Table 3: Initial magnetic energy $E_{{\rm mag}}$ and typical values of the ratio of magnetic to gravitational energy $\beta _{{\rm mag}}$ (the exact values depend also on the hydrodynamic initial model and its gravitational energy) for the models of series AaBbGg-DdM12. The magnetic energy of models with $b_0 \ne 10^{12}~{\rm G}$ can be obtained by a simple scaling relation, e.g. $E_{{\rm mag}}^{{\rm AaBbGg-D2M10}} = E_{{\rm mag}}^{{\rm AaBbGg-D2M12}}~ (10^{10} / 10^{12})^2$ .
Model $E_{{\rm mag}} \ [{\rm erg}]$ $\log \beta_{{\rm mag}}$

D0M12 $1 \times 10^{49}$ -2.7

D4M12 $6 \times 10^{48}$ -3.0

D3M12 $7 \times 10^{47}$ -3.9

D2M12 $7 \times 10^{46}$ -4.9

D1M12 $1 \times 10^{46}$ -5.8

**Table 3:** Initial magnetic energy $E_{{\rm mag}}$ and typical values of the ratio of magnetic to gravitational energy $\beta _{{\rm mag}}$ (the exact values depend also on the hydrodynamic initial model and its gravitational energy) for the models of series AaBbGg-DdM12. The magnetic energy of models with $b_0 \ne 10^{12}~{\rm G}$ can be obtained by a simple scaling relation, e.g. $E_{{\rm mag}}^{{\rm AaBbGg-D2M10}} = E_{{\rm mag}}^{{\rm AaBbGg-D2M12}}~ (10^{10} / 10^{12})^2$ .
Model	$E_{{\rm mag}} \ [{\rm erg}]$	$\log \beta_{{\rm mag}}$
D0M12	$1 \times 10^{49}$	-2.7
D4M12	$6 \times 10^{48}$	-3.0
D3M12	$7 \times 10^{47}$	-3.9
D2M12	$7 \times 10^{46}$	-4.9
D1M12	$1 \times 10^{46}$	-5.8

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