03 the gaussian kernel

3. The Gaussian kernel
Of all things, man is the measure.
Protagoras the Sophist (480-411 B.C.)
3.1 The Gaussian kernel
The Gaussian (better Gaußian) kernel is named after Carl Friedrich Gauß (1777-1855), a
brilliant German mathematician. This chapter discusses many of the attractive and special
properties of the Gaussian kernel.
<< FrontEndVision`FEV`; Show@Import@"Gauss10DM.gif"D, ImageSize -> 280D;
Figure 3.1 The Gaussian kernel is apparent on every German banknote of DM 10,- where it
is depicted next to its famous inventor when he was 55 years old. The new Euro replaces
these banknotes. See also: http://scienceworld.wolfram.com/biography/Gauss.html.
The Gaussian kernel is defined in 1-D, 2D and N-D respectively as
G1 D Hx; sL = 1
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅè!!!!!!!
2 p s
e- x2
ÅÅÅÅÅÅÅÅÅÅÅÅÅ2 s2
, G2 DHx, y; sL = 1
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅ2 ps2 e-
x2 +y2
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅ2 s2
, GND Hx”; sL = 1
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅ
I
è!!!!!!!
2 p sM
N e- »x”÷ »2
The s determines the width of the Gaussian kernel. In statistics, when we consider the
Gaussian probability density function it is called the standard deviation, and the square of it,
s2 , the variance. In the rest of this book, when we consider the Gaussian as an aperture
function of some observation, we will refer to s as the inner scale or shortly scale.
In the whole of this book the scale can only take positive values, s > 0. In the process of
observation s can never become zero. For, this would imply making an observation through
an infinitesimally small aperture, which is impossible. The factor of 2 in the exponent is a
matter of convention, because we then have a 'cleaner' formula for the diffusion equation, as
we will see later on. The semicolon between the spatial and scale parameters is
conventionally put there to make the difference between these parameters explicit.
3. The Gaussian kernel 37

The scale-dimension is not just another spatial dimension, as we will thoroughly discuss in
the remainder of this book.
The half width at half maximum (s = 2
è!!!!!!!!!!!
2 ln 2 ) is often used to approximate s, but it is
somewhat larger:
Unprotect@gaussD;
gauss@x_, s_D :=
1
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅ
s
è!!!!!!!
2 p
ExpA-
x2
ÅÅÅÅÅÅÅÅÅÅÅ
2 s2
E;
SolveA
gauss@x, sD
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅ
gauss@0, sD
==
1
ÅÅÅÅ
2
, xE
88x Ø -s
è!!!!!!!!!!!!!!!!!!!!
2 Log@2D <, 8x Ø s
è!!!!!!!!!!!!!!!!!!!!
2 Log@2D <<
% êê N
88x Ø -1.17741 s<, 8x Ø 1.17741 s<<
3.2 Normalization
The term 1
2 p s
in front of the one-dimensional Gaussian kernel is the normalization
constant. It comes from the fact that the integral over the exponential function is not unity:
Ÿ-¶
¶
e-x2 ê2 s2
„ x =
è!!!!!!!!
2 p s. With the normalization constant this Gaussian kernel is a
normalized kernel, i.e. its integral over its full domain is unity for every s.
This means that increasing the s of the kernel reduces the amplitude substantially. Let us
look at the graphs of the normalized kernels for s = 0.3, s = 1 and s = 2 plotted on the
same axes:
Unprotect@gaussD; gauss@x_, s_D :=
1
s
è!!!!!!!
2 p
ExpA-
x2
2 s2
E;
Block@8$DisplayFunction = Identity<, 8p1, p2, p3< =
Plot@gauss@x, s = #D, 8x, -5, 5<, PlotRange -> 80, 1.4<D & êü
8.3, 1, 2<D;
Show@GraphicsArray@8p1, p2, p3<D, ImageSize -> 400D;
-4 -2 2 4
0.2
0.4
0.6
0.8
1
1.2
-4 -2 2 4
0.2
0.4
0.6
0.8
1
1.2
-4 -2 2 4
0.2
0.4
0.6
0.8
1
1.2
Figure 3.2 The Gaussian function at scales s = .3, s = 1 and s = 2. The kernel is
normalized, so the total area under the curve is always unity.
