Page 71 - ITU Journal: Volume 2, No. 1 - Special issue - Propagation modelling for advanced future radio systems - Challenges for a congested radio spectrum
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ITU Journal: ICT Discoveries, Vol. 2(1), December 2019



          In  the  above,     (   )  is  the  Fresnel  reflection   Furthermore, the     in Equation (12) are the SPM
                                                                                     
                                
                              
          coefficient for    polarization as defined by:       polarization factors with
                                           2                                     (      −1)
                        (   ) =               − √      −             ,          ℎℎ  =  2      2   cos(   −    ),
                                                                                                         
                                                                                                             
                            
                      ℎℎ
                                           2
                                           + √      −                (cos       +√      −sin       )(cos       +√      −sin       )
                                                                                        2
          and                                                       ℎ  =     −(      −1)√      −sin        sin(   −    ),
                                                                                                          
                                                                                                               
                                                                                                2
                                                                                  2
                                                                     (      cos       +√      −sin       )(cos       +√      −sin       )
                                            2
                       (   ) =                      − √      −              .   (10)   (      −1)√      −            
                                                                                        2
                           
                         
                                            2
                                                + √      −                 ℎ    =   2           2   sin(   −    ),
                                                                                                               
                                                                                                          
                                                                     (cos       +√      −sin       )(      cos       +√      −sin       )
          Moreover,    (   −    )  and            are  the  Dirac  and   and
                              
                         
          Kronecker delta functions respectively:
                                                                                                2
                                                                                        2
                                                                     (      −1)(      sin       sin        −√      −sin         √       −sin        cos(      −      ) )
                             1,             =                                                              . (14)
                 (   −    ) = {                     (10a)              =                           2
                     
                         
                                                                                     2
                             0,          ℎ                               (      cos       +√      −sin       )(      cos       + √       −sin       )
           and                                                 For  Gaussian correlation  functions,  Equation  (12)
                                                               reduces to:
                         1,                   =   
                                                                                                        2
                           = {                      (10b)                     2            2    2              ℓ 2 }. (15)
                                                                                          )
                         0,          ℎ                                 (   ̂ ,    ̂ ) = (2     ℓ cos       cos        |        | exp {−  4
                                                                         
                                                                       
          Analytical  expressions  for  the  diffuse  bi-static   Fig.  2  depicts  the  value  for  the  backscattering
          scattering  coefficient  components  are  provided   coefficient based on SPM, Equation (15).
          below,  based  on  the  three  different  models  with
          values  of  cross-polarized  bi-static  scattering
          coefficients
                           
                                            
                         ℎ  (   ,    ), and    ℎ    (   ,    )
                                         ̂ ̂
                         ̂ ̂
                                             
                               
                            
                                               
          within the plane of incidence based on each model.
          3.     DIFFUSE BI-STATIC COEFFICIENT
                 BASED ON THE SMALL
                 PERTURBATION METHOD (SPM)
          The small  perturbation method  (SPM) applies for
          slightly  rough  surfaces  having  variance  and
          correlation length governed by equations (35) and
          (36) defined in [4]. Those equations are recalled as
          Equation (11).
                                                                   Fig. 2 – Vertically backscattering coefficient (ε_r=20)
                              < 0.3 ,          
                                                                 Case (1): kσ=0.1, kl=1.0, Case (2): kσ=0.2, kl=2.0, Case (3):
                             ℓ >  4.71     .         (11)                         kσ=0.3, kl=3.0
                                                               In  order  to  examine  values  of  cross-polarized
          The   diffuse   bi-static   scattering   coefficient   backscattering coefficients in the plane of incidence
                  ̂ ̂
                   (   ,    )  based  on  SPM  can  be  written  as   set
                   
                     
          (Equation (22) of [5], (21-67) of [6], (31) of [4], and              −    = 0 ,           ±    .   (16)
          (37) of [7])                                                              
                                             2
                    ̂ ̂
                                        2
                            2
                     (   ,    ) = 8 (   cos    cos    ) |   |    (   ). (12)   Then  introduce  Equation  (16)  into  Equation  (14)
                                               
                    
                                         
                      
                                                       
                                   
                                                               and the resultant into Equation (12) yielding null
          where   (   ) is the surface height spectral density   values  for  the  cross-polarized  bi-static  scattering
                        
          function  of  Equation  (4)  calculated  at  roughness   coefficients  within  the  plane  of  incidence.  Those
          wavenumber    equal to    .                          null  values  indicate  that  SPM  is  not  capable  of
                                      
                                                               predicting  the  cross-polarized  bi-static  scattering
                     2       2                       ) (13)
                    =    √sin       + sin       − 2 sin       sin       cos(      −        coefficients within the plane of incidence.

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