Small-scale and large-scale dynamos in global convection simulations of solar-like stars

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Table 2.

Energy densities for all runs.

Run	$E_{kin}^{tot}$ $E^{\mathrm{tot}}_{\mathrm{kin}}$	$E_{kin}^{dif}$ $E^{\mathrm{dif}}_{\mathrm{kin}}$	$E_{kin}^{mer}$ $E^{\mathrm{mer}}_{\mathrm{kin}}$	$E_{kin}^{flu}$ $E^{\mathrm{flu}}_{\mathrm{kin}}$	$E_{mag}^{tot}$ $E^{\mathrm{tot}}_{\mathrm{mag}}$	$E_{mag}^{tor}$ $E^{\mathrm{tor}}_{\mathrm{mag}}$	$E_{mag}^{pol}$ $E^{\mathrm{pol}}_{\mathrm{mag}}$	$E_{mag}^{flu}$ $E^{\mathrm{flu}}_{\mathrm{mag}}$	$E_{mag}^{tot} / E_{kin}^{tot}$ $E^{\mathrm{tot}}_{\mathrm{mag}}/E^{\mathrm{tot}}_{\mathrm{kin}}$	$E_{mag}^{flu} / E_{kin}^{flu}$ $E^{\mathrm{flu}}_{\mathrm{mag}}/E^{\mathrm{flu}}_{\mathrm{kin}}$
0M	2.225	1.562	0.006	0.658	0.369	0.072	0.048	0.250	0.166	0.379
0H	17.089	16.159	0.010	0.920

1M	1.267	0.546	0.006	0.716	0.604	0.172	0.047	0.385	0.476	0.538
1H	4.397	3.457	0.010	0.930

2M	0.933	0.213	0.005	0.715	0.763	0.198	0.044	0.521	0.819	0.729
2S	5.643	4.503	0.010	1.130	0.140	0.000	0.000	0.140	0.025	0.124
2H	8.697	7.514	0.012	1.171

3M	0.923	0.197	0.005	0.721	0.510	0.057	0.023	0.430	0.553	0.597
3S	1.448	0.542	0.007	0.900	0.228	0.000	0.000	0.228	0.158	0.254
3H	7.352	6.347	0.011	0.993

4M	0.854	0.144	0.005	0.705	0.876	0.190	0.030	0.656	1.026	0.931
4M2	1.016	0.132	0.006	0.879	0.604	0.009	0.006	0.590	0.594	0.671
4S	1.004	0.137	0.005	0.862	0.514	0.000	0.000	0.515	0.512	0.597

Notes. The energy densities (Cols. 2 to 9) are in 10⁵ J/m³, for their definitions see Eqs. (8)–(11).

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