taylor-Hood element (as Martin discussed).I tried reformulating the question above. Hopefully it is clearer now. I will clean the code up and get back to you. The pressure-correction scheme I am using is the incremental rotational, which has the smallest error caused due to the boundary layer. Could the boundary layer in this case still cause such a strong influence?