- Open Access
- Total Downloads : 594
- Authors : Garima Goyal, Ajay Kumar Bansal, Manish Singhal
- Paper ID : IJERTV2IS1317
- Volume & Issue : Volume 02, Issue 01 (January 2013)
- Published (First Online): 30-01-2013
- ISSN (Online) : 2278-0181
- Publisher Name : IJERT
- License: This work is licensed under a Creative Commons Attribution 4.0 International License
Impact & Analysis of Hybrid Median Filter on TEM Images
Garima Goyal1, Ajay Kumar Bansal2, Manish Singhal3
1Student-Mtech, 2Department of Electrical Engineering, 3Department of Electronics &
Communication Engineering
1,2, 3Poornima College of Engineering
Abstract:
TEM images are rapidly gaining prominence in various sectors like life sciences, pathology, medical science, semiconductors, forensics, etc. Hence, there is a critical need to know the effect of existing image restoration and enhancement techniques available for TEM images. This paper focuses on Hybrid Median Filter. The simulation is carried on greyscale and colored TEM images separately. To do so different types of noise (Gaussian Noise, Salt & Pepper Noise, Salt & Pepper Noise & Poisson Noise) is incorporated into image. Each degraded image is denoised by filters. The result is analyzed on the basis of four parameters namely mean of the image, mean square error, signal to noise ratio, peak signal to noise ratio respectively. This paper also notices the effect on TEM image with changing window size of hybrid median filter.
Keywords: TEM Image, Hybrid Median Filter, Noise, Window size
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Introduction
TEMs are capable of imaging at a significantly higher resolution than light microscopes, owing to the small de Broglie wavelength of electrons. This enables the instrument's user to examine fine detail even as small as a single column of atoms, which is tens of thousands times smaller than the smallest resolvable object in a light microscope. TEM forms a major analysis method in a range of scientific fields, in both physical and biological sciences. At smaller magnifications TEM image contrast is due to absorption of electrons in the material, due to
the thickness and composition of the material. At higher magnifications complex wave interactions modulate the intensity of the image, requiring expert analysis of observed images.
Compared to the vast amount of research in medical imaging modalities such as MRI and CT, the number of scientific papers on electron microscopy applications in the image processing community has been very limited. A microscopy image gets corrupted by noise, which may arise in the process of acquiring the image, or during its transmission, or even during reproduction of the image.
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Hybrid Median Filter
In median filtering, the neighboring pixels are ranked according to brightness (intensity) and the median value becomes the new value for the central pixel. Median filters can do an excellent job of rejecting certain types of noise, in particular, shot or impulse noise in which some individual pixels have extreme values. Median filters can tend to erase lines narrower than ½ the width of the neighborhood. They can also round off corners.
Hybrid median filters can get around these problems. The hybrid median filter is a three step ranking process that uses two subgroups of a 5×5 neighborhood. These subgroups are drawn from pixels parallel to the image frame edges, and at 45º to the edges, centered on the reference pixel [6].
B = hmf(A,n) performs hybrid median filtering of the matrix A using a n x n box. Hybrid median filter preserves edges
better than a square kernel median filter because it is a three-step ranking operation: data from different spatial directions are ranked separately[3]. Three median values are calculated: MR is the median of horizontal and vertical R pixels, and MD is the median of diagonal D pixels. The filtered value is the median of the two median values and the central pixel C: median([MR,MD,C]) [5]. As an example, for n = 5:
Fig 1. Median Calculation
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Noise in TEM Image
Noise is defined as an unwanted component of the image. Noise occurs in images for many reasons. Noise can generally be grouped into two classes, independent noise & the noise which is dependent on the image data.
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Gaussian Noise
Gaussian noise is characterized by adding to each image pixel a value from a zero-mean Gaussian distribution. The zero mean property of the distribution allows such noise to be removed by locally averaging pixel values [1]. Noise is modelled as additive white Gaussian noise (AWGN), where all the image pixels deviate from their original values following the Gaussian curve. That is, for each image pixel with intensity value Oij (1 i M, 1 j N for an M x N image), the corresponding pixel of the noisy image Xij is given by,
Xij=Oij+Gij (1)
where, each noise value G is drawn from a zero mean Gaussian distribution. Gaussian noise can be reduced using a spatial filter. However, it must be kept in mind that when
smoothing an image, we reduce not only the noise, but also the fine-scaled image details because they also correspond to blocked high frequencies.
