Our observations of the quiet Sun with the NST have yielded unanticipatedresults on smal-scale solar dynamic. Althought small-scale solar dynamic havebeen well-studied, the NST is enabling us to probe finer scale dynamicexploiting higher spatial resolution. We discuss NST resutls from data taken29th July 2009 using an broadband filter centered on TiO 705.7nm spectral line.Data are from the center of the solar disk where we observed quiet Sun. We registered bright-point like structures in most of the intergranularlanes. They vary in behaviour and evolution. Co-registered solar oscillationstend to congregate near certain types of bright-point like structures. Theoscillations with maximum power tend to appear only above or near thesestructures.
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