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Course Title: Pattern Recognition & Image Processing
Course Code: CSE-411
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Contents
Source of Image
Noise
Introduction
Simple Images &
Contents
Noise Model
Spatially Independent
Noise Models
Effects of Noise on
Images & Histograms
Spatially Dependent
Noise Models
Estimation of Noise
Parameters
Applicability of
Various Noise
Models
Conclusion
Noise is a disturbance of the image data (projection of
the scene) by image acquisition or the transmission of
images.
We may define noise to be any degradation in the image
signal.
Cleaning an image corrupted by noise is thus an
important area of image restoration.
Noises are mostly implemented in MATLAB.
모바일 이미지
Source of Image Noise
Error occurs in image signal, while an image
is being sent
electronically from one place to another .
Sensor Heat: while clicking an image
ISO Factor: ISO number indicates how quickly
a camera’s sensor absorbs , light , higher ISO
used mare chance of noticeable noise
By memory cell failure.
g ( x, y) = f ( x,
y) + η ( x, y)
f(x, y) = original
image pixel
η(x, y) = noise
term
g(x, y) = resulting
noisy pixel
Simple
Images &
Contents
Consider a noisy image is modelled as follows:
Page 04
Page 03
Page 02
Page 01
Noise Models
There are several ways that noise
can be introduced into an image,
depending on how the image is
created.
Page 02
Page 01
2 Spatially Dependent Noise Model
1 Spatially Independent Noise Models
Page 01
Page 01
Page 02
Spatially Independent Noise Models-
Page 01
Page 02
Page 02
P e r i o d i c N o i s e
Spatially
Dependent Noise
Model
Spatially Independent Noise Models
1 2 3 4 5 6
Gaussian
(Normal)
Impulse
(Salt-and-Pepper)
Uniform
Rayleigh
Gamma
(Erlang)
Exponential
There are many different models for the image noise term η(x, y):
Unifor
m
Impulse
Gamma
Exponenti
al
Rayleig
h
Gaussi
an
Spatially Independent Noise Models
The Gaussian noise, also
called normal noise, is
caused by random
fluctuations in the signal.
Its modeled by random
values added to an image.
Its
probability
density
function
(pdf) is:
Noise Models:
Gaussian
Noise
Figure: PDF of Gaussian Noise
Example of Gaussian Noise.
The Rayleigh distribution
is a continuous probability
distribution for positive
valued random variables.
Rayleigh noise presents in
radar range images.
Its
probability
density
function
(pdf) is:
Noise Models:
Rayleigh
Noise
Figure: Rayleigh Distribution
• mean,  = a+(b/4)1/2
• variance,  = b(4-)/4








azfor
azforeaz
bzp
baz
0
)(
2
)(
/)( 2
Example of Rayleigh Noise.
Gamma noise is the
noise which is occurs
in laser imaging and
can be used for
approximating
diagonal histograms. It
obeys the Gamma
distribution.
Its
probability
density
function
(pdf) is:
Noise Models:
Erlang (Gamma)
Noise
Figure: Gamma Distribution









00
0
)!1()(
1
zfor
zfore
b
za
zp
az
bb
• mean, =b/a;
• variance,  =b/a2
Example of Gamma Noise.
Its
probability
density
function
(pdf) is:
Noise Models:
Exponential
Noise
Figure: PDF of Exponential NoiseThe exponential
distribution is the
probability distribution
that describes the time
relation between events
in a Poisson process. It
is a particular case of
the gamma distribution