The normalization ensures that the average graylevel of the image remains the same when
we blur the image with this kernel. This is known as average grey level invariance.
38 3.1 The Gaussian kernel

3.3 Cascade property, selfsimilarity
The shape of the kernel remains the same, irrespective of the s. When we convolve two
Gaussian kernels we get a new wider Gaussian with a variance s2 which is the sum of the
variances of the constituting Gaussians: gnew Hx”; s1
2 + s2
2L = g1 Hx”; s1
2L ≈ g2 Hx”; s2
2L.
s =.; SimplifyA‡
-¶
¶
gauss@a, s1 D gauss@a - x, s2 D „a, 8s1 > 0, s2 > 0<E
‰
- x2
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅ
2 Is1
2 +s2
2 M
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅè!!!!!!!
2 p
è!!!!!!!!!!!!!!!
s1
2
+ s2
2
This phenomenon, i.e. that a new function emerges that is similar to the constituting
functions, is called self-similarity.
The Gaussian is a self-similar function. Convolution with a Gaussian is a linear operation, so
a convolution with a Gaussian kernel followed by a convolution with again a Gaussian
kernel is equivalent to convolution with the broader kernel. Note that the squares of s add,
not the s's themselves. Of course we can concatenate as many blurring steps as we want to
create a larger blurring step. With analogy to a cascade of waterfalls spanning the same
height as the total waterfall, this phenomenon is also known as the cascade smoothing
property.
Famous examples of self-similar functions are fractals. This shows the famous Mandelbrot
fractal:
cMandelbrot = Compile@88c, _Complex<<, -Length@
FixedPointList@#2
+ c &, c, 50, SameTest -> HAbs@#2D > 2.0 &LDDD;
ListDensityPlot@ -Table@cMandelbrot@a + b ID, 8b, -1.1, 1.1, 0.0114<,
8a, -2.0, 0.5, 0.0142<D, Mesh -> False, AspectRatio -> Automatic,
Frame -> False, ColorFunction -> Hue, ImageSize -> 170D;
Figure 3.3 The Mandelbrot fractal is a famous example of a self-similar function. Source:
www.mathforum.org. See also mathworld.wolfram.com/MandelbrotSet.html.

3.4 The scale parameter
In order to avoid the summing of squares, one often uses the following parametrization:
2 s2 Ø t, so the Gaussian kernel get a particular short form. In N
dimensions:GNDHx”, tL = 1
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅHp tLNê2 e- x2
ÅÅÅÅÅÅÅÅt .
It is this t that emerges in the diffusion equation ∑L
ÅÅÅÅÅÅÅ∑t
= ∑2 L
ÅÅÅÅÅÅÅÅÅÅ∑x2 + ∑2 L
ÅÅÅÅÅÅÅÅÅÅ∑y2 + ∑2 L
ÅÅÅÅÅÅÅÅÅÅ∑z2 . It is often referred
to as 'scale' (like in: differentiation to scale, ∑L
ÅÅÅÅÅÅÅ∑t
), but a better name is variance.
To make the self-similarity of the Gaussian kernel explicit, we can introduce a new
dimensionless spatial parameter, xè = x
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅ
s
è!!!!
2
. We say that we have reparametrized the x-axis.
Now the Gaussian kernel becomes: gnHxè; sL = 1
s
è!!!!!!!
2 p
e-xè2
, or gnHxè; tL = 1
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅHp tLNê2 e-xè2
. In
other words: if we walk along the spatial axis in footsteps expressed in scale-units (s's), all
kernels are of equal size or 'width' (but due to the normalization constraint not necessarily of
the same amplitude). We now have a 'natural' size of footstep to walk over the spatial
coordinate: a unit step in x is now s
è!!!!
