My question concerns the dimensions of the autocorrelation function of the white noise.
First is a short summary of what I understand about the random signals. If we have a stationary random signal $x(t)$ whose amplitude is a random variable distributed according to some probability law : $p(x)$, then :
- its autocorrelation function is an ensemble average of $x(t)\,x(t+\tau)$ : $$ R_{xx}(\tau) = \int_{-\infty}^{\infty}\ x(t)\,x(t+\tau)\,p(x)dx $$ -if the signal is ergodic, we can replace the ensemble average by the time average to obtain another expression for the signal autocorrelation : $$ R_{xx}(\tau) = \lim_{T \rightarrow \infty}\frac{1}{T}\int_{-T/2}^{T/2}\ x(t)\,x(t+\tau)\,dt $$ From both of these expressions, the dimensions of $R_{xx}$ are $[x^2]$ whatever are units of $x$. Suppose also that the signal is zero-mean, then $R_{xx}(0) = \sigma^2$, the variance of $x$. If $x(t)$ is a white-noise, then any source I read informs me that : $$ R_{xx}(\tau) = \sigma^2\,\delta(\tau) $$ But according to this last expression, the units of $R_{xx}$ are now : $[\frac{x^2}{s}]$.
Here is the question : how come that we change the dimensions of $R_{xx}$ by passing from the general expression to this particular expression for white-noise?
I would greatly appreciate your help. Let me know if I was not clear enough somewhere.
Hello everyone,
Thank you for your answers and corrections. I will put here the corrected version of $R_{xx}(\tau)$ in terms of an ensemble average :
$$ R_{xx}(\tau) = \iint_{-\infty}^{\infty}\ x_1\,x_2\,p(x_1,x_2,t_1,t_2)dx_1\,dx_2 $$
where $t_1 = t$, $t_2 = t + \tau$, $x_1 = x(t)$, $x_2 = x(t+\tau)$. I am assuming here that the $R_{xx}$ depends only on the separation between two different time moments and not their particular values.
This correct expression does not change the dimensions of $R_{xx}$ however, it is still $[x^2]$ or $V^2$ for example.
Unfortunately I am not quite sure I understand your answers. So, I will try ask one more question, which is related to my first one.
Suppose we have an ergodic bandwidth limited Gaussian noise $x(t)$ of zero-mean and finite variance $\sigma^2$ :
$$ x \sim \mathcal N (0, \sigma^2) $$
In addition, the values of the signal at any two moments of time are not correlated. From the time average form of $R_{xx}(\tau)$ we get :
$$ R_{xx}(\tau) = \left \{ \begin{aligned} \sigma^2\ , \tau = 0\\ 0\ , \text{otherwise} \end{aligned} \right . $$
The power spectral density $PSD$ is constant for any frequency :
$$ PSD(f) = \frac{\sigma^2}{F_s}\quad ,\text{where}\ -F_s/2 < f < F_s/2 $$
where $F_s$ is the sampling frequency. The area under the PSD gives the power of the signal :
$$ \text{Power} = \frac{\sigma^2}{F_s} F_s = \sigma^2 $$
So, for the signal considered the variance is finite, is not
$$ R_{xx}(\tau) = \sigma^2\,\delta(\tau) $$
and $R_{xx}(\tau)$ has dimensions of $V^2$.
Now imagine we let $F_s$ to increase infinitely to obtain a white Gaussian noise which has infinite frequency content. For me, $R_{xx}$ will remain the same. No matter how big is $F_s$. The only thing which will change, is $PSD$, which will become smaller and smaller, but in the way that the area under $PSD$ remains equal to $\sigma^2$.
Is there anything wrong with this reasoning? I do understand that to get $R_{xx}(\tau) = \sigma^2\,\delta(\tau)$ one needs to fix the PSD : $PSD = \sigma^2$. But this does not make any sens to me, as the area under the horizontal line does not have the units of the power any more.
Thanks in advance for your help.