All Tables

Table 1: The parameters $z_1^\prime$ (initial position of the boundary layer), $V^\prime$ (mean velocity of the boundary layer), and $\eta$ -q ( $\eta$ -quenching activated or not) that define the configurations analyzed, and the ranges of values of $B_{\rm s}$ , $C_\alpha$ and |q| used for the simulations. As regards $C_\alpha$ , we mainly used values between 5 and 200, since for smaller values the dynamo is not excited and for larger values the spin period would be too short.
Table 2: For each static configuration the critical value of $C_\alpha$ ( $C_{\alpha }^C$ ) and the corresponding global critical period of the PNS, $P_{\rm c}=\xi/C_{\alpha}^C~\rm ms$ , for $\xi \in [\rm 1,3]$ are reported.
Table 3: Ratio of the final intensity of the magnetic field in configurations A and B. The values in the table are calculated for |q|>10. For |q|<10 we still have ${\cal B}_{\rm t}^{\rm fin}(A)/{\cal B}_{\rm t}^{\rm fin}(B)>1$ and ${\cal B}_{\rm p}^{\rm fin}(A)/{\cal B}_{\rm p}^{\rm fin}(B)<1$ , but the exact value depends on the differential rotation.
Table 4: Indices of the power-law behaviour found in the dependence of $B^{\rm fin}$ on the degree of differential rotation |q| and the spin rate $C_\alpha$ . The errors, not reported in the table, are of a few percent only.