[Getdp] Magneto Dynamic
Christophe Geuzaine
cag32 at case.edu
Sat Nov 19 16:44:33 CET 2005
Alejandro Fernández Sela wrote:
> Dear Christophe:
>
> I am trying to understand the MagnetoDynamic 3D problem (wiki page)
> using the h-phi formulation, and I have some questions about it:
> I don't know why does the program need to call the MagSta formulation,
> Is it possible to build the code in only one formulation (one file) ?
In this particular formulation, you need a way to compute a "compatible"
source field. That's why the MagSta formulation is used. Look at the
reference mentioned in the .pro file for more info.
You can put all the formulations in a single file if you prefer, of course.
> Does the MagSta give the initial conditions, or is it used for all the
> resolution process?
It is used to compute the source field.
> Why do you use "Integral" instead of "Galerkin"(MagSta)?
These are actually synonyms. I've changed "Integral" into "Galerkin" in
the wiki.
> When I launch the program, using "getdp CoilAboveACore -solve
> MagDyn_hphi -pos Map_b Section_b Map_j Section_j" the convergence is not
> very fast. Could it be a problem of my "Solver" file? (I use the
> standard values).
You might want to increase the number of non-zero elements in the
incomplete ILU by increasing "Nb_Fill" in solver.par.
If you want to use a direct solver instead of an iterative algorithm,
you should download the source version and compile it with PETSc support
(./configure --enable-petsc).
> Is it really necesary to use "cuts" of the regions (done by the gmsh
> file) in order to solve that kind of problems (eddy currents)?
With this particular formulation: yes.
Christophe
> Thank you very much in advance, and thank you for developing that
> fantastic tool! I am really enjoying my work with it, and I am learning
> a lot about electromagnetism and FEA.
>
> Best regards!
>
>
>
>
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--
Christophe Geuzaine
Assistant Professor, Case University, Mathematics
http://www.case.edu/artsci/math/geuzaine