We investigate the nonlinear development of ideal kink instabilities i
n a line-tied coronal loop, using a three dimensional numerical code.
In order to understand how the equilibrium loop properties affect nonl
inear evolution, various different initial magnetic equilibria are con
sidered. In most cases, a fine-scale magnetic field structure is shown
to develop. However, the corresponding electric current structure dep
ends sensitively on the initial equilibrium: the initial magnetic twis
t profile, the loop length, and the nature of the outer potential regi
on. If there are resonant regions at the loop apex where the radial co
mponent of the linear perturbed magnetic field vanishes, a current con
centration develops there in the subsequent non linear phase. Otherwis
e current concentrations may develop as a consequence of the effect of
line-tying. The ensuing resistive evolution of the system and the imp
act on coronal activity are discussed.