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Poisson Noise
Poisson noise, is a basic form of uncertainty associated with the measurement of light, inherent to the quantized nature of light and the independence of photon detections. Its expected magnitude is signal-dependent and constitutes the dominant source of image noise except in low-light conditions. The magnitude of poisson noise varies across the image, as it depends on the image intensity [2].
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Salt & Pepper Noise
Another common form of noise is data drop- out noise (commonly referred to as intensity spikes, speckle or salt and pepper noise). Here, the noise is caused by errors in the data transmission. The corrupted pixels are either set to the maximum value (which looks like snow in the image) or have single bits flipped over. In some cases, single pixels are set alternatively to zero or to the maximum value, giving the image a `salt and pepper' like appearance. Unaffected pixels always remain unchanged. The noise is usually quantified by the percentage of pixels which are corrupted [2].
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Speckle noise
Increase in power of signal and noise introduced in the image is of same amount that is why speckle noise is termed as multiplicative noise [3]. It is signal dependent, non-Gaussian & spatially dependent. Due to microscopic variations in the surface, roughness within one pixel, the received signal is subjected to random variations in phase and amplitude. The variations in phase which are added constructively results in strong intensities while other which are added destructively results in low intensities. This variation is called as Speckle [1].
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Working Methodology
The complete simulation is carried in Matlab. Two original microscopic images, one greyscale and one colour, are taken. Noise is added to the original image. Four types of noises are added namely gaussian noise, speckle noise, salt & pepper noise & poisson noise respectively. This distorted image is then filtered using Hybrid Median Filter algorithm and is also analyzed with changing window size as shown in Fig.2.
Original Microscopic Image
Original Microscopic Image
Filtered Image
Filtered Image
Image with Noise
Fig. 2. Working Methodology
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Implementation of Hybrid Median Filter
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For color TEM image
Gaussian Noise
Window Size
Mean
MSE
SNR
PSNR
3
169.716
12.184
26.606
5
169.651
114.814
12.644
27.530
7
169.612
100.183
12.939
28.122
Speckle Noise
3
167.717
13.5681
17.273
36.805
5
167.681
14.1513
17.181
36.622
7
167.645
16.0291
16.909
36.081
Salt & Pepper Noise
3
167.861
23.183
16.111
34.479
5
167.792
16.623
16.832
35.923
7
167.734
14.524
17.124
36.509
Poisson Noise
3
167.736
23.921
16.043
34.343
5
167.695
22.355
16.188
34.636
7
167.655
22.945
16.131
34.523
Table1. Simulation Results with varying Window Size for colored TEM image
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For greyscale TEM image
Gaussian Noise
Window Size
Mean
MSE
SNR
PSNR
3
221.0272
3.57E+03
5.8168
12.6005
5
221.3432
3.46E+03
5.8858
12.7386
7
221.5175
3.39E+03
5.9286
12.8249
Speckle Noise
3
221.8892
3.67E+03
5.7815
12.4893
5
222.1347
3.56E+03
5.8462
12.6212
7
222.3019
3.49E+03
5.8871
12.7043
Salt & Pepper Noise
3
223.7385
3.83E+03
5.723
12.2968
5
224.0137
3.73E+03
5.7825
12.4172
7
224.1967
3.66E+03
5.8205
12.4937
Poisson Noise
3
221.7959
3.66E+03
5.7843
12.4986
5
222.0618
3.55E+03
5.8485
12.6287
7
222.2294
3.48E+03
5.8888
12.7103
Table2. Simulation Results with varying Window Size for greyscale TEM image
As shown in table 1 and table 2 for both type of images for gaussian noise hybrid median filter performed well. Higher kernel size gave the desired performance for salt & pepper noise for both types of images. For speckle noise low size kernel for colored image and higher sized kernel for greyscale image gave the required result. For poisson noise window size=5 gave better performance while for greyscale image window size =7 proved better.
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Conclusion
Simulation results are shown in figure 3which clearly indicates that Hybrid Median Filter not only performed well for salt & pepper noise but also performed well enough on other types of noise.
HYBRID MEDIAN FILTER
Original Image Noisy Image Filtered Image
Greyscale Normal Image
Greyscale Colored Image
Greyscale TEM
Image
Colored TEM
Image
Fig.3. Simulation Results
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REFERENCES
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Charles Boncelet (2005). "Image Noise Models". In Alan C. Bovik. Handbook of Image and Video Processing. Academic Press. ISBN 0-12-119792-1.
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I. Shanthi, Dr. M.L. Valarmathi, Speckle Noise Suppression of SAR color image using Hybrid Median Filter, International Journal of Computer Applications (0975-8887), Volume- 31-No-9, October 2011.
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