Entropy and Contrast Enhancement of Infrared Thermal Images Using the Multiscale Top-Hat Transform
Abstract
:1. Introduction
2. Entropy and Contrast in Digital Images
3. Enhancement of Thermal Infrared Images
3.1. Classic Top-Hat Transform
3.2. Modified Top-Hat Transform
3.3. How Entropy is Changed by Top-Hat Transform
- The old value g was unique in the region, with a count of 1, hence it disappears from the region and is replaced by value h. No change in entropy occurs because in the old g bin of the histogram the count of 1 becomes 0, and in the new h bin the count of 0 becomes 1; or
- The old value g existed in k > 1 pixels in the region. In this case the count in the g bin decreases to , and the count in the h bin increases to 1. The following Lemma shows that this change in the histogram increases the region’s entropy.
3.4. Proposed Method Using Multiscale Top-Hat Transform
Algorithm 1 Proposed method for TII Enhancement |
Input:I, G, , n, Output:(Enhanced image) Initialization: G, 1: for to n do 2: Calculation of top-hat transform. (Equation (11)) (Equation (12)) 3: Calculation of subtractions from neighboring scales, obtained through the top-hat transform. The top-hat is subtracted with the previous difference, from the first subtraction of the first neighboring top-hat. 4: end for 5: Calculation of the maximum values of all the multiple scales obtained. (Equation (15)) (Equation (16)) (Equation (17)) (Equation (18)) 6: TII enhancement calculation.The contrast enhancement calculation consists of adding the results of the multiple bright scales to the original image and subtracting the results of the multiple dark scales. (Equation (19)) 7: return |
4. Results and Discussion
- In the first part (Section 4.1) we perform a parameter adjustment to find good parameter values that maximize the entropy of the output image after applying the proposed method.
- Then, in the second part (Section 4.2) we analyze the proposed method per iteration and compare its performance with Multiscale Morphological Infrared Image Enhancement (MMIIE) (mathematical morphology-based multiscale approach) [4].
- Finally, in the last part (Section 4.3), we apply the proposed method and compare the results achieved with the proposed techniques with the following competitive methods from the literature: HE, Contrast Limited Adaptive Histogram Equalization (CLAHE) [51], the method of Kun Liang et al. [6] called IRHE2PL for infrared images, and the MMIIE method for infrared images.
4.1. Parameter Tuning
4.2. Performance of Proposed Method per Iteration
- The Standard Deviation (SD), which quantifies the global contrast of the infrared images, is defined as [16]:
- The metric adopted to measure the signal-to-noise ratio of an image is the PSNR.Given the original infrared image I and the infrared image with enhancement where the size of the images is , the PSNR between I and is given by [30]:The Mean Squared Error (MSE) is defined as:
- The Absolute Mean Brightness Error (AMBE) [11], which quantifies the conservation of the mean brightness of the processed image, is given by:
- The linear blur index [4] is used to measure the performance of the infrared image enhancement. It is defined as follows:
4.3. Comparison of the Performance of the Proposed Method with State of the Art Methods
4.3.1. Analysis of Methods by Scenes
- E metric: The CLAHE method and the proposed method are the methods that have the best performance in terms of entropy for scenes 1 to 8. However, in scene 9 the CLAHE and MMIIE methods have the best results.
- SD metric: The HE, CLAHE, IRHE2PL methods and the proposed method enhance the contrast of the TII in the 9 scenes. The MMIIE method did not enhance the contrast of scenes 2, 4, 7, 8, and 9. The HE method is the best performing method for all scenes and the proposed method is in second place.
- PSNR metric: The methods that produce the less distortion to TII are the IRHE2PL, the proposed method, and CLAHE.
- AMBE metric: For all scenes, the best method in regards to maintaining the average brightness is the proposed method.
- metric: The MMIIE method and the proposed method present the best results in terms of blurring.
