It seems to me: a factor common to all instances of visible interference effect is consistent phase relation.
I will go over a series of cases of interference effect, setting up for a discussion of the notion of consistent phase relation.
Thin film interference:
A well known instance of thin film interference effect is that some drops of gasoline have spilled into a puddle of water. The gasoline spreads out over the surface, creating a thin film, the thickness is in the order of micrometers.
The interference effect from the thin film gives rise to bands of colors; areas of equal color are areas of equal film thickness.
The thin film interference color effects occurs with straightforward daylight. As we know, daylight is wide band, and on an overcast sky all daylight is scattered light. So: for the source of the light we have: no temporal coherence, no spatial coherence.
The factor that makes it possible for interference effect to occur is that the reflection against the top surface and the reflection against the gasoline-water interface occur in very close proximity. (Close to the wavelength of visible light.)
A double slit interference demonstration with sunlight as light source.
Setting up a double slit interference demonstration with sunlight is challenging, but doable.
The demonstration is set up in a darkened room. The only light entering the room is through a small hole. I will refer to that as 'the source hole'. From the source hole the light travels to the screen with the two slits. The reason that the source hole needs to be small is as follows:
-all of the light that reaches the left hand slit must have traveled the same distance, to within the wavelength of the light.
-all of the light that reaches the right hand slit must have traveled the same distance, to within the wavelength of the light.
The size of the source hole must be small enough such that as seen from the screen with the slits the source is in effect a point source of light. When the source is (relative to the target) a point source then as the light reaches the target it has a property called 'spatial coherence'.
For the light that passes through the slit there is diffraction.
The property of spatial coherence carries over to the light that makes it through the slit.
By contrast: if the light that reaches the two slits comes from a wide source then no visible interference pattern can be obtained. It is when all of the light that reaches the slit has traveled the same distance (to within the wavelength) that a visible interference pattern is possible.
As we know, sunlight is a spectrum of frequencies. Because of that: the interference pattern that is obtained that way is sharply defined only for the central line. Away from the central line there are chromatic effects.
There is of course the famous Michelson-Morley experiment. According to the wikipedia article: for alignment light from a Sodium lamp was used, and for taking the measurements, which was done by looking into an eyepiece, white light was used.
So the light source that was used did not have the property of temporal coherence.
Not having a source of light with temporal coherence made the Michelson-Morley experiment very challenging, but still doable.
Just as in the case of a double slit setup: for the Michelson-Morley experiment the light source must be set up such that the light entering the interferometer has the property of spatial coherence.
The light travels two different paths through the interferometry setup. An interference pattern is obtained if and only if the two paths have the same length, to within the coherence length of white light, which is several micrometers. (The wavelength of visible light is from 0.4 to 0.7 micrometers.)
A Mercury vapor lamp produces light that is suitable for interferometry. The emission lines include 404.7 nm, 438.8 nm, and 546.1 nm lines. Filters are used to remove the wavelengths other than the 546.1 nm wavelength.
In the Kennedy-Thorndike experiment a Mercury vapor lamp was used as source, because the experiment was set up to use arms of different length. There is a relation between spectrum width and coherence length. Wide spectrum light, such as daylight, has short coherence length, the closer to monochromatic a light source is the longer the coherence length.
The Mercury 546.1 nm emission line has a coherence length of about 32 centimeter.
About 'temporal coherence':
Temporal coherence is about consistent phase relation. Given the degree of narrowness of the 546.1 nm emission line: there is over a longer length a sufficient phase relation so that there is still a visible interference effect.
While temporal coherence is a temporal property it is usually encountered in the form of managing length. How much difference in pathlength there can be while still obtaining an interference pattern.
Finally, we get to interference setups with a laser.
The light exits the laser cavity through a very small hole. The hole is so small that you get a divergent beam (diffraction). A collimating lens is used to refract that divergent beam to a parallel beam.
A laser source, when properly constructed, has spatial coherence. So that takes care of spatial coherence.
The large temporal coherence that a laser offers is a great asset; it makes interferometry setups much easier to accomplish; the paths can have large length difference..
Consistent phase relation
Returning to the case of thin film interference effect:
the incoming light is scattered light: in effect we can think of the incoming light as originating from an exceedingly large amount of individual sources, spread across the sky. For the thin film interference efffect: single source or many sources makes no difference: what counts is phase relation.
With a thin film interference effect the two reflections occur very close together. The thickness of the thin film is within the coherence length of daylight.
About double slit setup: a more performant version is a diffraction grating (When instrument makers succeeded in making high quality diffraction gratings astronomers started using them for spectral analysis of starlight.)
Obtaining interference fringes with a diffraction grating is more demanding in the sense that in order to obtain consistent phase relation the light source that illuminates the two diffraction grating must be (relative to the diffraction grating) a point source.
If a star is far enough away then the entire star is effectively a point source. The condition of consistent phase relation is met: an interference pattern is obtained.