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Modulation



                                                                                    Modulation 89

                        3. Set the analyzer’s SPAN to 1.25 times the signal’s  30 dB bandwidth.
                        4. Decrease the analyzer’s video bandwidth (VBW) setting to reduce the sig-
                           nal’s displayed noise.
                        5. Take the digital signal’s power measurement with the spectrum analyzer’s
                           frequency/amplitude MARKER placed at the center of the signal.
                        6. Now, find the true total average power of the digital signal by taking the
                           power in dBm (as measured in step 5), and adding a bandwidth correction
                           factor (BWCF):

                                                               signal BW 30 dB
                                             BWCF   10 log
                                                                 RBW
                             To find the true digital output power of the signal, calculate total digital
                           signal power (dBm)   measured power in dBm (from step 5)   BWCF
                        7. For a more accurate digital signal power measurement you can add another
                           correction factor that takes into account the internal RBW and log detection
                           stage losses, inherent in any spectrum analyzer, of approximately 2 dB. The
                           formula for digital power measurement now becomes:

                          True digital power (dBm)   measured power (dBm)   BWCF (dB)   2 dB

                        Constellation and eye diagrams. To view the degradation created by noise and
                        frequency instabilities in a digital signal, as well as other impairments, we can
                        employ constellation and eye diagrams.
                          To measure or view constellation or eye diagrams requires the ability to tap
                        into the digital receiver demodulator’s I and Q outputs, as well as the demod-
                        ulator’s timing clock (Fig. 2.43). The outputs of the demodulator’s I and Q
                        may be fed into an oscilloscope with an X-Y display that has the capability to
                        turn on a persistence function for a view of the I/Q outputs over time. Such a
                        setup will allow the operator to confirm the phase and amplitude differences
                        of the output signal—in the form of a constellation diagram—thus allowing
                        the viewing of the signal’s quality (lack of distortion, phase noise, or ampli-
                        tude instabilities). A perfect constellation diagram with no impairments is
                        shown in Fig. 2.44a.
                          Constellation diagrams display the digital modulation’s symbol patterns,
                        while eye diagrams (Fig. 2.44b) permit the transition of the symbols to be
                        viewed over time. Both measure the baseband signal’s modulation condition,
                        and whether impairments are degrading this expected pattern. In eye dia-
                        grams the eye itself is rounded, instead of square, because of the necessary
                        limiting of the baseband bandwidth by filters. The eye comprises two lines, one
                        at digital 1 and the other at digital 0, and is only a series of pulses displayed
                        on the phosphor of the test oscilloscope, with each pulse being sent out of the
                        receiver’s demodulator with noise and jitter added by the transmitter, the sig-
                        nal path, and the receiver. This makes each pulse slightly different from the



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