Use time dependence , positive wavenumber and aperture normal . Write on the aperture and extend by zero outside it. DefineThe outgoing branch has for propagating components and for evanescent components.
Fix the Green function normalization by , so . Its transverse Fourier transform satisfies . An outgoing solution on both sides is proportional to , and its derivative jump fixes . Thus the Weyl plane-wave representation for observation at isSince , the given aperture integral becomes a superposition of curls of . Each curl supplies . Therefore, with the unit prefactor in that integral,Every vector amplitude is transverse to , as Maxwell's equations require. The polarizer specifies the incident aperture field; diffraction can regenerate an component outside the aperture. In contrast, its component remains zero in this representation. Evanescent plane waves are needed for the complete near field, not just the propagating disk .
The factor follows explicitly from the standard outgoing Green function for the three-dimensional Helmholtz equation and the printed unit curl prefactor. If the intended kernel is the doubled half-space kernel , or the aperture formula carries the usual compensating factor , delete that . The latter normalization makes the tangential output trace equal to . Keeping the convention explicit avoids silently changing the supplied representation; the angular dependence and transversality of an electromagnetic plane wave are the same in either normalization. Reversing the specified normal also reverses the overall sign.
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