We have made detailed investigations on spiral growth of c-facets in h
elium crystals with dislocation densities similar to 10 cm(-2). Our re
sults at high temperatures T = 100 - 200 mK agree quite well with the
classical parabolic power law for spiral growth, whereas a linear depe
ndence on the driving pressure is observed at 2 - 20 mK. This is a con
sequence of the inertia of elementary steps in the situation when damp
ing due to phonons is small. At high velocities, all our data display
a tendency to saturation which is interpreted as an indication of step
localization at large driving forces.