Digital Signal Processing Reference
In-Depth Information
Fig. 3.12
Measured point spread functions for conventional imaging and imaging with a cubic
phase. PSFs for conventional system at (a) 113” (2870 mm), (b) 146.5” (3721 mm), and (c) 180”
(4572 mm). (d)-(f) PSFs for a system with cubic phase at the same distances for (a)-(c)
ˆ
ˆ
of the signal-to-noise ratio, and the functions
Φ
N
are the expected power
spectra of the object and noise, respectively. The optical transfer function is usually
estimated from the experimentally measured point responses. One can view the
estimated
i
p
(
Φ
L
and
x
,
y
)
as a diffraction limited response. Eq. (
3.18
) can be written in
matrix notation as
i
p
=
Wi
=
WHo
g
,
(3.20)
where
i
p
is the
N
2
×
1 column vector corresponding to array
i
p
(
x
,
y
)
and
W
is the
N
2
N
2
. The issue
we address in the remainder of this chapter is with what fidelity can one estimate
i
p
using less than
N
2
×
convolution matrix corresponding to the Wiener filter
w
(
x
,
y
)
measurements of
i
.
3.4.2
Accelerated Imaging with Extended Depth-of-Field
Since the objective is to form mmW images with reduced number of samples,
the following sampling strategy was proposed in [104]. Because the sensor is a
Search WWH ::
Custom Search