4.3.2. General Analysis of Methods
5. Conclusions
Author Contributions
Funding
Conflicts of Interest
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Parameter | Value(s) |
---|---|
n | |
G | |
n | |||||||||
---|---|---|---|---|---|---|---|---|---|
2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | |
0.05 | 6.5931 | 6.5962 | 6.6041 | 6.6188 | 6.6396 | 6.6656 | 6.6950 | 6.7271 | 6.7607 |
0.10 | 6.5971 | 6.6120 | 6.6394 | 6.6777 | 6.7224 | 6.7696 | 6.8174 | 6.8658 | 6.9129 |
0.15 | 6.6037 | 6.6315 | 6.6756 | 6.7326 | 6.7900 | 6.8502 | 6.9100 | 6.9653 | 7.0099 |
0.20 | 6.6145 | 6.6577 | 6.7190 | 6.7861 | 6.8548 | 6.9228 | 6.9848 | 7.0326 | 7.0593 |
0.25 | 6.6242 | 6.6821 | 6.7540 | 6.8316 | 6.9081 | 6.9788 | 7.0349 | 7.0661 | 7.0648 |
0.30 | 6.6293 | 6.6970 | 6.7790 | 6.8678 | 6.9498 | 7.0185 | 7.0633 | 7.0702 | 7.0348 |
0.35 | 6.6430 | 6.7217 | 6.8089 | 6.9025 | 6.9851 | 7.0475 | 7.0740 | 7.0519 | 6.9828 |
0.40 | 6.6518 | 6.7420 | 6.8398 | 6.9380 | 7.0181 | 7.0673 | 7.0688 | 7.0161 | 6.9169 |
0.45 | 6.6568 | 6.7545 | 6.8607 | 6.9637 | 7.0394 | 7.0735 | 7.0505 | 6.9706 | 6.8448 |
0.50 | 6.6806 | 6.7872 | 6.8957 | 6.9957 | 7.0596 | 7.0726 | 7.0225 | 6.9165 | 6.7668 |
0.55 | 6.6824 | 6.7928 | 6.9068 | 7.0085 | 7.0647 | 7.0610 | 6.9900 | 6.8619 | 6.6915 |
0.60 | 6.6914 | 6.8113 | 6.9314 | 7.0295 | 7.0702 | 7.0450 | 6.9516 | 6.8011 | 6.6111 |
0.65 | 6.6945 | 6.8201 | 6.9451 | 7.0404 | 7.0682 | 7.0249 | 6.9112 | 6.7406 | 6.5330 |
0.70 | 6.7066 | 6.8408 | 6.9655 | 7.0516 | 7.0631 | 7.0010 | 6.8676 | 6.6786 | 6.4556 |
0.75 | 6.7161 | 6.8588 | 6.9835 | 7.0602 | 7.0550 | 6.9745 | 6.8216 | 6.6152 | 6.3778 |
0.80 | 6.7221 | 6.8707 | 6.9979 | 7.0639 | 7.0433 | 6.9462 | 6.7747 | 6.5531 | 6.3032 |
0.85 | 6.7259 | 6.8791 | 7.0077 | 7.0650 | 7.0303 | 6.9167 | 6.7289 | 6.4929 | 6.2319 |
0.90 | 6.7309 | 6.8906 | 7.0183 | 7.0641 | 7.0140 | 6.8843 | 6.6802 | 6.4311 | 6.1612 |
0.95 | 6.7326 | 6.8959 | 7.0235 | 7.0604 | 6.9973 | 6.8515 | 6.6320 | 6.3702 | 6.0927 |
1.00 | 6.7791 | 6.9368 | 7.0460 | 7.0610 | 6.9780 | 6.8134 | 6.5783 | 6.3055 | 6.0210 |
n | Proposed Method | MMIIE | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
E | SD | PSNR | AMBE | Time (ms) | E | SD | PSNR | AMBE | Time (ms) | |||
2 | 6.643 | 40.835 | 40.417 | 0.129 | 0.332 | 2328 | 6.324 | 30.247 | 16.236 | 38.072 | 0.194 | 454 |
3 | 6.722 | 41.969 | 33.564 | 0.286 | 0.320 | 3752 | 6.447 | 32.069 | 16.176 | 37.775 | 0.193 | 902 |
4 | 6.809 | 43.632 | 29.256 | 0.466 | 0.311 | 6719 | 6.441 | 33.016 | 16.211 | 37.528 | 0.192 | 1605 |
