Summary

1911 Encyclopædia Britannica, Volume 8… (1911)

From this we may infer the limitation upon the width of the source of light, in order that the bands may be properly formed. If ω be the apparent magnitude of the source seen from A, ωb should be much smaller than the above quantity, or
If a be very great in relation to b, the condition becomes
so that if b is to be moderately great (1 metre) , the apparent magnitude of the sun must be greatly reduced before it can be used as a source. The values of V for the maxima and minima of intensity, and the magnitudes of the latter, were calculated by Fresnel.
Source: Wikisource

1911 Encyclopædia Britannica, Volume 8… (1911)

At the point O the intensity is one-quarter of that of the entire wave, and after this point is passed, that is, when we have entered the geometrical shadow, the intensity falls off gradually to zero, without fluctuations. The whole progress of the phenomenon is thus exhibited to the eye in a very instructive manner.
We will next suppose that the light is transmitted by a slit, and inquire what is the effect of varying the width of the slit upon the illumination at the projection of its centre.
Source: Wikisource

Get perspective with Kwize: daily news enlightened by great literature