2 , so in more blurred images we make bigger steps.
We call this basic Gaussian kernel the natural Gaussian kernel gnHxè; sL. The new coordinate
xè = x
s
è!!!!
2
is called the natural coordinate. It eliminates the scale factor s from the spatial
coordinates, i.e. it makes the Gaussian kernels similar, despite their different inner scales.
We will encounter natural coordinates many times hereafter.
The spatial extent of the Gaussian kernel ranges from -¶ to +¶, but in practice it has
negligible values for x larger then a few (say 5) s. The numerical value at x=5s, and the area
under the curve from x=5s to infinity (recall that the total area is 1):
gauss@5, 1D êê N
Integrate@gauss@x, 1D, 8x, 5, Infinity<D êê N
1.48672 µ 10-6
2.86652 µ 10-7
The larger we make the standard deviation s, the more the image gets blurred. In the limit to
infinity, the image becomes homogenous in intensity. The final intensity is the average
intensity of the image. This is true for an image with infinite extent, which in practice will
never occur, of course. The boundary has to be taken into account. Actually, one can take
many choices what to do at the boundary, it is a matter of consensus. Boundaries are
discussed in detail in chapter 5, where practical issues of computer implementation are
discussed.
3.5 Relation to generalized functions
The Gaussian kernel is the physical equivalent of the mathematical point. It is not strictly
local, like the mathematical point, but semi-local. It has a Gaussian weighted extent,
indicated by its inner scale s.
Because scale-space theory is revolving around the Gaussian function and its derivatives as a
physical differential operator (in more detail explained in the next chapter), we will focus
here on some mathematical notions that are directly related, i.e. the mathematical notions
underlying sampling of values from functions and their derivatives at selected points (i.e. that
is why it is referred to as sampling). The mathematical functions involved are the
generalized functions, i.e. the Delta-Dirac function, the Heaviside function and the error
function. In the next section we study these functions in detail.
40 3.4 The scale parameter

Because scale-space theory is revolving around the Gaussian function and its derivatives as a
physical differential operator (in more detail explained in the next chapter), we will focus
here on some mathematical notions that are directly related, i.e. the mathematical notions
underlying sampling of values from functions and their derivatives at selected points (i.e. that
is why it is referred to as sampling). The mathematical functions involved are the
generalized functions, i.e. the Delta-Dirac function, the Heaviside function and the error
function. In the next section we study these functions in detail.
When we take the limit as the inner scale goes down to zero (remember that s can only take
positive values for a physically realistic system), we get the mathematical delta function, or
Dirac delta function, d(x). This function is everywhere zero except in x = 0, where it has
infinite amplitude and zero width, its area is unity.
lims∞0 J 1
2 p s
e- x2
N = dHxL.
d(x) is called the sampling function in mathematics, because the Dirac delta function
adequately samples just one point out of a function when integrated. It is assumed that f HxL
is continuous at x = a:
‡
-¶
¶
DiracDelta@x - aD f@xD „x
f@aD
The sampling property of derivatives of the Dirac delta function is shown below:
‡
-¶
¶
D@DiracDelta@xD, 8x, 2<D f@xD „x
f££
@0D
The delta function was originally proposed by the eccentric Victorian mathematician Oliver
Heaviside (1880-1925, see also [Pickover1998]). Story goes that mathematicians called this
function a "monstrosity", but it did work! Around 1950 physicist Paul Dirac (1902-1984)
gave it new light. Mathematician Laurent Schwartz (1915-) proved it in 1951 with his
famous "theory of distributions" (we discuss this theory in chapter 8). And today it's called
"the Dirac delta function".
The integral of the Gaussian kernel from -¶ to x is a famous function as well. It is the error
function, or cumulative Gaussian function, and is defined as:
s =.; err@x_, s_D = ‡
0
x 1
s
è!!!!!!!
