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78   Chapter Three

                              The period P for the geostationary is 23 h, 56 min, 4 s mean solar time
                              (ordinary clock time). This is the time taken for the earth to complete
                              one revolution about its N–S axis, measured relative to the fixed stars
                              (see Sec. 2.9.4). Substituting this value along with the value for   given
                              by Eq. (2.3) results in

                                                            42164 km                      (3.2)
                                                      a GSO
                              The equatorial radius of the earth, to the nearest kilometer, is

                                                        a   6378 km                       (3.3)
                                                         E
                              and hence the geostationary height is

                                                     h GSO    a GSO    a E
                                                                42164   6378              (3.4)
                                                               35786 km

                              This value is often rounded up to 36,000 km for approximate calculations.
                                In practice, a precise geostationary orbit cannot be attained because
                              of disturbance forces in space and the effects of the earth’s equatorial
                              bulge. The gravitational fields of the sun and the moon produce a shift
                              of about 0.85°/year in inclination. Also, the earth’s equatorial ellipticity
                              causes the satellite to drift eastward along the orbit. In practice, station-
                              keeping maneuvers have to be performed periodically to correct for
                              these shifts, as described in Sec. 7.4.
                                An important point to grasp is that there is only one geostationary
                              orbit because there is only one value of a that satisfies Eq. (2.3) for a
                              periodic time of 23 h, 56 min, 4 s. Communications authorities
                              throughout the world regard the geostationary orbit as a natural
                              resource, and its use is carefully regulated through national and inter-
                              national agreements.



                              3.2 Antenna Look Angles
                              The look angles for the ground station antenna are the azimuth and ele-
                              vation angles required at the antenna so that it points directly at the
                              satellite. In Sec. 2.9.8 the look angles were determined in the general
                              case of an elliptical orbit, and there the angles had to change in order
                              to track the satellite. With the geostationary orbit, the situation is much
                              simpler because the satellite is stationary with respect to the earth.
                              Although in general no tracking should be necessary, with the large earth
                              stations used for commercial communications, the antenna beamwidth
                              is very narrow (see Chap. 6), and a tracking mechanism is required
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