00
0
)(
zfor
zforae
zp
az
In exponential noise model when
b=1 it tends to be Erlang noise
model.
• mean, =1/a;
• variance,  =1/a2
Example of Exponential
Noise.
Uniform noise is not often
encountered in real-world
imaging systems, but
provides a useful
comparison with Gaussian
noise. This implies that
nonlinear filters should be
better at removing uniform
noise than Gaussian noise.
Its
probability
density
function
(pdf) is:
Noise Models:
Uniform
Noise
Figure: PDF of Uniform Noise






otherwise
bzafor
abzp
0
1
)(
mean, =(a+b)/2;
variance,  =(b-a)2
/12
Example of Uniform Noise.
Its
probability
density
function
(pdf) is:
Noise Models: Impulse
(Salt and Pepper)
Noise
Figure: PDF of Impulse Noise








otherwise
bzfor
azfor
P
P
zp b
a
0
)(
It known as shot noise, impulse
noise or Spike noise .
Its appearance is randomly
scattered white or black or both
pixel over the image .
There are only two possible values
exists that is a and b
and the probability of each is less
than 0.2 .
Effects of
Noise on
Images &
Histograms
Spatially Dependent Noise Models: Periodic Noise (Example)
Periodic noise
usually arises from
electrical or
electromechanical
interference.
It can be
reduced
significantly
via frequency
domain
filtering.
Estimation of Noise Parameters
0
1
P e r i o d i c
N o i s e :The parameters of this
are estimated by Fourier
spectral components.
O n l y A v a i l i t y
o f I m a g e s :
It estimates the noise of
PDF from small patches
of reasonably constant
gray level.
A v a i l i t y o f
I m a g i n g S y s t e m :
It is the simple way to study the
characteristics of system noise
by acquiring a set of images of
flat environment under uniform
illumination (consistent
background).
Example
Once the PDF model is
determined, estimate the
model parameters
(mean  , variance 𝜎2).
Estimation of Noise Parameters(Contd.)
E x p o n e n t i a l
N o i s e :
Used to model noise in laser
imaging.
A p p l i c a b i l i t y
o f V a r i o u s
N o i s e M o d e l s
U n i f o r m N o i s e :
Used in simulations.
I m p u l s e N o i s e :
Quick transients take place
during imaging.
G a u s s i a n N o i s e :
Electronic circuit noise and sensor
noise due to poor illumination or
high temperature.
R a y l e i g h N o i s e :
Characterize noise in range
imaging.
E r l a n g N o i s e :
Noise in laser imaging.
Conclusion
Therefore, noise is added to the image during image
acquisition and to a lesser or greater extent affects the
image. So, the noise models are an important part of
digital image processing. Without having the knowledge
about these models it is nearly impossible to remove the
noise from the image and perform denoising actions.
Noise

