One property of light sources that is usually stated, which is of particular importance when trying to create interference fringes, is the coherence length (or coherence time). The equation for the coherence length is given by $l_c = \frac{c}{n\Delta{f}}$ where $c$ is the speed of light, $n$ is the refractive index of the medium and $\Delta{f}$ is the bandwidth of the source.
An alternate description that I've seen (but unfortunately have lost a decent reference for) is that given a source emitting with wavelength range $\lambda \pm \Delta{\lambda}$, $l_c$ is the length that light with wavelength $\lambda$ and $\lambda + \Delta{\lambda}$ travels before they go from completely in-phase to completely out of phase. It leads from these definitions that an ideal, monochromatic source has an infinite coherence length and a broadband white light source has a very short coherence length.
This definition I am fairly happy with and can see what $l_c$ is trying to describe. The problem arises when we begin to talk about the limitations on when these non-idea light sources can produce interference.
Consider a Mach-Zinder interferometer (MZI):
it is always stated that in order to see an interference pattern through the MZI, (or for any other interference experiment) you must match the path-lengths of each arm of the interferometer to within the coherence length of the source.
My question is, quite simply, why? Considering the MZI and the definition of the coherence length above, I cannot seem to form an image in my mind as to why this should be so. I am able to follow the mathematics of the MZI (including the introduction of the degree of first-order temporal coherence: $g^{(1)}(\tau)$ - which is where this question first arose) but creating a physical image in my mind is proving very tricky.