The frequency domain by HC121001044621


									                Frequency Domain

•The frequency domain
- the goal is to represent an image as a weighted sum
of sinusoidal functions
-a periodic function - a sinusoid function
-images of sinusoidal functions
What do we mean by the term “ Frequency Domain”?
 We can visualize&analyze a signal or a filter in either the
 spatial domain or the frequency domain

 Spatial domain: x, distance ( usually in pixels)
 Frequency domain: can be measured with either:
 -, angular frequency in radians per unit distance,or
 -f, rotational frequency in cycles per unit distance. =2f
 The period of a signal, T=1/f= 2/ 
 The signal [0 1 0 1 0 1…] has frequency f=.5 (.5 cycles per sample)
                       Frequency Domain
 The frequency domain is a space in which each image value at
 image position F represents the amount that the intensity values in
 image I vary over a specific distance related to F. In the frequency
 domain, changes in image position correspond to changes in the
 spatial frequency, (or the rate at which image intensity values)
 are changing in the spatial domain image I.

   For example, suppose that there is the value 20 at the point that
   represents the frequency 0.1 (or 1 period every 10 pixels). This
   means that in the corresponding spatial domain image I the
   intensity values vary from dark to light and back to dark over a
   distance of 10 pixels, and that the contrast between the lightest
   and darkest is 40 gray levels (2 times 20).
In most cases, the Fourier Transform is used to convert images
from the spatial domain into the frequency domain and vice-versa.
                            Spatial Domain
The spatial domain is the normal image space, in which a change in
position in image I directly projects to a change in position in scene S.
Distances in I (in pixels) correspond to real distances (e.g. in meters) in
We can also discuss the frequency with which image values change, that
is, over how many pixels does a cycle of periodically repeating intensity
variations occur. One would refer to the number of pixels over which a
pattern repeats (its periodicity) in the spatial domain.
A related term used in this context is spatial frequency, which refers to
the (inverse of the) periodicity with which the image intensity values
change. Image features with high spatial frequency (such as edges) are
those that change greatly in intensity over short image distances.
The spatial frequency domain is interesting because: 1) it may make
explicit periodic relationships in the spatial domain, and 2) some image
processing operators are more efficient or indeed only practical when
applied in the frequency domain.
                    Spatial frequency

Frequency has a precise meaning when we consider periodic
functions. A periodic function such as the sinusoid is Figure 8.1 (
page 189) consists of fixed pattern or cycle that repeats endlessly
in both directions. The length of this cycle , L , is known as the
period of the function . The frequency of variation is the
reciprocal of the period. If the variation is spatial and L is a
distance, then 1/L is termed the spatial frequency of the variation.
A periodic variation is characterized by two further parameters: an
amplitude and a phase. The amplitude ( labeled A is the size of the
variation- the height of a peak or dept of a trough. The phase ( ) is
the position of the start of a cycle , relative to some reference point
( the origin) A sine function has  =0, whereas a cosine function
has  = /2
                    Spatial frequency

* period - length of the cycle, L
* frequency - 1/L
* if L is a distance, 1/L is the spatial frequency
* amplitude - height of the peak, A
* phase - position of the start of a cycle
     A periodic function - a sinusoid function
 A function f(x) is said to be periodic with period p if

for n = 1, 2, .... For example, the sine function , is
periodic with period (as well as with period , , , etc.).
       A periodic function - a sinusoid function
One of the basic trigonometric functions encountered in trigonometry.
Let be an angle measured counterclockwise from the x-axis along the arc
of the unit circle Then is the vertical coordinate of the arc endpoint. As a
result of this definition, the sine function is periodic with period . By the
Pythagorean theorem , also obeys the identity
                    sin 2      c os2   1
The definition of the sine function can be extended to complex
arguments z using the definition
                               iz
                                       where e is the base of the
                 e e
  sin z                               natural logarithm and i is the
                        2i             imaginary number

The sine function can be defined algebraically by the infinite sum
              Images of sinusoidal functions
We can present image using sinusoidal variation of the x axis,
about a mean gray level of 128. Amplitude, A is a value in the
range [1,127], N is the width of the image, in pixels. The parameter
u is a dimensionless spatial frequency, corresponding to the
number of complete cycles of the sinusoid that fit into the width of
the image
             f ( x, y )  128  A sin(                   )
                                               N 1

  - u is the spatial frequency - number of cycles that fit into the
  width of the image
   - u/N is cycles per pixel -
            Images of sinusoidal functions

Of course, we can also have sinusoidal variation in the y
direction. We can introduce a second spatial frequency
parameter , v, representing the number of cycles of
variation that span the height of the image, to deal with this.
           Fourier theory- Basic concepts

