Through-Wall Imaging With UWB Radar System - KEMT FEI TUKE
Through-Wall Imaging With UWB Radar System - KEMT FEI TUKE
Through-Wall Imaging With UWB Radar System - KEMT FEI TUKE
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4.3 Highlighting of a Building Contours 70<br />
(r, θ) values defined by each (x, z) map points in the Cartesian image space to<br />
curves (i.e. sinusoids) in the polar Hough parameter space. This point-to-curve<br />
transformation is the HT for straight lines. Resulting peaks in the Hough space<br />
represent a corresponding straight line in the investigated image [58].<br />
The points (x, z) representing the line in Fig. 4.3.1 are transformed in Hough<br />
space into the number of sinusoids shown in Fig. 4.3.2. As can be seen, the<br />
maximum of summed sinusoids represents a peak at (rL, θL) position corresponding<br />
to the line in (X, Z) space. The longer the lines are, the higher the peaks will be.<br />
Lower peaks are considered to be shorter lines and thus are not interesting for our<br />
purpose, because we are looking for long and straight walls.<br />
The main idea of this section is to use the assumed information about the<br />
wall directions, which would considerably reduce falsely detected lines. Almost all<br />
buildings have all walls parallel, or perpendicular to the main outer walls. This<br />
means, that almost all of the walls are perpendicular or parallel to each other in<br />
one building. The radar scan is done alongside the one (or more) outer wall(s), as<br />
it is shown in Fig. 4.3.3 a). Therefore, there is a high probability that peaks in<br />
Hough space representing the scanned walls would be approximately at positions<br />
where the wall angle is equal to:<br />
θw = 0 and ± π<br />
. (4.3.6)<br />
2<br />
as it is shown in Fig. 4.3.3 b).<br />
The easiest way to reduce all of the lines that are not perpendicular, or in<br />
parallel with the wall along which the scan is done, is to clear all points in Hough<br />
space, that are not close to the θw. For that purpose, sharp window functions with<br />
peaks at θw are used. The final window function WH is made up from Hanning<br />
window functions as it is shown in Fig. 4.3.4. The investigated walls from image<br />
IHT in Hough space are then raised up from noise and clutters by window function<br />
WH:<br />
IW HT (r, θ) = IHT (r, θ)WH(r, θ). (4.3.7)<br />
The peaks found in Hough space are then transformed by the Inverse Hough<br />
Transform (IHT) back to the (X, Z) space as a certain number of straight lines:<br />
IF (xT , zT ) = IHT (IW HT (r, θ)). (4.3.8)<br />
These lines could be drawn over the original image, so the wall would be found<br />
much more easy.<br />
The sequence of processing steps from SAR scanning to obtain the final image<br />
with the detected building contours is shown in Fig. 4.3.5.