  Time variable delays due to radio wave propagation in the ionized
interstellar medium are a substantial source of error in pulsar timing array
efforts. We describe the physical origin of these effects, discussing
dispersive and scattering effects separately. Where possible, we give estimates
of the magnitude of timing errors produced by these effects and their scaling
with radio frequency. Although there is general understanding of the
interstellar medium propagation errors to be expected with pulsar timing array
observations, detailed comparison between theory and practice is still in its
infancy, particularly with regard to scattering effects.
