Depletion-related strain and velocity changes will perturb the travel path and length of a normally-incident ray.
The distance
travelled by the ray in time
at velocity
is given by
(1)
For small perturbations
,
and
, we can write
(2)
where,
is the vertical ``depth'' strain and
is the apparent ``time'' strain.
The
-factor (Hatchell and Bourne, 2005a) relates the fractional change in velocity
to the depth strain
and time strain
: