  The analysis of the Parker-Moffatt problem, recently revisited in Pezzi et
al. (2016), is here extended by including the Hall magnetohydrodynamics and two
hybrid kinetic Vlasov-Maxwell numerical models. The presence of dispersive and
kinetic features is studied in detail and a comparison between the two kinetic
codes is also reported. Focus on the presence of non-Maxwellian signatures
shows that - during the collision - regions characterized by strong temperature
anisotropy are recovered and the proton distribution function displays a beam
along the direction of the magnetic field, similar to some recent observations
of the solar wind.
