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Fresnel diffraction

   Also found in: Wikipedia 0.01 sec.
Fresnel diffraction [frā′nel di′frak·shən]
(optics)
Diffraction in which the source of light or the observing screen are at a finite distance from the aperture or obstacle.


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Although a relic of the early 19th century, the Fresnel diffraction integral (2) is still used today in its original form and has remained a most useful, reliable tool for diffraction calculations that have consistently yielded results which agree with experience and are well documented (2).
Similarly, the reverse Fresnel field is zero for z > 0 and equal to a Fresnel diffraction pattern superimposed on the reflected geometrical field for z < 0.
Shadow edges: Fresnel diffraction at a straight edge.
 
 
 
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