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4.2.1.1 Study the shape and morphology of solar high-latitude magnetic field structures as well as their relation to the flow fields.

4.2.1.2 Study the distribution of field strengths (and magnetic vectors) of solar high-latitude magnetic field structures.

4.2.1.3 Compare the results from the above objective (4.2.1.2) with the field strength distribution of sunspots and active regions.