Coriolis darkening in late-type stars - II. Effect of self-sustained magnetic fields in stratified convective envelopes

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Table B.3.

Set of simulations used in this work. The third last columns provide the time- and volume-averaged global Rossby number Ro = u_rms/Ωd, Reynolds number Re = Ro/E, and Nusselt number Nu. Here, u_rms is the time-and volume-averaged root mean squared total velocity. The (/) symbol for Pm indicates hydrodynamic runs.

N_ρ	Pr	E	Ra/Ra_c	Pm	Ro	Re	Nu
3	1	3 × 10⁻⁵	1.7	0.5	0.0030	101	1.71
3	1	3 × 10⁻⁵	1.7	1	0.0029	97	1.83
3	1	3 × 10⁻⁵	1.7	2	0.0031	104	1.73
3	1	3 × 10⁻⁵	1.7	3	0.0029	98	1.84
3	1	3 × 10⁻⁵	2.5	0.5	0.0062	207	2.81
3	1	3 × 10⁻⁵	2.5	1	0.0055	183	2.82
3	1	3 × 10⁻⁵	2.5	2	0.0057	189	2.95
3	1	3 × 10⁻⁵	2.5	3	0.0053	178	2.85
3	1	3 × 10⁻⁵	2.5	4	0.0045	149	2.73
3	1	3 × 10⁻⁵	3.7	1	0.0095	318	4.85
3	1	3 × 10⁻⁵	3.7	3	0.0090	301	5.30

3	0.3	3 × 10⁻⁵	2.8	0.5	0.0075	251	1.49
3	0.3	3 × 10⁻⁵	2.8	1	0.0079	262	1.70
3	0.3	3 × 10⁻⁵	2.8	2	0.0072	240	1.66
3	0.3	3 × 10⁻⁵	3.4	0.5	0.010	338	1.86

3	0.3	3 × 10⁻⁵	3.4	1	0.0090	300	1.94
3	0.3	3 × 10⁻⁵	3.4	2	0.0082	274	2.10
3	0.3	3 × 10⁻⁵	4.1	0.5	0.015	496	2.35
3	0.3	3 × 10⁻⁵	4.1	1	0.014	463	2.90
3	0.3	3 × 10⁻⁵	4.1	2	0.010	341	2.50

3.5	1	10⁻⁴	2.8	0.5	0.014	142	2.86
3.5	1	10⁻⁴	2.8	1	0.013	132	2.80
3.5	1	10⁻⁴	2.8	5	0.013	134	3.16
3.5	1	10⁻⁴	5.5	0.25	0.031	310	5.46
3.5	1	10⁻⁴	5.5	0.5	0.032	316	5.70
3.5	1	10⁻⁴	5.5	1	0.030	299	5.80
3.5	1	10⁻⁴	5.5	5	0.024	241	5.65

4	0.3	3 × 10⁻⁵	2.5	0.5	0.0071	235	1.25
4	0.3	3 × 10⁻⁵	2.5	2	0.0058	193	1.51
4	0.3	3 × 10⁻⁵	3	0.3	0.015	491	1.12
4	0.3	3 × 10⁻⁵	3	0.5	0.0091	303	1.50
4	0.3	3 × 10⁻⁵	3	2	0.0070	235	1.52
4	0.3	3 × 10⁻⁵	6.3	0.1	0.026	854	3.25
4	0.3	3 × 10⁻⁵	6.3	0.15	0.025	828	3.63
4	0.3	3 × 10⁻⁵	6.3	0.3	0.024	805	3.72
4	0.3	3 × 10⁻⁵	6.3	0.5	0.023	775	3.90
4	0.3	3 × 10⁻⁵	6.3	1	0.021	707	4.00
4	0.3	3 × 10⁻⁵	6.3	2	0.022	735	3.80
4	0.3	3 × 10⁻⁵	2.5	0.5	0.0071	235	1.25
4	0.3	3 × 10⁻⁵	2.5	2	0.0058	193	1.51
4	0.3	3 × 10⁻⁵	3	0.3	0.015	491	1.12
4	0.3	3 × 10⁻⁵	3	0.5	0.0091	303	1.50
4	0.3	3 × 10⁻⁵	3	2	0.0070	235	1.52
4	1	10⁻⁴	9.8	0.15	0.062	622	7.29
4	1	10⁻⁴	9.8	0.25	0.049	490	7.75
4	1	10⁻⁴	9.8	1	0.045	452	7.75
4	1	10⁻⁴	9.8	2	0.040	396	7.76
4	1	10⁻⁴	9.8	3	0.036	363	7.78
4	1	10⁻⁴	29	/	0.23	2300	12.4
4	1	10⁻⁴	29	0.15	0.23	2275	17.2
4	1	10⁻⁴	29	0.25	0.33	3300	16.0
4	1	10⁻⁴	29	1	0.042	420	14.5

5	1	10⁻⁴	4.2	0.25	0.022	221	2.35

5	1	10⁻⁴	4.2	1	0.016	163	2.65
5	1	10⁻⁴	4.2	5	0.014	138	2.82
5	1	10⁻⁴	6.2	0.25	0.026	264	3.48
5	1	10⁻⁴	6.2	0.4	0.024	242	3.90
5	1	10⁻⁴	6.2	1	0.024	238	3.75
5	1	10⁻⁴	6.2	2	0.024	235	4.05
5	1	10⁻⁴	6.2	3	0.023	226	4.00
5	1	10⁻⁴	6.2	5	0.019	190	3.80
5	1	10⁻⁴	8.3	0.25	0.032	319	4.32
5	1	10⁻⁴	8.3	0.4	0.028	282	5.03
5	1	10⁻⁴	8.3	1	0.026	263	5.00
5	1	10⁻⁴	8.3	2	0.027	270	4.80
5	1	10⁻⁴	8.3	3	0.028	282	4.90
5	1	10⁻⁴	16	0.25	0.16	1586	5.60
5	1	10⁻⁴	16	1	0.048	483	6.90
5	1	10⁻⁴	16	2	0.044	439	7.05
5	1	10⁻⁴	32	0.25	0.46	4550	20.5
5	1	10⁻⁴	32	1	0.11	1056	16.1
6	1	3 × 10⁻⁴	3	/	0.021	70	1.39
6	1	3 × 10⁻⁴	3	6	0.017	57	1.43
6	1	3 × 10⁻⁴	4	1	0.035	117	1.70
6	1	3 × 10⁻⁴	4	2	0.028	94	1.75
6	1	3 × 10⁻⁴	4	3	0.024	81	1.81
6	1	3 × 10⁻⁴	8	/	0.087	288	2.42
6	1	3 × 10⁻⁴	8	1	0.047	155	2.62
6	1	3 × 10⁻⁴	8	2	0.043	142	2.73
6	1	3 × 10⁻⁴	8	3	0.042	139	2.79
6	1	3 × 10⁻⁴	16	/	0.15	505	3.43
6	1	3 × 10⁻⁴	16	1	0.15	501	3.32
6	1	3 × 10⁻⁴	16	2	0.066	221	3.52
6	1	3 × 10⁻⁴	16	3	0.065	218	3.55
6	1	3 × 10⁻⁴	32	/	0.18	611	5.51
6	1	3 × 10⁻⁴	32	2	0.20	673	4.88

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