Ultimate large-Rm regime of the solar dynamo | Astronomy & Astrophysics (A&A)

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Table B.1.

Index of runs: V (viscous), M (moderate), T (turb.) runs from R21 ; S01 (Super-turb.) is new. Re = u_rms/(k_fν) and Rm = u_rms/(k_fη).

Run	(N_x, N_y, N_z)	L_z/L_f	ν⁻¹	η⁻¹	Pm	Re	Rm	u_rms	B_rms	${\bar{B}}_{rms}$ $Mathematical equation: $ {\overline{B}}_{\mathrm{rms}} $$
V02	(64, 64, 256)	4	500	500	1	46.2	46.2	0.58	0.57	0.42
V03	(128, 128, 512)	4	500	2000	4	39.9	159.7	0.50	0.54	0.21
V04	(128, 128, 512)	4	500	8000	16	35.6	570.0	0.44	0.58	0.14
V05	(256, 256, 1024)	4	500	16000	32	32.9	1054.0	0.41	0.59	0.12
M02	(64, 64, 256)	4	2000	500	0.25	197.6	49.4	0.62	0.56	0.38
M03	(128, 128, 512)	4	2000	2000	1	177.0	177.0	0.56	0.59	0.32
M04	(128, 128, 512)	4	2000	8000	4	163.3	653.2	0.51	0.60	0.18
M05	(256, 256, 1024)	4	2000	16000	8	165.9	1327.5	0.52	0.60	0.12
T02	(128, 128, 512)	4	8000	500	0.062	846.6	52.9	0. 66	0.58	0.42
T03	(128, 128, 512)	4	8000	2000	0.25	749.3	187.3	0.59	0.58	0.25
T04	(128, 128, 512)	4	8000	8000	1	748.1	748.1	0.58	0.60	0.16
T05	(256, 256, 1024)	4	8000	16000	2	683.4	1366.8	0.54	0.63	0.17
T06	(512, 512, 2048)	4	8000	32000	4	694.5	2778.0	0.55	0.62	0.12
S01	(512, 512, 2048)	4	32000	16000	0.5	2904.5	1452.2	0.57	0.63	0.15

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