2 p
ExpA-
y2
ÅÅÅÅÅÅÅÅÅÅÅÅ
2 s2
E „y
1
ÅÅÅÅ
2
ErfA
x
ÅÅÅÅÅÅÅÅÅÅÅÅÅè!!!
2 s
E

The y in the integral above is just a dummy integration variable, and is integrated out. The
Mathematica error function is Erf[x].
In our integral of the Gaussian function we need to do the reparametrization x Ø x
s
è!!!!
2
.
Again we recognize the natural coordinates. The factor 1
ÅÅÅÅ2
is due to the fact that integration
starts halfway, in x = 0.
s = 1.; PlotA
1
ÅÅÅÅ
2
ErfA
x
s
è!!!!
2
E, 8x, -4, 4<, AspectRatio -> .3,
AxesLabel -> 8"x", "Erf@xD"<, ImageSize -> 200E;
-4 -2 2 4
x
-0.4
-0.2
0.2
0.4
Erf@xD
Figure 3.4 The error function Erf[x] is the cumulative Gaussian function.
When the inner scale s of the error function goes to zero, we get in the limiting case the so-
called Heavyside function or unitstep function. The derivative of the Heavyside function is
the Delta-Dirac function, just as the derivative of the error function of the Gaussian kernel.
s = .1; PlotA
1
ÅÅÅÅ
2
ErfA
x
s
è!!!!
2
E, 8x, -4, 4<, AspectRatio -> .3,
AxesLabel -> 8"x", "Erf@xD"<, ImageSize -> 270E;
-4 -2 2 4
x
-0.4
-0.2
0.2
0.4
Erf@xD
Figure 3.5 For decreasing s the Error function begins to look like a step function. The Error
function is the Gaussian blurred step-edge.
Plot@UnitStep@xD, 8x, -4, 4<, DisplayFunction -> $DisplayFunction,
AspectRatio -> .3, AxesLabel -> 8"x", "Heavyside@xD, UnitStep@xD"<,
PlotStyle -> Thickness@.015D, ImageSize -> 270D;
-4 -2 2 4
x
0.2
0.4
0.6
0.8
1
Heavyside@xD, UnitStep@xD
Figure 3.6 The Heavyside function is the generalized unit stepfunction. It is the limiting case
of the Error function for lim s Ø 0.
The derivative of the Heavyside step function is the Delta function again:
42 3.5 Relation to generalized functions

D@UnitStep@xD, xD
DiracDelta@xD
3.6 Separability
The Gaussian kernel for dimensions higher than one, say N, can be described as a regular
product of N one-dimensional kernels. Example: g2 DHx, y; s1
2 + s2
2L = g1 D Hx; s1
2L
g1 D Hy; s2
2L where the space in between is the product operator. The regular product also
explains the exponent N in the normalization constant for N-dimensional Gaussian kernels in
(0). Because higher dimensional Gaussian kernels are regular products of one-dimensional
Gaussians, they are called separable. We will use quite often this property of separability.
DisplayTogetherArray@8Plot@gauss@x, s = 1D, 8x, -3, 3<D,
Plot3D@gauss@x, s = 1D gauss@y, s = 1D, 8x, -3, 3<, 8y, -3, 3<D<,
ImageSize -> 440D;
-3 -2 -1 1 2 3
0.1
0.2
0.3
0.4
Figure 3.7 A product of Gaussian functions gives a higher dimensional Gaussian function.
This is a consequence of the separability.
An important application is the speed improvement when implementing numerical separable
convolution. In chapter 5 we explain in detail how the convolution with a 2D (or better: N-
dimensional) Gaussian kernel can be replaced by a cascade of 1D convolutions, making the
process much more efficient because convolution with the 1D kernels requires far fewer
multiplications.
