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Table 1

Adopted parameters and initial conditions for the MHD models of accretion shocks.

Model |Blb | β slaba n str0 u str0 r str Magnetic field z dip Note
abbreviation [G] [cm-3] [km s-1] cm M yr-1 ] configuration [cm]

B50-D11-Unif 50 5 1011 500 1010 5 × 10-11 Uniform reference case
B500-D11-Unif 500 0.06 1011 500 1010 5 × 10-11 Uniform reference case
B50-D11-Dip1 50 10 1011 500 1010 5 × 10-11 Dipole − 3 × 1010
B500-D10.7-Dip1 500 0.05 5 × 1010 500 1010 2.5 × 10-11 Dipole − 3 × 1010
B500-D11-Dip1 500 0.2 1011 500 1010 5 × 10-11 Dipole − 3 × 1010
B50-D11-Dip2 50 100 1011 500 1010 5 × 10-11 Dipole − 1010
B500-D10.7-Dip2 500 10b 5 × 1010 500 1010 2.5 × 10-11 Dipole − 1010
B500-D11-Dip2 500 10b 1011 500 1010 5 × 10-11 Dipole − 1010

Notes.

(a)

βslab is an outcome of the simulation and is not set as an initial parameter.

(b)

In runs B500-D10.7-Dip2 and B500-D11-Dip2, βslab is measured in the slab generated by the oblique shock (see Sect. 3.2).

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