Fig. 6
From left to right: continuum image stemming from SP data, CaII-H (chromosphere), magnetic field strength map (inversion of SP data done by MERLIN code), G-band (photosphere). The crosses indicate identified MBPs. It can be clearly seen that no significant magnetic field activity is within the FOV (pores, sunspots). The magnetic field strengths in the data set vary between 3 and 1510 G.
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