Page 146 - Satellite Communications, Fourth Edition
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126  Chapter Five

                              assuming the earth station to be at mean sea level)

                                                           R cosl cosB                  (5.15a)
                                                      R x
                                                      R   R cosl sinB                   (5.15b)
                                                        y
                                                      R   R sinl                        (5.15c)
                                                        z
                              where B   f   f as defined in Eq. (3.8).
                                         E
                                              SS
                                The local gravity direction is r   R. The coordinates for the direc-
                              tion of propagation k are
                                                        k   R   a GSO                   (5.16a)
                                                              x
                                                         x
                                                        k   R y                         (5.16b)
                                                         y
                                                            R                           (5.16c)
                                                        k z   z
                                Calculation of the polarization angle is illustrated in the following
                              example.

                                Example 5.1 A geostationary satellite is stationed at 105°W and transmits a ver-
                                tically polarized wave. Determine the angle of polarization at an earth station at
                                latitude 18°N longitude 73°W.
                                Solution  Given data:
                                l   18°; f E   73°; f SS   105°; a GSO   42164 km; R   6371 km (spherical earth
                                of mean radius R assumed).
                                Eq. (3.8) gives:
                                                       B   f E   f SS   32°

                                Applying Eq. (5.15), the geocentric-equatorial coordinates for the earth station
                                position vector are:
                                                   R x    R cosl cosB

                                                        6371cos18° cos32°
                                                        5138.48 km

                                                   R y    R cosl sinB
                                                        6371cos18° sin32°

                                                        3210.88 km

                                                   R z    R sinl
                                                        6371sin18°

                                                        1968.75 km
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