Page 108 - Antennas for Base Stations in Wireless Communications
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Base Station Antennas for Mobile Radio Systems        81

                  an azimuth-over-elevation mount for the AUT or a high mounting loca-
                  tion for the AUT with the illuminating antenna at a lower elevation. For
                  slant-polar antennas, the AUT must be illuminated in turn with plane
                  waves polarized at ±45°.
                    Some facilities are equipped with very large anechoic chambers, but if
                  valid far-field measurements are to be obtained, their use requires the
                  application of correction techniques. These may include the installation
                  of movable or multiple source antennas and the recording of complex
                  field values for later computation. Such systems can be considered as a
                  class of very large near-field ranges.
                    Far-field measurements are fast to perform, and data for a large
                  number of frequencies can be gathered in a single rotation of the AUT.
                  It is also easy to conduct a swept gain/frequency measurement that
                  provides confidence that there are no frequencies at which the gain of
                  the antenna is unexpectedly lower than elsewhere. The main drawbacks
                  are the need for land for the facility, the cost of handling antennas, and
                  problems caused by inclement weather.
                    When measuring the radiation patterns of a dual-polar array, it is
                  important to appreciate that the radiation in the forward direction has
                  the opposite polarization sense to that of the rearward radiation (seen
                  from behind, the radiating element appears to have a mirror image ori-
                  entation compared with when it is seen from the front). This means that
                  to assess the F/b ratio, we must compare the forward radiation of one
                  polarization with the maximum rearward radiation of the other polar-
                  ization (or both of them to be certain of capturing the largest value).
                  Sometimes a total rearward power is computed by adding both polariza-
                  tion contributions power-wise.
                    Near-field measurements are usually carried out in a screened anechoic
                  chamber; they have the advantage of ease of accessibility and use and
                  being unaffected by weather conditions. The field radiated by the AUT
                  is probed by a small horn or open-ended waveguide. Because the main
                  area of interest in the radiation pattern of a BS antenna is within a
                  few degrees of the horizontal plane, a cylindrical near-field system can
                  be used rather than a full three-dimensional system—although high-
                  angle grating lobes will not be seen. The main constraint of a near-field
                  system is that gain measurements are only available at those frequen-
                  cies at which a pattern measurement is made, so no frequency-swept
                  gain measurement is possible.
                    Some  near-field  ranges  are  provided  with  multiple  illuminating
                  horns, allowing electronic switching of the source antenna rather than
                  much slower physical manipulation. A system of this type provides fast
                  measurements allowing more frequencies to be measured in a given
                  time, but the security of a continuous gain/frequency measurement is
                  still missing.
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