5 | 6.902 | 45.854 | 26.023 | 0.714 | 0.301 | 10,629 | 6.519 | 34.438 | 16.204 | 37.193 | 0.193 | 2759 |
6 | 6.985 | 48.556 | 23.509 | 1.107 | 0.293 | 11,947 | 6.515 | 35.486 | 16.216 | 36.902 | 0.194 | 4770 |
7 | 7.047 | 51.749 | 21.434 | 1.636 | 0.286 | 16,429 | 6.570 | 36.798 | 16.177 | 36.580 | 0.195 | 7187 |
8 | 7.074 | 55.353 | 19.693 | 2.299 | 0.281 | 19,979 | 6.565 | 37.558 | 16.194 | 36.318 | 0.196 | 9255 |
9 | 7.052 | 59.216 | 18.219 | 3.034 | 0.275 | 20,176 | 6.612 | 38.453 | 16.178 | 36.093 | 0.197 | 18,318 |
10 | 6.983 | 63.111 | 16.980 | 3.830 | 0.268 | 21,527 | 6.604 | 39.017 | 16.201 | 35.884 | 0.197 | 20,003 |
Methods | Percentage of Images Improved (%) |
---|---|
HE | 98.89% |
CLAHE | 82.67% |
IRHE2PL | 90.22% |
MMIIE | 47.56% |
Proposed method | 100% |
Methods | E | SD | PSNR | AMBE | ||
---|---|---|---|---|---|---|
Scene 1 | I | 6.814 | 32.336 | - | - | 0.284 |
HE | 6.596 | 73.420 | 11.543 | 48.519 | 0.406 | |
CLAHE | 7.557 | 50.808 | 15.984 | 24.259 | 0.401 | |
IRHE2PL | 6.814 | 36.776 | 29.603 | 7.065 | 0.293 | |
MMIIE | 6.910 | 43.573 | 17.005 | 25.392 | 0.164 | |
Proposed method | 7.418 | 60.136 | 16.767 | 1.887 | 0.273 | |
Scene 2 | I | 7.039 | 55.330 | - | - | 0.454 |
HE | 6.844 | 73.364 | 20.479 | 3.101 | 0.400 | |
CLAHE | 7.500 | 53.721 | 21.237 | 1.657 | 0.488 | |
IRHE2PL | 7.036 | 58.604 | 33.310 | 6.802 | 0.453 | |
MMIIE | 7.038 | 45.486 | 13.085 | 48.345 | 0.273 | |
Proposed method | 7.601 | 69.425 | 18.215 | 1.534 | 0.419 | |
Scene 3 | I | 5.945 | 18.269 | - | - | 0.477 |
HE | 5.881 | 73.063 | 10.789 | 47.807 | 0.408 | |
CLAHE | 6.970 | 32.154 | 19.839 | 18.275 | 0.485 | |
IRHE2PL | 5.945 | 42.197 | 20.011 | 13.270 | 0.326 | |
MMIIE | 6.133 | 20.900 | 17.288 | 32.819 | 0.127 | |
Proposed method | 6.826 | 30.332 | 23.205 | 0.136 | 0.273 | |
Scene 4 | I | 6.808 | 41.521 | - | - | 0.342 |
HE | 6.642 | 73.148 | 12.977 | 41.972 | 0.407 | |
CLAHE | 7.482 | 48.135 | 18.560 | 19.816 | 0.422 | |
IRHE2PL | 6.808 | 56.144 | 22.617 | 11.306 | 0.313 | |
MMIIE | 6.848 | 35.941 | 16.106 | 33.095 | 0.149 | |
Proposed method | 7.566 | 56.723 | 19.019 | 1.328 | 0.312 | |
Scene 5 | I | 7.052 | 40.839 | - | - | 0.356 |
HE | 6.901 | 73.319 | 14.793 | 32.298 | 0.404 | |
CLAHE | 7.620 | 50.630 | 17.786 | 15.352 | 0.433 | |
IRHE2PL | 7.048 | 45.807 | 32.631 | 11.444 | 0.307 | |
MMIIE | 7.025 | 44.123 | 15.660 | 34.956 | 0.173 | |
Proposed method | 7.505 | 61.669 | 17.599 | 2.584 | 0.317 | |
