Exploring the P vs. P relation with flux transport dynamo models of solar-like stars

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Table 2:

Starspot cycle period (in year), maximum of toroidal field (in 10⁴ G) at the base of the CZ and ratio between poloidal and toroidal field for 10 different cases with various rotation rates.
Case	$\Omega_{0}/\Omega_{\rm S}$	Cycle period	Max $B_{\phi}$	$B_{\rm pol}$ / $B_{\rm tor}$
G0.25	0.25	4.65	1.56	0.398
G0.5	0.5	5.42	3.66	0.179
G0.75	0.75	9.37	6.00	0.0889
G1	1	11.7	7.50	0.0555
G1.5	1.5	13.6	9.50	0.0319
G2	2	15.1	11.0	0.0222
G3	3	17.3	14.3	0.0120
G5	5	20.8	20.5	0.00500
G7	7	24.5	26.6	0.00380
G10	10	28.5	34.4	0.00210

Source LaTeX | All tables | In the text

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