The problem of dipole radiation in sinusoidally spacetime periodic media is studied and solved. The space-time periodicity can be considered as due to a strong pump wave and is expressed as a traveling-wave type change in the dielectric constant or the plasma density (i.e.,
![\\epsilon(z,t) = \\epsilon_{0}\\epsilon_{r}[1 + \\epsilon_{1} \\cos (Kz - \\Omega t)]](/images/tex/13350.gif)
and
![N(z,t) = N_{0}[1 + N_{1} \\cos (Kz - \\Omega t)])](/images/tex/13351.gif)
. The solution also covers the limit case of a sinusoidally stratified medium (

). The solution is formulated in a matrix form, such that the basic results and diagrams apply, with minor changes, to the different cases studied: electric and magnetic dipole in a dielectric, plasma, and uniaxial plasma. The wave-vector diagram is used extensively in studying and presenting the different properties of the solution: caustics, effect of the disturbance (pump wave) motion, harmonics, radiation outside the allowed cone in a uniaxial plasma. Many dipole radiation patterns are given and their features explained physically. Finally, our solution and results are extended to the generally space-time periodic media where

and

behave as
![\\eta(z,t) = \\eta_{0}[1 + \\eta_{1}f(Kz - \\Omega t)]](/images/tex/13355.gif)
where

is any periodic function.