Using our newly developed high-resolution ring analysis (HRRA) technique we measure subsurface flows within and surrounding magnetic active regions. With this procedure we are capable of measuring flows with a horizontal spatial resolution of 2° in heliographic angle (or roughly 20 Mm). Using MDI magnetograms, we define contours of equal magnetic field strength for all active regions that appear within 60° of disk center between 29 March - 24 April 2002. Using the flow fields computed with our HRRA procedure, we compute the average curl, divergence and inflow speed inside each of these contours, and characterize these mean flow properties as a function of magnetic field strength. We find that on average all active regions possess a mean inflow near the periphery of the region (weak field) and an outflow within the core of the active region (strong field) that is predominantly the result of the well-known sunspot outflows [1]. The mean divergence is consistent with these inflow results (net divergence in the core and convergence in the periphery). We find no evidence for a mean curl that is different from zero.
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