  In this work we follow a series of papers on high-resolution observations of
small-scale structures in the solar atmosphere \citep[][Cabello et al., in
prep]{Balmaceda2009, Balmaceda2010, Vargas2011, Palacios2012, Domingo2012,
Vargas2015}, combining several multi-wavelength data series. These were
acquired by both ground-based (SST) and space-borne (Hinode) instruments during
the joint campaign of the Hinode Operation Program 14, in September 2007.
Diffraction-limited SST data were taken in the G-band and G-cont, and were
restored by the MFBD technique. Hinode instruments, on the other hand, provided
multispectral data from SOT-FG in the CN band, and Mg~{\sc I} and Ca {\sc
II}~lines, as well as from SOT-SP in the Fe~{\sc I} line. In this series of
works we have thoroughly studied vortex flows and their statistical
occurrences, horizontal velocity fields by means of Local Correlation Tracking
(LCT), divergence and vorticity. Taking advantage of the high-cadence and high
spatial resolution data, we have also studied bright point statistics and
magnetic field intensification, highlighting the importance of the
smallest-scale magnetic element observations.
