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. ”