Basic concepts:
- any periodic function can be represented as a sum of simple
- basis functions - sine and cosine functions of a given frequency
- Fourier series - weighted sum of basis functions - equation 8.2
on is the frequency of a basis function - number of cycles that fit
into one period L
- Fourier series representation of f(x) can be given by two 1D
arrays (of infinite size) of coefficients
- Fourier coefficients - weighting factors for each sine and cosine
- example - summation of sinusoids can generate
           Fourier theory- Basic concepts

 A set of sine and cosine functions having particular
frequencies are chosen for image representation. These
are termed the basis functions of the representation. A
weighted sum of these basic functions is called a Fourier
series. The weighting factors for each sine and cosine
function are known as the Fourier coefficients. We can
write the summation as 2nx 
                             follows:         2nx 
         f ( x)   a n cos        bn sin       
                  n 0      L               L 

        The index n is the number of cycles of the sinusoid that
        fit within a one period of f(x). Thus n can be considered
        as a dimensionless measure of the frequency of a basis
                       2D Fourier series
1)use 2D sine and cosine functions - equation 8.3
2)Fourier series representation of f(x,y) can be given by two 2D
arrays (of infinite size) of coefficients
3)basis images - figure 8.7
4)coefficients determine contributions of each basis image to the
5) Fourier series
                          2D Fourier series

                 
                            2 (ux  vy )               2 (ux  vy ) 
  f ( x, y )   au ,v cos                 bu ,v sin                
               u 0 v 0         L                           L        

where u and v are the number of cycles fitting into one
horizontal and vertical period , respectively of f(x,y). We can
regard the Fourier series representation of f(x,y) as a pair of
two-dimensional arrays of coefficients, each of infinite extent.

The Fourier series can be used to represent any image. We can
visualize the basis function as “basic images” – see Figure 8.7.
The coefficients au,v and bu,v determine the relative
contributions of each basis image to the representation
                     2D Fourier series
 Fourier series are expansions of periodic functions f(x) in
 terms of an infinite sum of sines and cosines.

Fourier series make calculate the coefficients and in the sum.
The computation and use of the orthogonality relationships of
the sine and cosine functions, which can be used to study of
Fourier series is known as harmonic analysis.

   Two functions f(x) and g(x) are orthogonal on the
interval               if
                    Fourier Transform
 The Fourier Transform is an important image processing tool which
is used to decompose an image into its sine and cosine components.
The output of the transformation represents the image in the Fourier
or frequency domain, while the input image is the spatial domain
equivalent. In the Fourier domain image, each point represents a
particular frequency contained in the spatial domain image.
The Fourier Transform is used in a wide range of applications, such
as image analysis, image filtering, image reconstruction and image
The original curve has been sampled over 512
points, which means that, according to the theory we
can simulate it with the sum of 256 sine wave, which
can have any amplitude and any phase difference
from the original signal. The first of the sine waves
has a frequency of 0 which means it is just a straight
line and this always has the average value of the
signal. The second has a frequency 1 (i.e. there is one
wave in the original length of the signal). This has
been drawn so that it starts and finishes at 0 but it
can be moved to the left or right by any distance
required to make it fit. The peak to peak height can
also take on any value. The third sine wave has a
frequency of two etc. The FFT software calculates
the set of these waves with frequencies from 0 to 255
which will add up to give exactly the original wave.
The result is a list of 256 pairs of numbers: we
already know the frequencies (the first is 0 the
second 1 etc) so these pairs of numbers are just the
amplitude of each sine wave and the phase shift
which must be applied to make it fit. This all the
information we need to recreate the original
waveform but before we do that we can filter it by
editing the numbers.
           Discrete Fourier Transform (DFT)
   When applying Fourier transform to images, we must deal explicitly
   with the fact that an image is :
   1)   Two –dimensional
   2)   Sampled
   3) Of finite extent
The DFT is the sampled Fourier Transform and therefore does not
contain all frequencies forming an image, but only a set of samples
which is large enough to fully describe the spatial domain image. The
number of frequencies corresponds to the number of pixels in the spatial
domain image, i.e. the image in the spatial and Fourier domain are of the
same size.
For a square image of size N×N, the two-dimensional DFT is given by:
            1 N 1 N 1    2 (ux  vy          2 (ux  vy) 
  F (u, v)   f ( x, y)cos             j sin              
            N x 0 y 0         N                    N       
    Discrete Fourier Transform (DFT) – How is works
   Noting that  e  cos( )  j sin  )                         Euler’s formula
and DFT can be written is exponential form:
                          N 1 N 1
  F (u , v ) 
                          x 0 y 0
                                      f ( x, y )e  j 2 ( ux  v y ) / N

