35 Diffraction and Image Formation Where was modern

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35. Diffraction and Image Formation Where was modern optical imaging technology born? Zeiss Jena

35. Diffraction and Image Formation Where was modern optical imaging technology born? Zeiss Jena Abbe Schott

Geometrical Optics… point sources point images f f …implies perfect resolution.

Geometrical Optics… point sources point images f f …implies perfect resolution.

Physical Optics… diffracting source Imperfect image Every lens is a diffracting aperture.

Physical Optics… diffracting source Imperfect image Every lens is a diffracting aperture.

Multiple Slits b a b a b r

Multiple Slits b a b a b r

Central maximum Principle maxima secondary maxima

Central maximum Principle maxima secondary maxima

Diffraction Grating A special corner of multi-slit-space: N ~ 104, a ~ l, b

Diffraction Grating A special corner of multi-slit-space: N ~ 104, a ~ l, b ~ l: central maximum is very large! a ~ l: principle maxima are highly separated! (most don’t exist) N ~ 104: Principle maxima are very narrow! Secondary maxima are very low! typical grating specs: 900 g/mm, 1 cm grating. N = 9, 000 a = 1. 11 microns b = 1. 11 microns l = 0. 633 microns!

m=1 “first order” grating m=0 monochromatic light Maxima at:

m=1 “first order” grating m=0 monochromatic light Maxima at:

Abbe Theory of Image Formation grating m = +1 m=0 m = -1 focal

Abbe Theory of Image Formation grating m = +1 m=0 m = -1 focal plane diffraction plane

Abbe Theory of Image Formation grating m = +1 Resulting interference pattern is the

Abbe Theory of Image Formation grating m = +1 Resulting interference pattern is the image m=0 m = -1 focal plane diffraction plane

Image formation requires a lens large enough to capture the first order diffraction. m

Image formation requires a lens large enough to capture the first order diffraction. m = +1 Grating Equation: a m=0 f D To resolve a: Resolution (diffraction limited):

Rectangular Apertures P(X, Y, Z) r d. A(x, y, z) R a b Rather

Rectangular Apertures P(X, Y, Z) r d. A(x, y, z) R a b Rather than an aperture, consider an object:

Remember, the integral is over the aperture area: Let’s rearrange that a little it

Remember, the integral is over the aperture area: Let’s rearrange that a little it (this is where the magic happens): THAT’S A FOURIER TRANSFORM!! EP(X, Y, Z) = F{EFeynman} Where does diffraction put the spatial frequencies in EFeynman?