Assume a cold, unmagnetized, weakly collisional plasma, a small fractional bandwidth and ω≫ωp. The dispersion relation is ω2=c2k2+ωp2, with ωp2=nee2/(ϵ0me). The group velocity and propagation time areThe lower frequencies arrive later. Taking the magnitude of the frequency derivative over Δω givesFor a nonuniform line of sight, replace neL by the dispersion measure ∫nedl. The light travels at the group velocity, not at the phase velocity.
vg=dkdω=c1−ω2ωp2,τ(ω)=cL(1−ω2ωp2)−1/2≃cL(1+2ω2ωp2).
Δτ≃cω3LΔωϵ0menee2.
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