When migrating seismic primary reflections obtained from arbitrary sou
rce-receiver configurations (e.g., common shot or constant offset) int
o depth, a pulse distortion occurs along the reflector. This distortio
n exists even if the migration was performed using the correct velocit
y model. Regardless of the migration algorithm, this distortion is a c
onsequence of varying reflection angle, reflector dip, and/or velocity
variation. The relationship between the original time pulse and the d
epth pulse after migration can be explained and quantified in terms of
a prestack, Kirchhoff-type, diffraction-stack migration theory.