A Plane Wave Expansion Theorem for Cylindrically Radiated Fields

Cover A Plane Wave Expansion Theorem for Cylindrically Radiated Fields
A Plane Wave Expansion Theorem for Cylindrically Radiated Fields
Samuel Karp
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In this respect again our result differs from the more usual expansion theorem, which proceeds in inverse powers of r.
h. It is convenient to bear in mind that the functions v"- ^ (O) really contain the new coordinates x and y. For example , ^, ik(x cos6 + y sinS) v(Oj = e . J I-/ -11- 5.
v(0) = e vW (0) ikx ikye ikx _ dv(p)| ^^ P=0 / vl2J(0) = ik[-x + iky^J 2t ikx d V e = — dp 3=0.
, etc.
A), Consider for example the expanGion of the function H (kr).
We have i(kr4)" nf ^(^^ - J^ ^ 1+ 0(i) r r—
... > 00 Hence f(0) h 1, f (e) = - . Applying (2a) we find l(M-f) ikx e + Jiik[-x-Hky]e ^.
2_ i(^ jtkd ^ v(0) + |rj^^ (y(0) + W'-2J(o)) + Uv^^^fO)) + We shall now explain, in brief, how the expansion theorem may be employed in calciilating the diffraction of an arbitrary radiating field.
In such a calculation the function f (S) for the incident radiation will be known. The incident radiation will then be represented in the form (2a), in a coordinate system x, y fixed in the neighborhood of the scatterer.


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