Page 232 - Phase-Locked Loops Design, Simulation, and Applications
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MIXED-SIGNAL PLL APPLICATIONS PART 1: INTEGER-N FREQUENCY
                SYNTHESIZERS   Ronald E. Best                                                          140

                      This is the noise power within the frequency interval from 10,000 to 10,001 Hz relative to
                    the carrier frequency. Next S *(f ) is to be computed. We get
                                             θθ
                                                 m





                      Hence, S *(f )  becomes
                                  m dB
                              θθ



                      We conclude that the noise power within a bandwidth of 1 Hz at offset frequency f  = 10
                                                                                               m
                    kHz is 120 dB below carrier power. Furthermore, we see that the mean square value of phase
                                                                                                    2
                    perturbation within a bandwidth of 1 Hz at modulating frequency f  = 10 kHz is 10 −12  rad .
                                                                               m
                    For the rms value of phase perturbation in that frequency interval we get




                      To avoid confusion  with the standards used in practically all books and papers on
                    frequency synthesizers, we will nevertheless use the familiar unit dBc/Hz for power density
                    of phase jitter, although this unit has been shown to be somewhat incorrect.

                 As mentioned earlier, real amplifiers add further noise. Noise performance of amplifiers is
               specified by noise figure F which is defined by



                                                                                           (6.10)



               in other words, F is the ratio of signal-to-noise at the output to signal-to-noise at the input. For
               a real amplifier S ,  (f ) becomes larger than S ,  (f ) by factor F; thus, we now have
                               θθ out m                       θθ out m






                 When we assume F = 6 dB, S ,      (f )  increases by 6 dB, thus
                                              θθ out m dB




                 In real amplifiers, we are not only confronted with thermal noise, but there is always
               another noise source called flicker noise. Flicker noise is also referred to as 1/f noise, because
               the power spectral density of flicker noise varies with   amplifier, however, at frequencies
               below a corner frequency denoted as f  [cf. Fig. 6.16]. For operational amplifiers, for example,
                                                    c
               f  can be on the order of 10 Hz to some kHz. In oscillators, f can easily extend into the MHz
                c                                                         c
               region.
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