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Noise

  • 1. Course Title: Pattern Recognition & Image Processing Course Code: CSE-411
  • 2. 1 2 3 4 5 6 7 8 9 1 0 Contents Source of Image Noise Introduction Simple Images & Contents Noise Model Spatially Independent Noise Models Effects of Noise on Images & Histograms Spatially Dependent Noise Models Estimation of Noise Parameters Applicability of Various Noise Models Conclusion
  • 3. Noise is a disturbance of the image data (projection of the scene) by image acquisition or the transmission of images. We may define noise to be any degradation in the image signal. Cleaning an image corrupted by noise is thus an important area of image restoration. Noises are mostly implemented in MATLAB.
  • 4. 모바일 이미지 Source of Image Noise Error occurs in image signal, while an image is being sent electronically from one place to another . Sensor Heat: while clicking an image ISO Factor: ISO number indicates how quickly a camera’s sensor absorbs , light , higher ISO used mare chance of noticeable noise By memory cell failure.
  • 5. g ( x, y) = f ( x, y) + η ( x, y) f(x, y) = original image pixel η(x, y) = noise term g(x, y) = resulting noisy pixel Simple Images & Contents Consider a noisy image is modelled as follows:
  • 6. Page 04 Page 03 Page 02 Page 01 Noise Models There are several ways that noise can be introduced into an image, depending on how the image is created.
  • 7. Page 02 Page 01 2 Spatially Dependent Noise Model 1 Spatially Independent Noise Models
  • 8. Page 01 Page 01 Page 02 Spatially Independent Noise Models-
  • 9. Page 01 Page 02 Page 02 P e r i o d i c N o i s e Spatially Dependent Noise Model
  • 10. Spatially Independent Noise Models 1 2 3 4 5 6 Gaussian (Normal) Impulse (Salt-and-Pepper) Uniform Rayleigh Gamma (Erlang) Exponential There are many different models for the image noise term η(x, y):
  • 12. The Gaussian noise, also called normal noise, is caused by random fluctuations in the signal. Its modeled by random values added to an image. Its probability density function (pdf) is: Noise Models: Gaussian Noise Figure: PDF of Gaussian Noise Example of Gaussian Noise.
  • 13. The Rayleigh distribution is a continuous probability distribution for positive valued random variables. Rayleigh noise presents in radar range images. Its probability density function (pdf) is: Noise Models: Rayleigh Noise Figure: Rayleigh Distribution • mean,  = a+(b/4)1/2 • variance,  = b(4-)/4         azfor azforeaz bzp baz 0 )( 2 )( /)( 2 Example of Rayleigh Noise.
  • 14. Gamma noise is the noise which is occurs in laser imaging and can be used for approximating diagonal histograms. It obeys the Gamma distribution. Its probability density function (pdf) is: Noise Models: Erlang (Gamma) Noise Figure: Gamma Distribution          00 0 )!1()( 1 zfor zfore b za zp az bb • mean, =b/a; • variance,  =b/a2 Example of Gamma Noise.
  • 15. Its probability density function (pdf) is: Noise Models: Exponential Noise Figure: PDF of Exponential NoiseThe exponential distribution is the probability distribution that describes the time relation between events in a Poisson process. It is a particular case of the gamma distribution        00 0 )( zfor zforae zp az In exponential noise model when b=1 it tends to be Erlang noise model. • mean, =1/a; • variance,  =1/a2 Example of Exponential Noise.
  • 16. Uniform noise is not often encountered in real-world imaging systems, but provides a useful comparison with Gaussian noise. This implies that nonlinear filters should be better at removing uniform noise than Gaussian noise. Its probability density function (pdf) is: Noise Models: Uniform Noise Figure: PDF of Uniform Noise       otherwise bzafor abzp 0 1 )( mean, =(a+b)/2; variance,  =(b-a)2 /12 Example of Uniform Noise.
  • 17. Its probability density function (pdf) is: Noise Models: Impulse (Salt and Pepper) Noise Figure: PDF of Impulse Noise         otherwise bzfor azfor P P zp b a 0 )( It known as shot noise, impulse noise or Spike noise . Its appearance is randomly scattered white or black or both pixel over the image . There are only two possible values exists that is a and b and the probability of each is less than 0.2 .
  • 19. Spatially Dependent Noise Models: Periodic Noise (Example) Periodic noise usually arises from electrical or electromechanical interference. It can be reduced significantly via frequency domain filtering.
  • 20. Estimation of Noise Parameters 0 1 P e r i o d i c N o i s e :The parameters of this are estimated by Fourier spectral components. O n l y A v a i l i t y o f I m a g e s : It estimates the noise of PDF from small patches of reasonably constant gray level. A v a i l i t y o f I m a g i n g S y s t e m : It is the simple way to study the characteristics of system noise by acquiring a set of images of flat environment under uniform illumination (consistent background).
  • 21. Example Once the PDF model is determined, estimate the model parameters (mean  , variance 𝜎2). Estimation of Noise Parameters(Contd.)
  • 22. E x p o n e n t i a l N o i s e : Used to model noise in laser imaging. A p p l i c a b i l i t y o f V a r i o u s N o i s e M o d e l s U n i f o r m N o i s e : Used in simulations. I m p u l s e N o i s e : Quick transients take place during imaging. G a u s s i a n N o i s e : Electronic circuit noise and sensor noise due to poor illumination or high temperature. R a y l e i g h N o i s e : Characterize noise in range imaging. E r l a n g N o i s e : Noise in laser imaging.
  • 23. Conclusion Therefore, noise is added to the image during image acquisition and to a lesser or greater extent affects the image. So, the noise models are an important part of digital image processing. Without having the knowledge about these models it is nearly impossible to remove the noise from the image and perform denoising actions.