Three Experiments in One



 

 


Single Slit Diffraction in the Fraunhofer Plane:


        To understand the Single Slit example, one must revert to Huygen's Principle of 1678 which describes how a point on a wave-front can be thought of as contributing to a secondary forward travelling spherical wavelet.   In the case of the Single slit, any part of the slit can be thought of as such a point.  The coherent superposition of these wavelets produced at the slit results in the diffraction pattern seen at the focal length of the lens (the Fraunhofer Plane).   This diffraction pattern can be explained by the Fresnel-Kirchoff Formula explained in the introduction to this lab.  With the below situation,

singleslit.jpg (7219 bytes)

L represents the slit length, b the slit width, and y the point of origin of the forward travelling wavelet.  Plugging these constraints and variables into the Fresnel-Kirchoff formula yields the diffraction intensity relationship in the following Fourier transform integral:

Image104.gif (1245 bytes)

The Ldy replaces LdA and r is replaced by ro+ySin(theta) (**ro is the value for r when y=0) in the Fresnel-Kirchoff formula.  This integral is easily evaluated over this range in a program such as mathmatica.   Integration and simplification yields the result

Image105.gif (1659 bytes)Here ß = kbSin(theta)/2 and C' = eikroCbL.  This expression represents the total amplitude of light diffracted in a given direction defined by the term ß.  In terms of frequency and slit width, ß = (b/2)(kv/f) where k and v are constants.  A note about this relationship is that it is defined at the Fraunhofer Plane (focal point of the lens), thus reapplying Huygen's principle this plane leads to some interesting new concepts.

    If one thinks of the Fraunhofer plane as we previously did the single slit, then it ALSO represents a source for secondary forward travelling wavelets.  Each point on the diffraction pattern on the plane will cause these wavelets to superpose and recombine at some other point in the image plane of the lens.  It can also be characterized by a Fourier integral and believe it or not it is the expression for the diffraction pattern at the Fraunhofer plane wpeA.jpg (1304 bytes)!!!  Performing the Fourier transform of this should then give us a relationship describing the slit itself.  In other words, at some point beyond the Fraunhofer plane we will see an image of the slit!   To see whether or not all of this actually occurs, check out our data section where we show you....or not!

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Theory of Screen Diffraction in the Fraunhofer Plane:


    The screen situation is analogous to several square slits next to each other, both horizontally and vertically.  Mathematically, the problem is an extension of the single and double slit examples in two dimensions.  All of the variables that we need for a one-dimensional discussion are defined in the picture below:

multislit.gif (2880 bytes)

In the picture of multiple slits above, b represents the slit width and h their separation.  It also consists of N identical parallel slits, of course that may be an impossible situation to produce on the production line of the chicken wire, but we theorize for the fun of it!  Using the base equation for the single slit and modifying to fit our situation, we are blessed with the following integral:

So, to solve this problem, we integrate over each slit individually and add them together which makes sense intuitively as well.  The solution to this integral, with N number of slits of width b and separation h, is also similar to the solution of the single slit problem, with a few extra terms of course, and looks like this:

Above, and while N normalizes the expression. The observed intensity is again the square of this expression times the incident intensity at the slits. 

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Theory of Pinhole Diffraction in the Fraunhofer Plane:


    This experiment is basically the equivalent of sending light from a source through a circular aperture, in our case a piece of aluminum foil with a pinhole punched through it.  We therefore have the following scenario:

circular.gif (4734 bytes)

Imagine the square with the circle in it as the front view of the vertical aperture on the right in the picture above.  In this case, we are integrating over y with dy defined as above.  The dA term of the Fresnel-Kirchoff equation now becomesNow it is easy to define a relationship that describes our situation by merely adjusting the Fresnel-0Kirchoff

formula again.  Substituting our adjusted dA term into it and simplifying, we arrive at the following relationship:

Even though it was somewhat easily derived, the solution to this integral is very nasty and involves what are known as bessel functions.  Thus, a change of variables is performed to simplify our anguish a little.  We define two new variables, mu and rho, which are expressed as and .   Our integral now becomes which can be integrated using mathmatica:

Untitled-1.txtgr1.gif (1293 bytes)

Untitled-1.txtgr3.gif (1457 bytes)

The solution reveals a first order Bessel function (oh the joy!) which then gives us a function describing the diffraction in the Fraunhofer plane.  The function is plotted below using mathmatica.  The picture on the right is the diffraction amplitude as mathmatica says it will appear in three dimensions (we go from rho=0 to rho=15).  The actual intensity observed at the Fraunhofer plane is seen in the picture on the right (Intensity is simply the square of the solution)

 kmart.txtgr8.gif (2325 bytes)wpe38.jpg (7691 bytes)

The central fringe, which is appears as a circle, can be seen very clearly in relationship to the smaller outer fringes. 

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What is Spatial Filtering?

With each of the previous apertures we used some sort of spatial filter at the Fraunhofer Plane to prohibit certain components of the diffraction pattern from recombining at the image plane.

Consider the diffraction aperture a function of the spatial variable.  Expanding what was previously discussed, Fourier transforming the aperture function should yield the diffraction pattern (as a function of a 'spatial frequency') observed at the Fraunhofer Plane.  Taking another Fourier transform should return the aperture function.

If one includes a spatial filter in the system, a representative function of 'spatial frequency' must be included in the second Fourier integral.  This filtering results in information blocked and prevented from reaching the image plane.  Thus, 'holes' appear in the image.  As will be seen in the data and conclusions section, when we blocked the central peak of the diffraction pattern and allowed the outside fringes to pass to the image plane, this information did little to build the central portion of the image, but constructed the edges of the image.

A helpful analogy to this is in considering the composition of a square wave g(y).  

sqrwave1.JPG (2553 bytes) It's Fourier transform demonstrates that it is composed of many sine waves, with one dominant frequency.

sqrwave2.JPG (6280 bytes) When the central peak (or, in the Fourier transform analogy, the dominant frequency) is removed, only the fringes (or the other frequencies composing the square wave) remain to form the image.

sqrwave3.JPG (6226 bytes) Thus, when the dominant frequency is removed, only the edges of the image will appear clearly at the image plane.

Likewise, when the fringes surrounding the central bright spot are removed, information carried in the diffraction pattern about the edges of the object is lost.  Thus, at the image plane, the object's edges do not appear clearly.

Click here to see an example of how this is modeled, via. mathematica, for a single-slit aperture.


  1. Abstract
  2. Introduction to Theory
  3. The Setup
  4. The Data and Conclusions

References:

Pictures and derivation adapted from:

Fowles, Grant R.  Introduction to Modern Optics.   Dover Publications: New York.  1975.