Large-scale galactic magnetic fields are probably caused by some magne
tic field amplification mechanism starting from a seed field. The's se
ed field is still enigmatic. In this contribution it is shown that mac
roscopic sheared relative velocities of the charged and neutral compon
ents of a protogalactic partially ionized plasma generate magnetic fie
lds during the protogalactic collapse. Plasma-neutral gas fluid simula
tions are performed in order to illustrate this magnetic field-self ge
neration mechanism.