As stated in Wikipedia's page:
Correlation or dependence is any statistical relationship, whether causal or not, between two random variables.
Now in "The Quantum Theory of Optical Coherence" Glauber introduces a set of functions he says quantifies correlations:
The field average (3.3) which determines the counting rate of an ideal photodetector is a particular form of a more general type of expression whose properties are of considerable interest. In the more general expression, the fields $E^{(-)}$ and $E^{(+)}$ are evaluated at different spacetime points. Statistical averages of the latter type furnish a measure of the correlations of the complex fields at separated positions and times. We shall define such a correlation function, $G^{(1)}$, for the $\mathbf{e}$ components of the complex fields as $$G^{(1)}(\mathbf{r},t;\mathbf{r}',t')=\operatorname{tr}\left\{\rho E^{(-)}(\mathbf{r},t)E^{(+)}(\mathbf{r}',t')\right\}\tag{3.6}$$
He then more generaly defines the $n$-th order correlation functions as a function of $2n$ spacetime points $x_1,\dots, x_{2n}$:
$$G^{(n)}(x_1,\dots, x_n;x_{n+1},\dots, x_{2n})=\operatorname{tr}\left\{\rho E^{(-)}(x_1)\cdots E^{(-)}(x_n)E^{(+)}(x_{n+1})\cdots E^{(+)}(x_{2n})\right\}\tag{3.8}$$
In all the above, $\rho$ is the quantum state of the electromagnetic field.
My question here is the following: why these $G^{(n)}$ are called correlation functions? How they are connected with the statistical idea of correlation?
I imagine in some sense they should quantify some sort of statistical relationship between measurements associated to photons at each of the spacetime points (detection of the photons, perhaps?), but this is an impression because of the name. I want to understand really why these $G^{(n)}$ functions quantify correlations and what are the correlations they are quantifying.