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![logo_short_small](uploads/1e4ee858ca174663b210647640da0976/logo_short_small.png) `4`
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![logo_short_small](uploads/1e4ee858ca174663b210647640da0976/logo_short_small.png) `4.1`
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The following limitations in the code usage apply with respect to
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geometry, AMR and MPI:
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The following notes and limitations in the code usage apply with respect to
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geometry, AMR, MPI and numerical methods:
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- Rectangular domain decomposition in *ϕ*-direction (cylindrical- and
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spherical coordinates) and *θ*-direction (spherical coordinates) is
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... | ... | @@ -9,9 +9,15 @@ geometry, AMR and MPI: |
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non-local character of such BC.
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- AMR is generally not working in combination with standard BC of
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’F’-type.
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’F’-type because of its non-local character.
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- The selfgravity solver works only for 3D Cartesian geometry.
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- The selfgravity solver works only in 3D Cartesian geometry or in 2D
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axissymmetric cylindrical geometry when the cylinder axis is included.
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- The magnetic field splitting scheme becomes unstable when the magnetic
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energy density associated with the evolved residual field becomes too large
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compared to the thermal energy density for unknown reason. The HLLD+CT algorithm
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is more affected by this than the CU+CCT algorithm.
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