  We summarise the X-ray temporal and spectral variability properties of GRBs
as observed using the Swift satellite. Despite much individual complexity, the
flux and spectral variability can be reasonably well described by a combination
of two components - which we denote as the prompt and the afterglow. The first,
prompt component consists of the burst and its initial decay while the second,
afterglow component fits the X-ray plateau phase and subsequent decline
observed in the majority of GRBs. When strong spectral variability occurs it is
associated with the prompt component while the X-ray plateau and later emission
shows little if any spectral variability. We briefly compare the observations
with some of the proposed models. Any model for the early or late emission must
explain the differences in both temporal and spectral behaviour.