3.7 Relation to binomial coefficients
Another place where the Gaussian function emerges is in expansions of powers of
polynomials. Here is an example:
Expand@Hx + yL30
D
x30
+ 30 x29
y + 435 x28
y2
+ 4060 x27
y3
+ 27405 x26
y4
+ 142506 x25
y5
+
593775 x24
y6
+ 2035800 x23
y7
+ 5852925 x22
y8
+ 14307150 x21
y9
+
30045015 x20
y10
+ 54627300 x19
y11
+ 86493225 x18
y12
+ 119759850 x17
y13
+
145422675 x16
y14
+ 155117520 x15
y15
+ 145422675 x14
y16
+
119759850 x13
y17
+ 86493225 x12
y18
+ 54627300 x11
y19
+ 30045015 x10
y20
+
14307150 x9
y21
+ 5852925 x8
y22
+ 2035800 x7
y23
+ 593775 x6
y24
+
142506 x5
y25
+ 27405 x4
y26
+ 4060 x3
y27
+ 435 x2
y28
+ 30 x y29
+ y30
The coefficients of this expansion are the binomial coefficients Hm
n
L ('n over m'):

ListPlot@Table@Binomial@30, nD, 8n, 1, 30<D,
PlotStyle -> 8PointSize@.015D<, AspectRatio -> .3D;
5 10 15 20 25 30
2.5µ107
5µ107
7.5µ107
1µ108
1.25µ108
1.5µ108
Figure 3.8 Binomial coefficients approximate a Gaussian distribution for increasing order.
And here in two dimensions:
BarChart3D@Table@Binomial@30, nD Binomial@30, mD, 8n, 1, 30<, 8m, 1, 30<D,
ImageSize -> 180D;
0
10
20
30
0
10
20
30
0
1µ1016
2µ1016
0
10
20
30
0
10
20
30
Figure 3.9 Binomial coefficients approximate a Gaussian distribution for increasing order.
Here in 2 dimensions we see separability again.
3.8 The Fourier transform of the Gaussian kernel
We will regularly do our calculations in the Fourier domain, as this often turns out to be
analytically convenient or computationally efficient. The basis functions of the Fourier
transform are the sinusoidal functions eiwx . The definitions for the Fourier transform and
its inverse are:
the Fourier transform: FHwL = 8 f HxL< = 1
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅè!!!!!!!
2 p
Ÿ-¶
¶
f HxL ei w x „ x
the inverse Fourier transform: -1 8FHwL< = 1
2 p
Ÿ-¶
¶
FHwL e-i w x „w
s =.; gauss@w_, s_D =
SimplifyA
1
2 p
IntegrateA
1
s
è!!!!!!!
2 p
ExpA-
x2
2 s2
E Exp@I w xD, 8x, -¶, ¶<E,
8s > 0, Im@sD == 0<E
‰- 1
ÅÅÅÅ2 s2 w2
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅè!!!!!!!
2 p
44 3.7 Relation to binomial coefficients

The Fourier transform is a standard Mathematica command:
Simplify@FourierTransform@gauss@x, sD, x, wD, s > 0D
‰- 1
ÅÅÅÅ2 s2 w2
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅè!!!!!!!
2 p
Note that different communities (mathematicians, computer scientists, engineers) have
different definitions for the Fourier transform. From the Mathematica help function:
With the setting FourierParametersØ{a,b} the discrete Fourier transform computed
by FourierTransform is "##############»b»
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅH2 pL1-a Ÿ-¶
¶
fHtL ei b w t
„t. Some common choices for {a,b}
are {0,1} (default), {-1,1} (data analysis), {1,-1} (signal processing).
In this book we consistently use the default definition.
