The dynamics of thin current sheets takes on special importance in stu
dying the processes occurring in both laboratory and astrophysical pla
smas. In this paper, the dynamics of current filamentation is consider
ed using a dynamic model that was first proposed by B. A. Trubnikov in
order to study the initiation of pinches in the interaction of magnet
ized plasma clouds. It is shown that this dynamic system is Hamiltonia
n, and collapse resulting in the formation of individual current filam
ents that each carry a finite current inevitably occurs in this system
. Self-similar solutions are obtained describing the collapse of an in
dividual current filament both in the ''self-compression'' regime and
with allowance for the influence of the remaining current filaments.