We started by obtaining a set of 22 images which
were taken using different lighting conditions. The position of the camera
was kept constant during the acquisition of the images. As you can see, the
training set has a hide variety of lighting conditions.

The input images were normalized using two different mean and standard
deviation. The following pictures show the mean image obtained using the
values bellow. The picture on the left is less vulnerable to light changes.
On the other hand, the one on the right gives a more clear image.
mean =
100 std = 80 mean = 100 std = 100

The tests that were carried were performed using the
second case (100,100). Bellow is an explanation of the type of changes that
were made to the original model and the results obtained. You can click on
the image number to see the input image.
|
Test # |
Description of the change made to model |
Max distance |
Min distance |
|
1 |
1 small pin was removed (Upper left) |
39253 |
36720 |
|
2 |
2 small pins were removed |
40539 |
37848 |
|
3 |
4 small pins were removed |
48114 |
44846 |
|
4 |
1 white pin, 1 small pin (upper right) |
47576 |
44556 |
|
5 |
2 white pins (upper left and right) |
49145 |
46473 |
|
6 |
Lights off |
52783 |
49967 |
|
7 |
1 blue rod was removed (lower right) |
48300 |
45623 |
|
8 |
1 small pin was added (middle) |
47640 |
44640 |
|
9 |
1 white star was removed (left) |
47725 |
44506 |
|
10 |
1 blue star replaced the white one |
47361 |
44178 |
|
11 |
2 white pins were replaced with 2 gray ones (bottom) |
48378 |
45285 |
|
12 |
1 white star was removed (lower right) |
47559 |
44394 |
|
13 |
4 green small pins were changed by black ones |
48321 |
45077 |
|
14 |
1 orange bar was added (lower right) |
47602 |
44349 |
|
15 |
1 piece was removed from the right edge |
47507 |
44123 |
|
16 |
same as 15 but with different background color |
47507 |
44123 |
|
17 |
upper right corner was substituted by a different one |
48037 |
44746 |
|
18 |
upper right corner was removed |
47802 |
44482 |
|
19 |
3 red pieces representing fire were added (middle right) |
47890 |
44860 |
|
20 |
2 fires in the middle section |
48034 |
44834 |
|
21 |
1 white pin was added in the middle section |
52800 |
50266 |
|
22 |
1 piece was removed from the buttom edge |
47865 |
44633 |
| |
|
|
|
|
23 |
traiming set image # 3 |
37875 |
34749 |
|
24 |
traiming set image # 18 |
40657 |
34703 |
|
25 |
traiming set image # 21 |
39296 |
36349 |
| |
|
|
|
|
26 |
images not in the training set |
48346 |
45430 |
|
27 |
images not in the training set |
48168 |
43624 |
|
28 |
images not in the training set |
50923 |
46194 |
These images will give you the overall
idea of how the tests were performed.









Discussion:
The first 22 images agree with what was expected; as more parts are removed,
the Euclidian distance increases. Images 19 and 20 simulate a case when fire
occurs. When looking at input images that are within the training set, 2 out
of the three images (23-25) are greater than the maximum expected value of
39253. This value was chosen based on the results of the first input image.
We should note that they were performed under different lighting conditions.
Finally, if the images are not within the training set (26-28) the distance
is considerably higher, even though they didn't have any defects. One
of the explanations, is that the shadow of the wall is sufficiently
different from the images in the training set, yielding a large Euclidian
distance.
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