The horseshoe vortex system is a series of vortices which develop at the junction between an endwall and a bluff body during impinging flow. Pin-fin arrays are an internal cooling feature where bluff-bodies are arranged in an array to act as turbulators and increase heat transfer to a cooling fluid. The present study examines how the horseshoe vortex system evolves at pin-fins of different row positions in a low aspect ratio pin-fin array. Time-resolved stereo particle image velocimetry was employed in the stagnation plane of pin-fins in rows 1, 3, and 5 for a Reynolds number, based on pin-fin diameter, of 2.0e4. The shape of the timemean horseshoe vortex profile was found to change from row 1 to row 3 due to upstream flow acceleration and buffeting by turbulence. The bimodal nature of the horseshoe vortex was established regardless of row number, and the oscillation between the backflow and zero-flow modes was shown to drive regions of maximum ' ' ̅̅̅̅̅ and ' ' ̅̅̅̅̅. ' ' ̅̅̅̅̅̅ was found to be dominated by upstream wake shedding instead of horseshoe vortex effects. Turbulent kinetic energy in the horseshoe vortex region was found to be amplified above mid-channel levels for each row. The shape of turbulent kinetic energy in this region was found to vary with row location due to the changing influences of ' ' ̅̅̅̅̅ , ' ' ̅̅̅̅̅ , and ' ' ̅̅̅̅̅̅. Finally, the backflow was discovered to have strong, negative values of ' ' ̅̅̅̅̅ , while the region closer to the pin on the opposite side of the spiral node contained strong, positive values of ' ' ̅̅̅̅̅ .