rayleigh_sommerfeld_conv¶
- dnois.optics.df.rayleigh_sommerfeld_conv(pupil: Tensor, wl: Real | Sequence[Real] | Tensor = None, distance: Real | Sequence[Real] | Tensor = None, dx: float | Tensor = None, dy: float | Tensor = None, **kwargs) Tensor ¶
Computes Fresnel diffraction integral using convolution method:
\[\begin{split}U'(x,y)&=-\frac{1}{2\pi}\iint U(u,v)\pfrac{}{d}\frac{\e^{\i kr_d}}{r_d}\d u\d v\\ &=-\frac{1}{2\pi}U(x,y)\ast\pfrac{}{d}\frac{\e^{\i kr}}{r}\\ &=U(x,y)\ast\frac{z}{2\pi r^2}(\frac{1}{r}-\i k)\e^{\i kr}\end{split}\]where \(U\) and \(U'\) are the complex amplitude on source and target plane, respectively, \(d\) is the distance between two planes, \(r=\sqrt{x^2+y^2+d^2}\), \(\lambda\) is wavelength, \(k=2\pi/\lambda\) and \(\ast\) represents convolution.
Note that some intermediate computational steps don’t depend on
pupil
and pre-computing their results can avoid repeated computation if this function is expected to be called multiple times, as long as the arguments other thanpupil
don’t change. This can be done by callinginit_rayleigh_sommerfeld_conv()
and passing its return value asintermediate
argument. In this case,wl
,distance
,dx
anddy
cannot be passed. If all of them are given,intermediate
will be ignored anyway.- Parameters:
pupil (Tensor) – Pupil function \(U\). A tensor of shape \((\cdots,N_d,N_\lambda,H,W)\).
wl (float, Sequence[float] or Tensor) – Wavelengths \(\lambda\). A scalar or a tensor of shape \((N_\lambda,)\).
distance (float, Sequence[float] or Tensor) – Propagation distance \(d\). A scalar or a tensor of shape \((N_d,)\).
dx (float or Tensor) – Grid spacing in horizontal direction to ensure correct scale for DFT. A scalar or a tensor of shape \((\cdots,N_d,N_\lambda)\). Default: ignored.
dy (float or Tensor) – Grid spacing in vertical direction, similar to
dx
. Default: same asdx
. Note thatdy
will be also ignored ifdx
isNone
even thoughdy
is given.kwargs –
Optional keyword arguments:
Parameter
Type
Description
ksize
int | tuple[int, int]
Spatial dimension of the kernel function in vertical and horizontal directions. Default: identical to that of
pupil
.padding
int | str
See
dconv()
. Default:linear
.dft_scale
bool
Whether to apply DFT-scale. See Fourier transform. Default:
True
.short_wl
bool
Whether to ignore \(\frac{1}{r}\) term in kernel function. Default:
True
.intermediate
dict
Cached intermediate results returned by
init_rayleigh_sommerfeld_conv()
. This can be used to speed up computation. Default: omitted.
- Returns:
Diffracted complex amplitude \(U'\). A tensor of shape \((\cdots,N_d,N_\lambda,H,W)\).
- Return type:
Tensor