  We used photospheric intensity images and magnetic field measurements from
the New Solar Telescope in Big Bear and Helioseismic Magnetic Imager on board
Solar Dynamics Observatory (SDO) to study the the effect that the new
small-scale emerging flux induces on solar granulation. We report that emerging
flux appears to leave different types of footprint on solar granulation: i)
diffuse irregular patches of increased brightness, ii) well defined
filament-like structures and accompanied bright points, and iii) bright
point-like features that appear inside granules. We suggest that the type of
the footprint depends on the intensity of emerging fields. Stronger fields,
emerging as a part of large magnetic structure, create on the solar surface a
well defined filamentary pattern with bright points at the ends of the
filaments, while weak turbulent fields are associated with bright patches
inside the host granule.
