Editing Appendix/CGH/ParallelApertures2D

__FORCETOC__ <!--  will force the creation of a Table of Contents -->
<!-- __NOTOC__ will force TOC off -->
=CGH:  2D Rectangular Apertures that are Parallel to the Image Screen=


<table border="1" align="center" width="100%" colspan="8">
<tr>
  <td align="center" bgcolor="lightblue" colspan="4" cellpadding="8">
Computer Generated Holography
  </td>
</tr>
<tr>
  <td align="left" bgcolor="lightblue" width="25%" rowspan="2">
<ul>
<li>[[Appendix/CGH/Preface|Preface]]</li>
<li>[[Appendix/Ramblings/FourierSeries#One-Dimensional_Aperture|Fourier Series]]</li>
<li>[[Appendix/CGH/ParallelAperturesConsolidate|Consolidated Expressions]]</li>
<li>[[Appendix/QED|Feynmann's Path-Integral Formulation]]</li>
</ul>
  </td>
  <td align="center" bgcolor="lightblue" width="75%" rowspan="1" colspan="3" cellpadding="8">
Apertures Parallel to Image Screen
  </td>
</tr>
<tr>
  <td align="center" bgcolor="lightblue" width="25%"><br />[[Appendix/CGH/ParallelApertures|Part I: &nbsp; One-Dimensional Apertures]]
&nbsp;
  </td>
  <td align="center" bgcolor="lightblue" width="25%"><br />[[Appendix/CGH/ParallelApertures2D|Part II: &nbsp; Two-Dimensional Apertures]]
&nbsp;
  </td>
  <td align="center" bgcolor="lightblue"><br />[[Appendix/CGH/ParallelAperturesHolograms|Part III: &nbsp; Relevance to Holograms]]
&nbsp;
  </td>
</tr>
</table>


This chapter is intended primarily to replicate [http://www.phys.lsu.edu/faculty/tohline/phys4412/howto/slit2d.html &sect;I.B from the online class notes] &#8212; see also an updated [[Appendix/Ramblings#Computer-Generated_Holography|Table of Contents]] &#8212; that I developed in conjunction with a course that I taught in 1999 on the topic of ''Computer Generated Holography (CGH)'' for a subset of LSU physics majors who were interested in computational science.  This discussion parallels the somewhat more detailed one presented in [[Appendix/CGH/ParallelApertures|&sect;I.A]] on the one-dimensional aperture oriented parallel to the image screen.

==Utility of FFT Techniques==
Consider the amplitude (and phase) of light that is incident at a location (x<sub>1</sub>, y<sub>1</sub>) on an image screen that is located a distance Z from a rectangular aperture of width ''w'' and height ''h''.  By analogy with [[Appendix/CGH/ParallelApertures#Utility_of_FFT_Techniques|our accompanying discussion in the context of 1D apertures]], the complex number, A, representing the light amplitude and phase at (x<sub>1</sub>, y<sub>1</sub>) will be,
<table border="0" cellpadding="5" align="center">

<tr>
  <td align="right">
<math>~A(x_1, y_1)</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~ \sum_j \sum_k
a_{jk} e^{i(2\pi D_{jk} /\lambda + \phi_{jk})} 
\, ,
</math>
  </td>
</tr>
</table>
where, here, the summations are taken over all "j,k" elements of light across the entire 2D aperture, and now the distance D<sub>jk</sub> is given by the expression,

<table border="0" cellpadding="5" align="center">

<tr>
  <td align="right">
<math>~D^2_{jk}</math>
  </td>
  <td align="center">
<math>~\equiv</math>
  </td>
  <td align="left">
<math>~
(X_j - x_1)^2 + (Y_k - y_1)^2 + Z^2  
</math>
  </td>
</tr>

<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
Z^2 + y_1^2 - 2y_1 Y_k + Y_k^2 + x_1^2 - 2x_1 X_j + X_j^2 
</math>
  </td>
</tr>

<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~
L^2 \biggl[1 - \frac{2(x_1 X_j + y_1 Y_k ) }{L^2}  + \frac{X_j^2 + Y_k^2}{L^2} \biggr] \, ,
</math>
  </td>
</tr>
</table>
and,
<table border="0" cellpadding="5" align="center">

<tr>
  <td align="right">
<math>~L</math>
  </td>
  <td align="center">
<math>~\equiv</math>
  </td>
  <td align="left">
<math>~
[Z^2 + y_1^2  + x_1^2]^{1 / 2} \, .
</math>
  </td>
</tr>
</table>

If <math>~|X_j/L| \ll 1</math> and <math>~|Y_k/L| \ll 1</math> we can drop the quadratic terms in favor of the linear ones in the expression for  D<sub>jk</sub> and deduce that,
<table border="0" cellpadding="5" align="center">

<tr>
  <td align="right">
<math>~D_{jk}</math>
  </td>
  <td align="center">
<math>~\approx</math>
  </td>
  <td align="left">
<math>~
L \biggl[1 - \frac{2(x_1 X_j + y_1 Y_k ) }{L^2}  \biggr]^{1 / 2} 
</math>
  </td>
</tr>

<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~\approx</math>
  </td>
  <td align="left">
<math>~
L \biggl[1 - \frac{(x_1 X_j + y_1 Y_k ) }{L^2}  \biggr] \, .
</math>
  </td>
</tr>
</table>

Hence, the double-summation expression for the amplitude at screen location (x<sub>1</sub>, y<sub>1</sub>) becomes,
<table border="0" cellpadding="5" align="center">

<tr>
  <td align="right">
<math>~A(x_1, y_1)</math>
  </td>
  <td align="center">
<math>~\approx</math>
  </td>
  <td align="left">
<math>~ A_0 \sum_j \sum_k
a_{jk} e^{i\phi_{jk} } \cdot \exp\biggl\{ -i \biggl[ \frac{2\pi(x_1 X_j + y_1Y_k}{\lambda L} \biggr] \biggr\}
\, ,
</math>
  </td>
</tr>
</table>
where, 
<div align="center">
<math>~A_0 \equiv e^{i(2\pi L/\lambda)}</math>.
</div>
When written in this form, it should be apparent why discrete Fourier transform techniques &#8212; specifically, 2D-FFT techniques &#8212; are useful tools for evaluation of the complex amplitude, A(x<sub>1</sub>, y<sub>1</sub>).

