Fig. 8
Magnetic field strength distribution of the identified MBP features in the quiet solar FOV of the high spatial resolution data set (data set IV). The reduced χ2 for the fit is 4.4. The component related to MBPs is fitted at (1110 ·| ÷ 1.14) G. For this data set, 2614 identified MBP features were analysed, which covered about 1.4% of the total FOV.
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