Abstract
When monochromatic electromagnetic waves with electric and magnetic vectors* E
i
, H
i
are incident on a perfectly reflecting screen
S
, the waves are scattered at the surface of the screen. The problem of reflexion and diffraction consists in determining the scattered field E
s
, H
s
, which satisfies the following conditions: (i) it is a solution of Maxwell’s equations
i
k
E = curl H,
i
k
H = — curl E, div E = 0, div H = 0; (ii) on
S
, (E
i
+ E
s
) x N = 0, (H
i
+ H
s
). N = 0, where N is the outward normal unit vector to
S
; (iii) it satisfies Sommerfeld's radiation condition at infinity. There is only one field E
s
, H
s
which satisfies these conditions. The simplest form of the radiation condition is to assume that
k
=
p
—
iq
, where
p
and
q
are positive and
q
is small, and to require each field component to vanish at infinity. This corresponds physically to assuming that the medium has a small conductivity. The imaginary part of
k
can be made zero at the end of the analysis. It is important to note that a field which satisfies the radiation condition and which has no singularity anywhere in space is null.
Reference7 articles.
1. H uygens;Copson;Principle,1939
2. Theory of Diffraction by Small Holes
3. Copson 1945 Quart. J . M ath (in th e Press).
4. Magnus 1941 Z . P hys. 117 168-179.
5. R ayleigh 1896 Theory of Sound 2 107 and 109. London.
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