Analysis of unresolved photospheric magnetic field structure using Fe I 6301 and 6302 lines
Analysis of unresolved photospheric magnetic field structure using Fe I 6301 and 6302 lines
Early magnetographic observations indicated that magnetic field in the solar photosphere has unresolved small-scale structure. Near-infrared and optical data with extremely high spatial resolution show that these structures have scales of few tens of kilometres, which are not resolved in the majority of solar observations. The goal of this study …