So the Fourier transform of the Gaussian function is again a Gaussian function, but now of
the frequency w. The Gaussian function is the only function with this property. Note that the
scale s now appears as a multiplication with the frequency. We recognize a well-known fact:
a smaller kernel in the spatial domain gives a wider kernel in the Fourier domain, and vice
versa. Here we plot 3 Gaussian kernels with their Fourier transform beneath each plot:
Block@8$DisplayFunction = Identity<,
p1 = Table@Plot@gauss@x, sD, 8x, -10, 10<, PlotRange -> All,
PlotLabel -> "gauss@x," <> ToString@sD <> "D"D, 8s, 1, 3<D;
p2 = Table@Plot@ gauss@w, sD, 8w, -3, 3<, PlotRange -> All,
PlotLabel -> " gauss@x," <> ToString@sD <> "D"D, 8s, 1, 3<DD;
Show@GraphicsArray@8p1, p2<D, ImageSize -> 400D;
-3 -2 -1 1 2 3
0.1
0.2
0.3
0.4
gauss@x,1D
-3 -2 -1 1 2 3
0.1
0.2
0.3
0.4
gauss@x,2D
-3 -2 -1 1 2 3
0.1
0.2
0.3
0.4
gauss@x,3D
-10 -5 5 10
0.1
0.2
0.3
0.4
gauss@x,1D
-10 -5 5 10
0.05
0.1
0.15
0.2
gauss@x,2D
-10 -5 5 10
0.02
0.04
0.06
0.08
0.1
0.12
gauss@x,3D
Figure 3.10 Top row: Gaussian function at scales s=1, s=2 and s=3. Bottom row: Fourier
transform of the Gaussian function above it. Note that for wider Gaussian its Fourier
transform gets narrower and vice versa, a well known phenomenon with the Fourier
transform. Also note by checking the amplitudes that the kernel is normalized in the spatial
domain only.
There are many names for the Fourier transform gHw; sL of gHx; sL: when the kernel
gHx; sL is considered to be the point spread function, gHw; sL is referred to as the
modulation transfer function. When the kernel g(x;s) is considered to be a signal, gHw; sL
is referred to as the spectrum. When applied to a signal, it operates as a lowpass filter. Let us
plot the spectra of a series of such filters (with a logarithmic increase in scale) on double
logarithmic paper:

There are many names for the Fourier transform gHw; sL of gHx; sL: when the kernel
gHx; sL is considered to be the point spread function, gHw; sL is referred to as the
modulation transfer function. When the kernel g(x;s) is considered to be a signal, gHw; sL
is referred to as the spectrum. When applied to a signal, it operates as a lowpass filter. Let us
plot the spectra of a series of such filters (with a logarithmic increase in scale) on double
logarithmic paper:
scales = N@Table@ Exp@t ê 3D, 8t, 0, 8<DD
spectra = LogLinearPlot@ gauss@w, #D,
8w, .01, 10<, DisplayFunction -> IdentityD & êü scales;
Show@spectra, DisplayFunction -> $DisplayFunction, AspectRatio -> .4,
PlotRange -> All, AxesLabel -> 8"w", "Amplitude"<, ImageSize -> 300D;
81., 1.39561, 1.94773, 2.71828,
3.79367, 5.29449, 7.38906, 10.3123, 14.3919<
0.01 0.05 0.1 0.5 1 5 10
w0
0.1
0.2
0.3
0.4
Amplitude
Figure 3.11 Fourier spectra of the Gaussian kernel for an exponential range of scales s = 1
(most right graph) to s = 14.39 (most left graph). The frequency w is on a logarithmic scale.
The Gaussian kernels are seen to act as low-pass filters.
Due to this behaviour the role of receptive fields as lowpass filters has long persisted. But the
retina does not measure a Fourier transform of the incoming image, as we will discuss in the
chapters on the visual system (chapters 9-12).
