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talk.qmd

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@@ -912,18 +912,59 @@ Now, if we wanted to reconstruct all the cells of the finest level, we'd only ne
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## Burgers results (MR+MLF sol. order 1) small hat {.fs-6}
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## Burgers 2D results (MR+MLF solution order 1)
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::::{.center-page-vertically}
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:::{.text-center}
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<video data-autoplay width="99%" src="videos/burgers2d.mp4" />
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:::
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::::
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---
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## Euler 2D results (MR+MLF solution order 3 (OSMP scheme))
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<!-- :::{.text-center}
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<video data-autoplay width="80%" src="videos/burgers/MRA_upwind_with_portion-min_1-max_12-eps_0.01-reg_0.mp4" />
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![](figures/Bsvortex_osmp3_InitialState_MRAMLF_eps1e-03.png){width=47%}
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![](figures/Bsvortex_osmp3_Tf10_MRAMLF_eps1e-03.png){width=47%}
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::: -->
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{{< include python_sections/anim_hat_bis.qmd >}}
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::: {layout-nrow=2}
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![](figures/Bsvortex_osmp3_InitialState_MRAMLF_eps1e-03.png){width=47%}
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![](figures/Bsvortex_osmp3_Density_T00_MRAMLF_eps1e-03.png){width=47%}
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![](figures/AdaptedMesh_BSvortex_Tf10_level3_9_eps1e-03_MRAFLF_highest.png){width=47%}
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![](figures/Density_contours_BSvortex_Tf10_level3_9_eps1e-03_MRAFLF_highest.png){width=47%}
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<!-- ![](figures/Bsvortex_osmp3_Density_T00_MRAMLF_eps1e-03){width=47%}
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![](figures/Bsvortex_osmp3_VelocityMagnitude_T00_MRAMLF_eps1e-03.png){width=47%}
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![](figures/Bsvortex_osmp3_Density_T10_MRAMLF_eps1e-03.png){width=47%}
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![](figuresBsvortex_osmp3_VelocityMagnitude_T10_MRAMLF_eps1e-03.png){width=47%} -->
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:::
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## Burgers results (MR+MLF sol. order 1) sinus {.fs-6}
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## Euler 2D results (MR+MLF solution order 3 (OSMP scheme))
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<!-- :::{.text-center}
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![](figures/Bsvortex_osmp3_InitialState_MRAMLF_eps1e-03.png){width=47%}
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![](figures/Bsvortex_osmp3_Tf10_MRAMLF_eps1e-03.png){width=47%}
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::: -->
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::: {layout-nrow=2}
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![](figures/Bsvortex_osmp3_InitialState_MRAMLF_eps1e-03.png){width=47%}
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![](figures/VelocityMagnitude_contours_BSvortex_Tf00_level3_9_eps1e-03_MRAFLF_highest.png){width=47%}
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![](figures/AdaptedMesh_BSvortex_Tf10_level3_9_eps1e-03_MRAFLF_highest.png){width=47%}
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![](figures/VelocityMagnitude_contours_BSvortex_Tf10_level3_9_eps1e-03_MRAFLF_highest.png){width=47%}
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:::
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{{< include python_sections/anim_sin_bis.qmd >}}
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# Adaptive mesh refinement software
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---
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## Five projects - NASA Modelling Summer Visit 2025
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Five groups from France involving 15 students / post-doctoral fellows / research software engineers / faculties
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- Mathematical modeling and simulation of non-equilibrium plasmas for the prediction of electric propulsion and plasma discharges including sheath
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- Code coupling : multistep coupling algorithm (Tuesday's seminar)
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- A two-phase flow model with scale separation for the separated-to-disperse phase transition in high-velocity regimes
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- A dual splitting/ImEx strategy for multicomponent reacting flows with space/time adaptation and error control
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- Simulation of hybrid dense-rarefied flows relying on relaxation schemes and a
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hierarchy of moment methods
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:::{.row .text-center .align-items-center}
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::::{.col}
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![](figures/logo_nasa.jpg){height="130px"}
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::::
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::::{.col}
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![](figures/ESM-logo.png){height="110px"}
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::::
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::::{.col}
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![](figures/logo.png){height="130px"}
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::::
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::::{.col}
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![](figures/logo_polytechnique.png){height="100px"}
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::::
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:::{.row .text-center}
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<h3>Thank you for your attention</h3>
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## Burgers results (MR+MLF sol. order 1) small hat {.fs-6}
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<!-- :::{.text-center}
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<video data-autoplay width="80%" src="videos/burgers/MRA_upwind_with_portion-min_1-max_12-eps_0.01-reg_0.mp4" />
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::: -->
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{{< include python_sections/anim_hat_bis.qmd >}}
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---
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## Burgers results (MR+MLF sol. order 1) sinus {.fs-6}
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{{< include python_sections/anim_sin_bis.qmd >}}
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---
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:::{.text-center}
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<div>
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<video data-autoplay width="80%" src="videos/burgers/MRA_upwind_without_portion-min_1-max_12-eps_0.01-reg_0.mp4" />

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