Solar turbulent magnetic fields: Non-LTE modeling of the Hanle effect in the C2 molecule

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Table 1

Parameters for best fits.

Observation	B [G]	ρ_C	ρ_J

Syn. obs.^*	7.41	0.054	1.58
stddev σ	0.76	0.010	0.23
err. of mean σ/	0.09	0.001	0.03

Atlas	9.1 ± 1.5	0.045 ± 0.006	1.2 ± 0.2

ms₀₈₀₅₀₉	8.1 ± 0.8	0.047 ± 0.003	1.4 ± 0.1

Notes.

^(*)

Averages of 78 synoptic measurements with 0.07 < μ < 0.13, their standard deviations σ and their errors of the mean. To obtain errors of the mean, the standard deviations are divided by , assuming a normal distribution of the errors.

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