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Go to start of metadata Follow the evolution of the magnetic flux at different latitudes over the solar cycle (full disk). Follow individual magnetic features flux from lower to high latitudes (high spatial resolution). Determine flow rates (differential rotation, meridional flow) obtained by tracking magnetic features and compare with those determined from tracking granules and from Doppler shifts. How do supergranular flows facilitate or impede the latitudinal transport of small-scale magnetic features? Compare measurements of the magnetic flux from high and low heliographic latitudes (full disk and high resolution). How strongly do (near) Earth-based magnetic field measurements need to be corrected at higher latitudes?