Scene 6 | I | 6.272 | 24.626 | - | - | 0.152 |
HE | 6.158 | 72.882 | 8.091 | 86.636 | 0.408 | |
CLAHE | 7.200 | 42.379 | 16.477 | 31.714 | 0.263 | |
IRHE2PL | 6.272 | 37.308 | 21.316 | 17.733 | 0.179 | |
MMIIE | 6.035 | 28.802 | 21.602 | 15.389 | 0.048 | |
Proposed method | 6.702 | 40.545 | 20.893 | 2.284 | 0.114 | |
Scene 7 | I | 6.990 | 67.015 | - | - | 0.348 |
HE | 6.783 | 73.516 | 18.535 | 19.921 | 0.398 | |
CLAHE | 7.548 | 66.298 | 19.828 | 7.159 | 0.400 | |
IRHE2PL | 6.987 | 75.173 | 33.982 | 14.009 | 0.295 | |
MMIIE | 7.125 | 53.062 | 12.017 | 54.459 | 0.327 | |
Proposed method | 7.204 | 75.462 | 19.735 | 1.405 | 0.323 | |
Scene 8 | I | 6.219 | 28.522 | - | - | 0.237 |
HE | 6.131 | 72.805 | 8.042 | 89.033 | 0.409 | |
CLAHE | 7.134 | 41.543 | 16.828 | 31.090 | 0.309 | |
IRHE2PL | 6.219 | 62.031 | 11.319 | 60.173 | 0.334 | |
MMIIE | 5.952 | 23.883 | 21.792 | 14.567 | 0.077 | |
Proposed method | 6.589 | 37.486 | 23.014 | 2.426 | 0.118 | |
Scene 9 | I | 6.191 | 53.458 | - | - | 0.448 |
HE | 6.001 | 80.909 | 13.975 | 41.396 | 0.329 | |
CLAHE | 6.459 | 59.638 | 19.045 | 13.075 | 0.440 | |
IRHE2PL | 6.188 | 67.644 | 30.537 | 10.979 | 0.386 | |
MMIIE | 6.438 | 50.305 | 11.052 | 65.813 | 0.433 | |
Proposed method | 6.254 | 66.401 | 18.794 | 7.105 | 0.378 |
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Mello Román, J.C.; Vázquez Noguera, J.L.; Legal-Ayala, H.; Pinto-Roa, D.P.; Gomez-Guerrero, S.; García Torres, M. Entropy and Contrast Enhancement of Infrared Thermal Images Using the Multiscale Top-Hat Transform. Entropy 2019, 21, 244. https://doi.org/10.3390/e21030244
Mello Román JC, Vázquez Noguera JL, Legal-Ayala H, Pinto-Roa DP, Gomez-Guerrero S, García Torres M. Entropy and Contrast Enhancement of Infrared Thermal Images Using the Multiscale Top-Hat Transform. Entropy. 2019; 21(3):244. https://doi.org/10.3390/e21030244
Chicago/Turabian StyleMello Román, Julio César, José Luis Vázquez Noguera, Horacio Legal-Ayala, Diego P. Pinto-Roa, Santiago Gomez-Guerrero, and Miguel García Torres. 2019. "Entropy and Contrast Enhancement of Infrared Thermal Images Using the Multiscale Top-Hat Transform" Entropy 21, no. 3: 244. https://doi.org/10.3390/e21030244
APA StyleMello Román, J. C., Vázquez Noguera, J. L., Legal-Ayala, H., Pinto-Roa, D. P., Gomez-Guerrero, S., & García Torres, M. (2019). Entropy and Contrast Enhancement of Infrared Thermal Images Using the Multiscale Top-Hat Transform. Entropy, 21(3), 244. https://doi.org/10.3390/e21030244