Page 231 - Satellite Communications, Fourth Edition
P. 231

The Space Segment  211





























                              Figure 7.10  The rectangular box shows the positional
                              limits for a satellite in geostationary orbit in relation to
                              beams from a 30-m and a 5-m antenna.

                              of the box and therefore could miss the satellite. Such narrow-beam
                              antennas therefore must track the satellite.
                                The diameter of the 5-m antenna beam at the satellite will be about
                              464 km, and this does encompass the box, so tracking is not required.
                              The positional uncertainty of the satellite also introduces an uncer-
                              tainty in propagation time, which can be a significant factor in certain
                              types of communications networks.
                                By placing the satellite in an inclined orbit, the north-south station-
                              keeping maneuvers may be dispensed with. The savings in weight
                              achieved by not having to carry fuel for these maneuvers allows the com-
                              munications payload to be increased. The satellite is placed in an
                              inclined orbit of about 2.5° to 3°, in the opposite sense to that produced
                              by drift. Over a period of about half the predicted lifetime of the mis-
                              sion, the orbit will change to equatorial and then continue to increase
                              in inclination. However, this arrangement requires the use of tracking
                              antennas at certain ground stations.


                              7.5 Thermal Control
                              Satellites are subject to large thermal gradients, receiving the sun’s
                              radiation on one side while the other side faces into space. In addition,
                              thermal radiation from the earth and the earth’s albedo, which is the
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