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The Method of Moments in Electromagnetics

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A Brief Review <strong>of</strong> <strong>Electromagnetics</strong> 17½Ö ¾ ½Ö ¿ etc., because <strong>of</strong> the differential operators. In the far field we expect thatonly those fields vary<strong>in</strong>g accord<strong>in</strong>g to ½Ö will have significant amplitude. <strong>The</strong>secomponents behave like a plane wave with no components along the direction <strong>of</strong>propagation. <strong>The</strong> far electric field will therefore be computed asand the magnetic field obta<strong>in</strong>ed from the electric field asE´rµ A´rµ (2.99)H´rµ ½ r ¢ E´rµ (2.100)where we have assumed the field to be a plane wave propagat<strong>in</strong>g along the vector r.2.5.2.1 Three-Dimensional Far FieldWe can write the expression for the far-zone electric field by us<strong>in</strong>g (2.98) with (2.99),result<strong>in</strong>g <strong>in</strong> the well-known expressionE´rµ Ö ÖÎJ´r ¼ µ r¼ ¡r r ¼ (2.101)For scatter<strong>in</strong>g problems with an <strong>in</strong>cident field E and scattered far field E × , the threedimensionalradar cross section ¿ is def<strong>in</strong>ed as [1] ¿ Ö ¾ E× ¾E ¾ Ö¾ E × ¾ (2.102)where it is usually assumed that E ½for computational convenience.2.5.2.2 Two-Dimensional Far FieldIn two dimensions the radiated far electric field is given byE´µ A´µ J´ ¼ µÀ ´¾µ¼ ´ ¼ µ ¼ (2.103)Us<strong>in</strong>g the large-argument approximation <strong>of</strong> the Hankel function [4]×À Ò ´¾µ ´µ ¾ Ò ½ (2.104)and (2.98) we write×¾¼ ´µ ¼ ¡À ´¾µ(2.105)

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