  We propose a reflection model of the time delays detected during an
exceptionally bright, single flare in MCG-6-30-15. We consider a scenario in
which the delays of the hard X-rays with respect to the soft X-rays are caused
by the presence of the delayed reflection component. We employ a model of the
flare, which is accompanied by reprocessed emission. We consider two
geometries/thermal states of the reprocessing medium: a partially ionized
accretion disk surface and a distribution of magnetically confined, cold blobs.
The reprocessing by cold blobs predicts positive time delays and a saturation
in the time delay -- energy relation, which is likely present in the data. The
model requires a strong reflection component and relies on the apparent
pivoting of the combined primary and reflected spectrum. The reflection by the
ionized disk surface does not reproduce the observed delays. We discuss the
relation between the two reflection scenarios and argue that they are both
present in MCG-6-30-15.
