Past exam of the physics A course of the University of Cambridge / 2014 / Paper 2 / Section B / B9

For time dependence $e^{-i\omega t}$, a scalar Fresnel-Kirchhoff aperture formula for a point-source amplitude $A$ isHere $s=|S-Q|$, $r=|P-Q|$, and $K$ is the obliquity factor, approximately the mean of the incident and outgoing direction cosines measured with the forward aperture normal. The factors describe incident spherical spreading, outgoing spreading and accumulated phase. This is the scalar Kirchhoff aperture approximation; it does not supply an exact electromagnetic edge boundary solution.

In the Fresnel regime, expand path lengths to quadratic order in aperture coordinates while replacing slowly varying amplitude and obliquity factors by their axial values. In the Fraunhofer regime the quadratic aperture phase is negligible, leaving the aperture Fourier transform. For characteristic aperture size $D$, the latter requires $D^2/(\lambda R)\ll 1$ in the relevant finite-source geometry; a lens can supply the Fourier-plane configuration.

For the one-dimensional Cornu construction, put $S,O,P$ on the unobstructed straight ray, with the aperture plane perpendicular at $O$. An element is displaced transversely by $x$, with $|x|\ll a,b$, where $a=SO$ and $b=OP$. A long straight edge or slit makes the other transverse direction separable. Then

For knife-edge diffraction at the fence, the edge is $h=0.5\mathrm{m}$ above the direct ray, with $a=5\mathrm{m}$, $b=45\mathrm{m}$, $\lambda \simeq 0.100\mathrm{m}$, and $R=4.5\mathrm{m}$. The unblocked aperture extends upward from $h$, so its Cornu chord runs from $u_h=h\sqrt{2/(\lambda R)}=1.054$ to infinity. Using $C(\infty )=S(\infty )=1/2$ and normalizing by the full unobstructed chord givesThe approximate chord coordinates are $C=0.775$, $S=0.492$. This is the standard single-knife-edge Fresnel normalization.^[ref]

For geometric spreading in a moving-receiver diffraction measurement, set $b=d$ while retaining $a=5$ and $h=0.5$:Normalized transmission decreases toward the fence. Absolute received intensity initially increases, because the free-space spherical-wave intensity rises as source–receiver distance decreases. In this model it reaches a maximum near $d\simeq 2.3\mathrm{m}$, then falls. The formal paraxial small-$d$ behavior is $I\propto d/(5+d{)}^3$; extrapolation to $d\lesssim h$ is outside the small-angle approximation. The sketch distinguishes the absolute signal from its ratio to the unobstructed signal at each position.