Magnetic field morphologies in convective zones influenced by a turbulent surface layer

Open Access

Table B.1.

A summary of simulations in this paper and their parameters.

Label	$\tilde{Ra}$ $\widetilde{Ra}$	Ra_F^*	Ro	Re	Rm	Nu	$E_{mag}^{l \leq 7, m = 0} / E_{mag}^{l \leq 7}$ $E^{l\leq 7, m = 0}_{mag}/E^{l\leq 7}_{mag}$	$E_{mag}^{m = 0} / E_{mag}^{tot}$ $E^{m = 0}_{mag}/E^{tot}_{mag}$
N_ρ = 2, Ra_cr = 1.483 ⋅ 10⁵

`n21`	32	2.32 ⋅ 10⁻³	0.615	517	1035	18.1	0.146	0.043

`n22`	64	7.31 ⋅ 10⁻³	0.955	816	1633	28.5	0.102	0.0287

`n23`	72	7.75 ⋅ 10⁻³	0.971	865	1731	26.9	0.147	0.0294

`n24`	96	12.82 ⋅ 10⁻³	1.01	1224	2448	33.4	0.137	0.044

N_ρ = 4, Ra_cr = 4.224 ⋅ 10⁵

`n41`	16	2.74 ⋅ 10⁻³	0.393	528	264	9.2	0.254	0.091

`n42`	32	9.28 ⋅ 10⁻³	0.664	459	918	15.6	0.150	0.028

N_ρ = 6, Ra_cr = 6.898 ⋅ 10⁵

`n61`	4	0.13 ⋅ 10⁻³	0.057	28.4	56.8	1.76	0.03	0.037

`n62`	8	0.41 ⋅ 10⁻³	0.116	57.6	115.3	2.75	0.597	0.264

`n63`	16	1.05 ⋅ 10⁻³	0.181	98	197	3.5	0.437	0.202

`n64`	32	3.76 ⋅ 10⁻³	0.295	352	704	6.3	0.293	0.071

Notes. All parameters were averaged over time, except of $\tilde{Ra}$ $\widetilde{Ra}$ . The run n61 with $\tilde{Ra} = 4$ $\widetilde{Ra} = 4$ near convection onset corresponds to weakly developed turbulence and has a strongly non-axisymmetric large-scale magnetic field, concentrated in the southern hemisphere and was not discussed here in detail.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.