  We relate the underlying properties of a population of fast radio-emitting
transient events to its expected detection rate in a survey of finite
sensitivity. The distribution of the distances of the detected events is
determined in terms of the population luminosity distribution and survey
parameters, for both extragalactic and Galactic populations. The detection rate
as a function of Galactic position is examined to identify regions that
optimize survey efficiency in a survey whose field of view is limited. The
impact of temporal smearing caused by scattering in the Interstellar Medium has
a large and direction-dependent bearing on the detection of impulsive signals,
and we present a model for the effects of scattering on the detection rate. We
show the detection rate scales as Omega S0^{-3/2 + delta}, where Omega is the
field of view, and S0 is the minimum detectable flux density, and 0 < delta =<
3/2 for a survey of Galactic transients in which interstellar scattering or the
finite volume of the Galaxy is important. We derive formal conditions on the
optimal survey strategy to adopt under different circumstances for fast
transients surveys on next generation large-element, widefield arrays, such as
ASKAP, LOFAR, the MWA and the SKA, and show how interstellar scattering and the
finite spatial extent of a Galactic population modify the choice of optimal
strategy.
