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Table 1

Three-dimensional view of a simulation setup with northward IMF orientation: density distribution (color scale), exoplanet magnetic field lines (red lines) and IMF (pink lines).

Model Rin Rout Rcr L(106 m) Rm η (108 m2 s−1) ν (108 m2 s−1)
B250 0.6 16 1.0 2.44 1800 1.37 0.30
B1000 0.8 30 1.4 4.30 1020 2.42 0.42
B6000 2.4 75 2.8 36.59 120 25.81 5.47
Q02 2.0 65 2.5 28.58 150 16.06 4.10
Q04 1.5 50 2.0 17.82 250 10.01 1.67

Notes. Model inner boundary (Col. 2), outer boundary (Col. 3), soft coupling region (Col. 4), characteristic length (Col. 5), numerical magnetic Reynolds number (Col. 6.), and numerical magnetic diffusivity (Col. 7).

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