In a 3D treatment of the inverse Gertsenshtein effect, an isotropic unpolarized gravitational wave background scattering off a dipolar magnetic field yields partially linearly polarized radio emission, with peak intensity at the dipole equator.
Gertsenshtein, Wave Resonance of Light and Gravitational Waves , Sov
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Gravitational Wave Scattering on Magnetic Fields
In a 3D treatment of the inverse Gertsenshtein effect, an isotropic unpolarized gravitational wave background scattering off a dipolar magnetic field yields partially linearly polarized radio emission, with peak intensity at the dipole equator.