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Implement Collisionless heat flux into the Braginskii module #317
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…lay which slope limiter is used, fixed typo in the braginskii doc
updated ShowConfig functions from braginskii tc and viscosity to disp…
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Hum, it looks like the non regression tests from the FargoMHDspherical is trying to compare 16x16x128 cubes with 16x16x64 cubes. I did not touch this file, is this expected ? |
glesur
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Ok, except for the userdef function signature which would benefit from using a single std::vector<IdefixArray3D> as parameter for all of the implementations.
glesur
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All good, just change std::vector[] by std::vector.at() and we're good to go
## [2.2.01] 2025-04-16 ### Changed - Fix a bug that led to instabilities in the RKL scheme with very small grid spacings (#323) - Fix a bug that prevented Idefix from running with Sycl backend (required on Intel GPUs) (#331) - Fix an error that led to incorrect electrical current regularisation around the polar axis in non-Ideal MHD (#333) - Improve div(B) checks with a dimensionless implementation, avoiding too large divB errors in grids with large stretch factors (#334) ### Added - Time-Implicit drag for multiple dust species, preventing small time steps for strongly coupled dust grains (#321) - Collisionless heat flux added to the Braginskii module (#317) - New global `idfx::DumpArray` debugging function to dump any Idefix array into a numpy array that can read from python (#318) - Automatic benchmark plots in the documentation (#319) - More CI tests of grid coarsening (#329) - Dump outputs based on wallclock time (#335) --------- Co-authored-by: Victor Réville <victorreville@gmail.com> Co-authored-by: Hal Bal <vreville@irap.omp.eu> Co-authored-by: Jean Kempf <jean.kempf@irap.omp.eu> Co-authored-by: Victor Réville <47865059+vreville@users.noreply.github.com> Co-authored-by: Marc Coiffier <marc.coiffier@univ-grenoble-alpes.fr> Co-authored-by: pre-commit-ci-lite[bot] <117423508+pre-commit-ci-lite[bot]@users.noreply.github.com>
This PR adds an option to the
bragTDiffusionmodule. A new keyword is set to eithernosatorwcless. With the latter, the heat flux is a combination of the Braginskii heat flux and a collisionless heat flux \propto p v (where p is the thermal fluid pressure and v the bulk velocity). The transition from the Braginskii to the collisionless form is handled through a third parameter alpha (typically an array that depends on the coordinates or the density) while the amplitude of the collisionless heat flux is controlled by a fourth parameter beta, usually constant but can be userdef.A test and 1D example is given in test/MHD/clessTDiffusion/.
bragTDiffusion tests have been updated to include the new option.