  We investigate possible links between the large-scale and small-scale
features of solar wind fluctuations across the frequency break separating fluid
and kinetic regimes. The aim is to correlate the magnetic field fluctuations
polarization at dissipative scales with the particular state of turbulence
within the inertial range of fluctuations. We found clear correlations between
each type of polarization within the kinetic regime and fluid parameters within
the inertial range. Moreover, for the first time in literature, we showed that
left-handed and right-handed polarized fluctuations occupy different areas of
the plasma instabilities-temperature anisotropy plot, as expected for
Alfv$\acute{\textrm{e}}$n Ion Cyclotron and Kinetic Alfv$\acute{\textrm{e}}$n
waves, respectively.
