Table 4: Fraction of irregular Stokes V profiles of the Fe I 15 648 and 6302 Å lines with reduced resolution as a function of $\langle B\rangle$ . Only the profiles with amplitudes 3 times above the noise of $3 \times 10^{-4} I_{\rm c}$ are considered. The last two columns give the fraction of profiles above the threshold in the infrared and the visible.
$\langle B\rangle$ [G] Fe I 15 648 Fe I 6302 N_15 648 N₆₃₀₂

10 22% 21% 36% 31%

20 29% 30% 64% 54%

30 26% 29% 86% 88%

80 19% 28% 99% 100%

140 16% 17% 100% 100%

**Table 4:** Fraction of irregular Stokes V profiles of the Fe I 15 648 and 6302 Å lines with reduced resolution as a function of $\langle B\rangle$ . Only the profiles with amplitudes 3 times above the noise of $3 \times 10^{-4} I_{\rm c}$ are considered. The last two columns give the fraction of profiles above the threshold in the infrared and the visible.
$\langle B\rangle$ [G]	Fe I 15 648	Fe I 6302	N_15 648	N₆₃₀₂
10	22%	21%	36%	31%
20	29%	30%	64%	54%
30	26%	29%	86%	88%
80	19%	28%	99%	100%
140	16%	17%	100%	100%

Source LaTeX | All tables | In the text

	1 Introduction
	2 Radiative MHD simulations
	3 Spectral synthesis
	4 Classification of Stokes V profiles
	5 Amplitudes of Stokes V
	6 Asymmetries
	7 Zero-crossing velocity
	8 Comparison of IR and visible data
	9 Discussion and conclusions
	References