<font color="red"><b>NOTE:</b></font>  If x<sub>1</sub> and/or y<sub>1</sub> are ever comparable in size to Z &#8212; which may be the case for large apertures or for apertures tilted by nearly 90&deg; to the image screen &#8212; then the variation of L with image screen position cannot be ignored and, accordingly, the coefficient A<sub>0</sub> cannot be moved outside of the double summation.

==Analytic Results==
Now, as in [[Appendix/CGH/ParallelApertures#Parallels_With_Example_.232|&sect;I.A]], we would like to consider the case where the rectangular aperture is divided into an infinite number of divisions in both the X and Y dimensions and convert the summations in this last expression into integrals whose limits in both directions are given by the edges of the aperture.  If we specifically consider the case where the aperture is assumed to be uniformly bright (''i.e.,'' a<sub>jk</sub>  = a<sub>0</sub> dX DY, and a<sub>0</sub> is the brightness per unit area), and the phase <math>~\phi_{jk} = 0</math> at all locations on the aperture, we can write,
<table border="0" cellpadding="5" align="center">

<tr>
  <td align="right">
<math>~A(x_1, y_1)</math>
  </td>
  <td align="center">
<math>~\approx</math>
  </td>
  <td align="left">
<math>~ A_0 a_0 \iint \exp\biggl\{ -i \biggl[ \frac{2\pi(x_1 X_j + y_1Y_k}{\lambda L} \biggr] \biggr\} dX dY
</math>
  </td>
</tr>

<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~ A_0 a_0 
\int \exp\biggl\{ -i \biggl[ \frac{2\pi x_1 X_j }{\lambda L} \biggr] \biggr\} dX
\cdot \int \exp\biggl\{ -i \biggl[ \frac{2\pi y_1Y_k}{\lambda L} \biggr] \biggr\} dY
\, .
</math>
  </td>
</tr>
</table>

Both of these integrals can be completed in the same fashion as described in [[Appendix/CGH/ParallelApertures#Parallels_With_Example_.232|&sect;I.A]] for the 1D slit, giving,
<table border="0" cellpadding="5" align="center">

<tr>
  <td align="right">
<math>~A(x_1, y_1)</math>
  </td>
  <td align="center">
<math>~\approx</math>
  </td>
  <td align="left">
<math>~ A_0 a_0 (wh) e^{-i\Theta_1} ~ e^{-i\vartheta_1} \mathrm{sinc}(\alpha_1) \mathrm{sinc}(\beta_1)
\, ,
</math>
  </td>
</tr>
</table>
where,
<table border="0" cellpadding="5" align="center">

<tr>
  <td align="right">
<math>~\alpha_1</math>
  </td>
  <td align="center">
<math>~\equiv </math>
  </td>
  <td align="left">
<math>~\frac{\pi x_1 (X_1 - X_2)}{\lambda L}= \frac{\pi x_1 h}{\lambda L} \, ,</math>
  </td>
</tr>

<tr>
  <td align="right">
<math>~\Theta_1</math>
  </td>
  <td align="center">
<math>~\equiv </math>
  </td>
  <td align="left">
<math>~\frac{\pi x_1 (X_1 + X_2)}{\lambda L} \, ,</math>
  </td>
</tr>

<tr>
  <td align="right">
<math>~\beta_1</math>
  </td>
  <td align="center">
<math>~\equiv </math>
  </td>
  <td align="left">
<math>~\frac{\pi y_1 (Y_1 - Y_2)}{\lambda L}= \frac{\pi y_1 w}{\lambda L} \, ,</math>
  </td>
</tr>

<tr>
  <td align="right">
<math>~\vartheta_1</math>
  </td>
  <td align="center">
<math>~\equiv </math>
  </td>
  <td align="left">
<math>~\frac{\pi y_1 (Y_1 + Y_2)}{\lambda L} \, .</math>
  </td>
</tr>
</table>

It is worth noting that this derivation closely parallels the one presented in &sect;8.5.1 (p. 393) of Born &amp; Wolf (1980) (see the [[#See_Also|reference below]]).  Specifically, our double-integral expression is identical to the "Fraunhofer diffraction integral" written down by Born &amp; Wolf at the beginning of their &sect;8.5.1; and if we follow Born &amp; Wolf's lead and position the origin of our coordinate system at the center of the rectangle, then <math>~\Theta_1 = \vartheta_1 = 0</math> and the intensity <math>~I(P)</math> at point <math>~P</math> that is given by their equation (1) precisely matches the expression for the square of the amplitude, <math>~A^*A(x_1, y_1)</math>, that is obtained from our last expression.

=See Also=
* Updated [[Appendix/Ramblings#Computer-Generated_Holography|Table of Contents]]
* Born, M. and Wolf, E. (1980) ''Principles of Optics,'' 3<sup>rd</sup> Edition.  New York:  Pergamon Press.  [See especially their &sect;&sect;8.5 and 8.10.]  A link to the 6<sup>th</sup> edition of this book can be found [https://www.sciencedirect.com/book/9780080264820/principles-of-optics here].


{{ SGFfooter }}