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Noise Rejection Performance

In this section the ability of a phaselock loop to cope with noise is examined. Consider the input signal of a phaselock loop and assume that as well as a sinusoidal signal, additive noise of n(t)volts with one sided spectral density Sn(f) is also admitted. Therefore the input voltage to the phase detector is given by

\begin{displaymath}
v_i(t)=V_s\sin(\omega_it+\varphi_i)+n(t)\quad [V].\end{displaymath}

The other input to the phase detector is due to the VCO. Because it is typical that VCO's lock in quadrature to the incoming signal, the VCO signal is typically $\frac{\pi}{2}$ out of phase with vi. In anticipation of this fact, it is useful to write

\begin{displaymath}
v_o(t)=V_o\cos(\omega_it+\varphi_o).\end{displaymath}

The additive noise n(t) can be expanded into two quadrature components

\begin{displaymath}
n(t)=n_c(t)\cos\omega_it-n_s(t)\sin\omega_it\end{displaymath}

One may then define the dimensionless quantity n' as

\begin{displaymath}
n'(t)=\frac{n_c(t)}{V_s}\cos\varphi_0\frac{n(t)}{V_s}\end{displaymath}

It can be shown [11] that the variance, $\overline{\varphi_{no}}$ of the output noise n(t) is given by

\begin{displaymath}
\overline{\varphi_{no}}=\int_0^{\infty}S_{n'}(f)\vert H(j\omega)\vert^2df.\end{displaymath}

where $H(j\omega)$ is the filter transfer function defined by equation (3.13), Sn'(f) is the one-sided spectral density of n' and $\omega=2\pi f$. In general, the form of Sn(f) impedes the evaluation of the above integral. If one considers white noise where $S_n(f)=\frac{1}{2}\eta$, the above integral simplifies to

\begin{displaymath}
\overline{ \varphi_{no}}=\frac{\eta}{V_s^2}\int_0^{\infty}\vert H(j\omega)\vert^2df\end{displaymath}

where

\begin{displaymath}
B_L=\int_0^{\infty}\vert H(j\omega)\vert^2df\end{displaymath}

is the noise bandwidth . Hence for input white noise, the phase variance is simply  
 \begin{displaymath}
\overline{ \varphi_{no}}=\frac{\eta B_L}{V_s^2}.\end{displaymath} (21)
Gardner [11] details the noise bandwidths of various loop types and they are reproduced in table 3.3.
 
Table 3.3:  Noise bandwidths of common loops
Loop Description Noise Bandwidth, BL(Hz))
First Order $\frac{1}{4}K$
Second order passive $\frac{1}{4}K\frac{K+\frac{1}{\tau_2}}{K+\frac{1}{\tau_1}}$
Second order active $\frac{1}{4}K\left(1+\frac{1}{\tau_2K}\right)$

where K is the open loop gain defined for various loops in table 3.2. It can be seen that K plays a central role in establishing the noise bandwidth and hence the output phase variance. It is necessary for K and hence KoKd, to be small in order to minimise the output jitter due to external noise.
next up previous contents
Next: PLL Tracking Up: Performance Comparison of Different Previous: Performance Comparison of Different
Mark J Ivens
11/13/1997