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Movement and coalescence of magnetic elements could explain the evolution andgrowth of pores. There have been numerous studies focusing on flow fields inand around individual pores. We have undertaken a systematic study of thestatistical properties of such flows. Data of the Hinode Solar OpticalTelescope offer an opportunity for this type of research, because of theuniform data quality and absence of seeing so that pores can directly becompared in different environments and at various stages of their evolution. Weanalyzed about 220 time-series of G-band images using local correlationtracking. The thus computed flow maps make up a database, which covers variousscenes on the solar surface. We use an isolated pore to illustrate thestatistical parameters collected for further statistical analysis, whichinclude information about morphology, horizontal flows, evolutionary stage(young, mature, or decaying), complexity of the surrounding magnetic field, andproximity to sunspots or cluster of G-band bright points.

Statistical characteristics of horizontal proper motions in the vicinity of pores