Investigating the variation of latitudinal stellar spot rotation and its relation to the real stellar surface rotation

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Table 1

Dynamo models.

Name	r _in	C _Ω	C _α	e ₀	e ₁	e _n	period

	[R_⋆]			[B_eq]	[B_eq]	[B_eq]	[years]

L1	0.4	184	20	0.06	0.05	6 × 10^-5	6.8
L2	0.27	250	13	0.12	0.16	0.008	2.7
L2a	0.27	250	13	0.10	0.2	0.04	2.7
L2b	0.27	250	13	0.11	0.15	0.01	2.7

Notes. Name of the model, radius of the inner boundary in stellar radii, dynamo numbers, the distribution of the magnetic energy in different modes, and the cycle period are given.

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