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PLL PERFORMANCE IN THE PRESENCE OF NOISE   Ronald E. Best                               96






























                      Figure 4.3 Definition of noise parameters, for symbols (cf. text).

             Fig. 4.3. (Note that H is plotted versus frequency f here, and not versus radian frequency ω.)
             This simply means that the PLL is able to track frequencies within a passband centered at the
             down-scaled center frequency  f ′ (f ′ =  ω ′/2π). The symbol  B  stands for  noise
                                             0     0        0                        L
             bandwidth (this term will be defined in Sec. 4.3). Let us state for the moment that the one-
             sided noise bandwidth B /2 is approximately equal to the earlier-defined 3-dB bandwidth f 3dB
                                    L
             (f   = ω    /2π). As we easily recognize from Fig. 4.3, the noise spectrum that is outside of
              3dB     3dB
             the passband of the PLL will  be suppressed by the loop, hence only the part of the noise
             spectrum within the noise bandwidth is able to corrupt PLL performance. As will be explained
             in the following sections, two important parameters describe noise performance:
             ■ The signal-to-noise ratio SNR  = P /P  at the input of the PLL
                                            i    s  n
             ■ The ratio B /B  of input noise bandwidth B  to PLL noise bandwidth B
                           i  L                          i                         L



             The Impact of Noise on PLL Performance

                                                                                   1
             The noise analysis presented here is based on the work of  Gardner.  We shall consider
             amplitude and power density spectra of information signals and noise signals. Two types of
             power density spectra have been defined: one-sided and two-sided. If an information signal
             has one single spectral  line at a frequency  f —for example, the one-sided power density
                                                          0
             spectrum shows up a line at f , but the two-sided spectrum would have two spectral lines at f
                                                                                                       0
                                         0
             and at −f , respectively. The same applies for noise spectra. It is a matter of taste whether to
                      0
             use one-sided or two-sided power spectra. When using two-sided power spectra, the total
             power of a signal can be calculated by integrating its power density spectrum over the
             frequency interval −∞ < f < ∞. For one-sided spectra, however,
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