Page 400 - Electromagnetics
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Other important relationships include the orthogonality of the longitudinal fields,

                                                        ˇ
                                                    ˇ
                                                    E zm E zn dS = 0,  m 
= n,                (5.149)
                                                  CS

                                                        ˇ
                                                    ˇ
                                                    H zm H zn dS = 0,  m 
= n,                (5.150)
                                                 CS
                        and the orthogonality of transverse fields,

                                                        ˇ
                                                    ˇ
                                                    E tm · E tn dS = 0,  m 
= n,
                                                 CS

                                                    ˇ
                                                        ˇ
                                                   H tm · H tn dS = 0,  m 
= n.
                                                 CS
                        These may also be combined to give an orthogonality relation for the complete fields:

                                                        ˇ
                                                    ˇ
                                                    E m · E n dS = 0,  m 
= n,                (5.151)
                                                  CS

                                                        ˇ
                                                    ˇ
                                                    H m · H n dS = 0,  m 
= n.                (5.152)
                                                 CS
                        For proofs of these relations the reader should see Collin [39].
                        Power carried by time-harmonic waves in lossless waveguides. The power car-
                        ried by a time-harmonic wave propagating down a waveguide is defined as the time-
                        average Poynting flux passing through the guide cross-section. Thus we may write
                                                      1
                                                               ˇ
                                                                   ˇ ∗
                                                 P av =    Re E × H   · ˆ z dS.
                                                      2  CS
                        The field within the guide is assumed to be a superposition of all possible waveguide
                        modes. For waves traveling in the +z-direction this implies
                                     ˇ  "              − jk zm z  ˇ  "   ˇ     ˇ  	  − jk zn z
                                    E =    (ˇ e tm + ˆ zˇ e zm ) e  ,  H =  h tn + ˆ zh zn e  .
                                         m                            n
                        Substituting we have
                                             #                                        $
                                    1         "              − jk zm z  "       	  jk zn z
                                                                                    ∗
                                                                        ˇ ∗
                               P av =  Re         (ˇ e tm + ˆ zˇ e zm ) e  ×  h + ˆ zh ˇ ∗ zn  e  · ˆ z dS
                                                                         tn
                                    2      CS  m                     n

                                    1     " "    − j(k zm −k zn )z
                                                       ∗
                                                                      ˇ ∗
                                  =   Re        e            ˆ z · ˇ e tm × h tn  dS .
                                    2                      CS
                                           m  n
                        By (5.148) we have

                                              1     "   − j(k zn −k zn )z
                                                              ∗
                                        P av =  Re     e            ˆ z · ˇ e tn × h ˇ ∗ tn  dS .
                                              2                  CS
                                                     n
                        For modes propagating in a lossless guide k zn = β zn . For modes that are cut off k zn =
                        − jα zn . However, we find below that terms in this series representing modes that are cut
                        off are zero. Thus
                                                 1
                                              "                     	       "
                                                                  ˇ ∗
                                         P av =    Re     ˆ z · ˇ e tn × h tn  dS =  P n,av .
                                                 2
                                               n        CS                   n
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