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a Matlab package for phased array beam shape inspection

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4.9 The power integral <strong>for</strong> an <strong>array</strong> with directional elements 21<br />

4.9. The power integral <strong>for</strong> an <strong>array</strong> with directional elements<br />

When the element gain G E depends on direction, the power integral cannot in general<br />

evaluated in a closed <strong>for</strong>m. However, <strong>for</strong> <strong>array</strong>s with reasonably large number of elements<br />

both in the x- and y-directions, an approximation can be found as follows. For such an<br />

<strong>array</strong>, the <strong>array</strong> factor resembles a sum of delta functions, that is, AF has narrow <strong>beam</strong>s<br />

around the widely separated grating directions, and pretty much zero elsewhere. Denoting<br />

by ∆Ω g the solid angle around the grating direction u g that contain the essential<br />

part of the AF in that direction, we write the power integral as the sum of integrals over<br />

the support regions,<br />

∫<br />

4π · PI = G E |AF| 2 dΩ ≈ ∑ ∫<br />

G E |AF| 2 dΩ . (65)<br />

4π g ∆Ω g<br />

We assume that the element gain is wide compared to the size ∆Ω g , so that we can take<br />

G E to be constant in that region, and take it out of the integral, and use Eq. (42) to<br />

replace AF by the 2-D Fourier trans<strong>for</strong>m of the excitation amplitude-sequence,<br />

4π · PI ≈ ∑ ∫<br />

G E (u g ) |ã((u − u 0 )D)| 2 dΩ(û) . (66)<br />

g<br />

∆Ω g<br />

The differential surface element, on the surface of unit sphere, corresponding the solid<br />

angle dΩ, is equal of the size of the projection d 2 u to xy-plane of that surface element,<br />

divided by the cosine of the polar angle θ g of û at the element,<br />

dS g (û) =<br />

d2 u<br />

cos θ g<br />

. (67)<br />

This corresponds to change of variables from the spherical coordinates on the surface of<br />

the sphere to the cartesian coordinates on the xy-plane. The precise boundary of the<br />

area of integration does not matter, as it anyway is assumed to be in the 0-region of the<br />

integrand. We make the substitution Eq. (67) to Eq. (66). Then we also expand the<br />

area of integration to cover the whole grating zone Z g hosting the direction u g ; this just<br />

adds some more 0-region to the area, <strong>for</strong> there is at most one grating <strong>beam</strong> in a grating<br />

zone. The power integral becomes<br />

4π · PI = ∑ g<br />

G E (u g )<br />

cos θ g<br />

∫<br />

Z g<br />

|ã((u − u 0 )D)| 2 d 2 u . (68)<br />

Finally, we use Parseval’s theorem <strong>for</strong> 2-D sequencies, Eq. (56), to get<br />

( )<br />

∑<br />

∑<br />

G E (u g ) 1 |am | 2<br />

PI =<br />

. (69)<br />

cos θ<br />

g g D x D y 4π<br />

4.10. Array gain <strong>for</strong> an <strong>array</strong> with directional elements<br />

Consider an <strong>array</strong> with the excitation amplitudes all unity, and directional elements with<br />

power gain G E . From Eq. (50), Eq. (58) and Eq. (69), the absolutely normalized gain is<br />

G(û) = G E(û)(M x M y ) 2 [diric()diric()] 2 4πD x D y<br />

M x M y<br />

∑g<br />

=<br />

G E (û)<br />

∑ G E (u g)<br />

g cos θ g<br />

G E (u g)<br />

cos θ g<br />

4πA<br />

λ 2 · [diric()diric()] 2 , (70)

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