where f(x,y) is the image in the spatial domain and the exponential
term is the basis function corresponding to each point F(u,v) in the
Fourier space. The equation can be interpreted as: the value of each
point F(u,v) is obtained by multiplying the spatial image with the
corresponding base function and summing the result.
The basis functions are sine and cosine waves with increasing
frequencies, i.e. F(0,0) represents the DC-component of the image
which corresponds to the average brightness and F(N-1,N-1)
represents the highest frequency.
                                  Math Review
Most functions ( including sine, cosine and ex) can be represented as
an infinite sun of polynomial terms
                      x2   x3   x5   x6   x7
          ex  1 x                      ......
                      2!   3!   5!   6!   7!
                                     3
                                                 5
                                                             7
         s in( )                                             .....
                                   3!         5!           7!
                                     2
                                                 4
                                                             6
         cos ( )  1                                            ....
                                   2!         4!           6!
Letting x= j, Euler’s formula becomes obvious to the most casual
observer:        2     3    5     6   7
                 x      x    x     x      x
  e  1 x 
                                          ......
                 2!     3!    5!    6!    7!
                ( j ) 2 ( j ) 3 ( j  ) 4 ( j  ) 5 ( j ) 6 ( j ) 7
   1  (i )                                                      ..
                   2!        3!        4!        5!      6!       7!
         2       4       6                     3       5         7
   1                         ...  j (                             ....)
         2!       4!       6!                     3!       5!         7!
                   Inverse Fourier transform
   In a similar way, the Fourier image can be re-transformed to the
   spatial domain. The inverse Fourier transform is given by:
                           N 1 N 1
      f ( x, y ) 
                            F (u , v )e j 2 ( ux  vy) / N
                           x 0 y 0

The only material difference is the sigh of the exponent. It is clear
that the forward transform of an N x N image yields an N x N
array of coefficients. Since the inverse transform reconstructs the
original image from this set of coefficients, they must constitute a
complete representation of the information present in the image
                        N 1 N 1
  F (u , v ) 
                        x 0 y 0
                                     f ( x, y )e  j 2 ( ux  v y ) / N

                                    forward transform
                   Fast Fourier Transform
Fourier Transform is separable, it can be written as


   Using these two formulas, the spatial domain image is first
   transformed into an intermediate image using N one-
   dimensional Fourier Transforms. This intermediate image is
   then transformed into the final image, again using N one-
   dimensional Fourier Transforms. Expressing the two-
   dimensional Fourier Transform in terms of a series of 2N
   one-dimensional transforms decreases the number of
   required computations.
              Fast Fourier Transform

 Even with these computational savings, the ordinary
one-dimensional DFT has N2 complexity. This can be
reduced toNLog2N if we employ the Fast Fourier
Transform (FFT) to compute the one-dimensional DFTs.
This is a significant improvement, in particular for large
images. There are various forms of the FFT and most of
them restrict the size of the input image that may be
transformed, often to N=2n where n is an integer.
         Image Transformations – Math Review
 •Let an image f be represented as an M x N matrix of integer


•General transform                                      (2)

can be rewritten as

      Image Transformations - Math Review
•If P and Q are non-singular (non-zero determinants),
inverse matrices exist and


•If P and Q are both symmetric (M=M^T), real, and orthogonal
(M^T M = I), then


       and the transform is an orthogonal transform.
            Fourier transform - Math Review
•Let JJ be a transform matrix of size J x J :


•The discrete Fourier transform can be defined according to equation (2)



 •The kernel function of the discrete transform (.8) is
                The spectra of an image

The Fourier Transform produces a complex number valued
output image which can be displayed with two images,
either with the real and imaginary part or with magnitude
and phase. In image processing, often only the magnitude
of the Fourier Transform is displayed, as it contains most of
the information of the geometric structure of the spatial
domain image. However, if we want to re-transform the
Fourier image into the correct spatial domain after some
processing in the frequency domain, we must make sure to
preserve both magnitude and phase of the Fourier image.
                   The spectra of an image
The result of an FFT is always a complex number. This however, is not
complicated, all it means is that we get a pair of numbers and from this
pair we can calculate the pair of numbers we really want from each
harmonic: the amplitude and phase (often called the modulus and
argument).                  The result of the FFT is a complex
                           C = a + ib illustrated as the point on the
                           diagram. The position of this point can
                           also be described by the distance from
                           the center of the diagram A and the
                           angle  with the real axis. A is
                           amplitude (or modulus) and  is phase
                           (or argument). Simple algebra tells us
          Fourier spectra play an important role
•The Fourier transform of a real function is a complex function

                                                       i ( u ,v )
                                   F (u, v) e
 where R(u,v) and I(u,v) are, respectively, the real and imaginary
                     components of F(u,v).
 •The magnitude function |F(u,v)| is called the frequency
 spectrum of image f(m,n). The magnitudes correspond to
 the amplitudes of the basis images in our Fourier
 representation. The array of magnitudes is termed the
 amplitude spectrum of the image
           Fourier spectra play an important role
  The array of phases is termed the phase spectrum.

  When the term “spectrum” is used on its own, the amplitude
  spectrum is normally implied.

The power spectrum of an image is simply the square of its amplitude
spectrum :
Part 2 ????

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