Let's summarize the derivation in Whitham's Linear and Nonlinear Waves, $\S 4.1$: The Cole-Hopf Transformation
Burgers' equation
The Burgers equation is the simplest example of a partial differential equation demonstrating both diffusive and nonlinear propagation effects.
$$
u_{\color{red}{t}} + u u_{\color{blue}{x}} = \nu u_{\color{blue}{xx}}
\tag{1}
$$
Coloring distinguishes $\color{red}{time}$ derivatives from $\color{blue}{space}$ derivatives.
Cole-Hopf transform
The nonlinear transform of Cole and Hopf is,
$$
u = -2\nu \frac{\varphi_{\color{blue}{x}}}{\varphi},
$$
similar to the Thomas transformation of exchange equations. The transformation is resolved into two steps.
Step 1
Set $$u = \psi_{\color{blue}{x}},$$ and equation (1) becomes
$$
\psi_{\color{red}{t}} + \frac{1}{2}\left(\psi_{\color{blue}{x}}\right)^{2} = \nu \psi_{\color{blue}{xx}}
\tag{2}
$$
Step 2
Set $$\psi = -2\nu \ln \varphi,$$ and equation (2) reduces to the heat equation
$$
\boxed{
\varphi_{\color{red}{t}} = \nu \varphi_{\color{blue}{xx}}
}
\tag{3}
$$
The nonlinear term has vanished because of the nonlinear transformation.
Transforming heat equation solutions to Burgers equation solution
The initial value problem which starts with a spatial waveform
$$
u = F(x), \qquad t =0
$$
transforms into
$$
\varphi = \Phi(x) = e^{-\frac{1}{2\nu}\int_{0}^{x} F(\varphi)d\eta}, \qquad t = 0
$$
The heat equation solution for this IVP is
$$
\varphi = \frac{1}{\sqrt{4\pi \nu t}} \int_{-\infty}^{\infty} \Phi(\eta)e^{-\frac{(x-\eta)^{2}}{4\nu t}} d\eta
$$
Going back to the Cole-Hopf transform to recover the solution function $u$:
$$
u(x,t) = \frac
{\int_{-\infty}^{\infty} \frac{x-\eta}{t} e^{-\frac{G}{2\nu}} d\eta}
{\int_{-\infty}^{\infty} e^{-\frac{G}{2\nu}} d\eta}
$$
with the function
$$
G\left(\eta; x, t \right) =\frac{\left( x - \eta \right)^{2}}{2t} +
\int_{\eta}^{0} F\left(\xi \right) d\xi
$$