  The partial ionization of the solar plasma causes several nonideal effects
such as the ambipolar diffusion, the Hall effect, and the Biermann battery
effect. Here we report on the first three-dimensional realistic simulations of
solar local dynamo where all three effects were taken into account. The
simulations started with a snapshot of already saturated battery-seeded dynamo,
where two new series were developed: one with solely ambipolar diffusion and
another one also taking into account the Hall term in the generalized Ohm's
law. The simulations were then run for about 4 hours of solar time to reach the
stationary regime and improve the statistics. In parallel, a purely MHD dynamo
simulation was also run for the same amount of time. The simulations are
compared in a statistical way. The results show that, with the inclusion of the
ambipolar diffusion, the amplitudes of the incompressible perturbations related
to Alfven waves are reduced, and the Poynting flux is absorbed, with a
frequency dependence. The Hall effect causes the opposite action: significant
excess of incompressible perturbations is generated and an excess of the
Poynting flux is observed in the chromospheric layers. The model with ambipolar
diffusion shows, on average, sharper current sheets and slightly more abundant
fast magneto-acoustic shocks in the chromosphere. The model with the Hall
effect has higher temperatures at the lower chromosphere and stronger and more
vertical magnetic field concentrations all over the chromosphere. The study of
high-frequency waves reveals that significant power of incompressible
perturbations is associated with areas with intense and more vertical magnetic
fields and larger temperatures. We find a positive correlation between the
magnitude of the ambipolar heating and the temperature increase at the same
location after a characteristic time of 10^2 sec.
