Small-scale dynamo in cool stars - III. Changes in the photospheres of F3V to M0V stars

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Table 3

Average values for various quantities related to υ_𝓏 and I_bol.

Simulation	Upflow frac. [%]								Contrast [%]

	SSD	HD	SSD	HD	SSD	HD	SSD	HD	SSD	HD
F3V	57.33	57.14	5.167	5.568	4.653	4.662	1.002	1.026	21.54	22.01
G2V	56.64	56.83	2.518	2.561	2.543	2.535	0.440	0.444	17.30	17.50
K0V	55.38	55.69	1.316	1.335	1.043	1.038	0.120	0.121	11.51	11.65
M0V	60.31	60.05	0.632	0.660	0.425	0.425	0.011	0.011	2.63	2.63

Notes. For each quantity, the left column lists the SSD, and the right column lists HD. The contrast is defined as σ_I/〈I_bol〉. All units are cgs.

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