3.9 Central limit theorem
We see in the paragraph above the relation with the central limit theorem: any repetitive
operator goes in the limit to a Gaussian function. Later, when we study the discrete
implementation of the Gaussian kernel and discrete sampled data, we will see the relation
between interpolation schemes and the binomial coefficients. We study a repeated
convolution of two blockfunctions with each other:
f@x_D := UnitStep@1 ê 2 + xD + UnitStep@1 ê 2 - xD - 1;
g@x_D := UnitStep@1 ê 2 + xD + UnitStep@1 ê 2 - xD - 1;
Plot@f@xD, 8x, -3, 3<, ImageSize -> 140D;
-3 -2 -1 1 2 3
0.2
0.4
0.6
0.8
1
Figure 3.12 The analytical blockfunction is a combination of two Heavyside unitstep functions.
We calculate analytically the convolution integral
46 3.8 The Fourier transform of the Gaussian kernel

h1 = Integrate@f@xD g@x - x1D, 8x, -¶, ¶<D
1
ÅÅÅÅ
2
H-1 + 2 UnitStep@1 - x1D - 2 x1 UnitStep@1 - x1D - 2 x1 UnitStep@x1DL +
1
ÅÅÅÅ
2
H-1 + 2 x1 UnitStep@-x1D + 2 UnitStep@1 + x1D + 2 x1 UnitStep@1 + x1DL
Plot@h1, 8x1, -3, 3<, PlotRange -> All, ImageSize -> 150D;
-3 -2 -1 1 2 3
0.2
0.4
0.6
0.8
1
Figure 3.13 One times a convolution of a blockfunction with the same blockfunction gives a
triangle function.
The next convolution is this function convolved with the block function again:
h2 = Integrate@Hh1 ê. x1 -> xL g@x - x1D, 8x, -¶, ¶<D
-1 +
1
ÅÅÅÅ
8
H1 - 2 x1L2
+
1
ÅÅÅÅ
8
H1 + 2 x1L2
+
1
ÅÅÅÅ
8
H3 - 4 x1 - 4 x12
L +
1
ÅÅÅÅ
8
H3 + 4 x1 - 4 x12
L +
1
ÅÅÅÅ
8
J-4 + 9 UnitStepA
3
ÅÅÅÅ
2
- x1E - 12 x1 UnitStepA
3
ÅÅÅÅ
2
- x1E + 4 x12
UnitStepA
3
ÅÅÅÅ
2
- x1E +
UnitStepA-
1
ÅÅÅÅ
2
+ x1E - 4 x1 UnitStepA-
1
ÅÅÅÅ
2
+ x1E + 4 x12
UnitStepA-
1
ÅÅÅÅ
2
+ x1EN +
1
ÅÅÅÅ
4
J-UnitStepA
1
ÅÅÅÅ
2
- x1E + 4 x1 UnitStepA
1
ÅÅÅÅ
2
- x1E - 4 x12
UnitStepA
1
ÅÅÅÅ
2
- x1E -
UnitStepA
1
ÅÅÅÅ
2
+ x1E - 4 x1 UnitStepA
1
ÅÅÅÅ
2
+ x1E - 4 x12
UnitStepA
1
ÅÅÅÅ
2
+ x1EN +
1
ÅÅÅÅ
8
J-4 + UnitStepA-
1
ÅÅÅÅ
2
- x1E + 4 x1 UnitStepA-
1
ÅÅÅÅ
2
- x1E +
4 x12
UnitStepA-
1
ÅÅÅÅ
2
- x1E + 9 UnitStepA
3
ÅÅÅÅ
2
+ x1E +
12 x1 UnitStepA
3
ÅÅÅÅ
2
+ x1E + 4 x12
UnitStepA
3
ÅÅÅÅ
2
+ x1EN
-1 +
1
ÅÅÅÅ
8
H1 - 2 x1L2
+
1
ÅÅÅÅ
8
H1 + 2 x1L2
+
1
ÅÅÅÅ
8
H3 - 4 x1 - 4 x12
L +
1
ÅÅÅÅ
8
H3 + 4 x1 - 4 x12
L +
1
ÅÅÅÅ
8
J-4 + 9 UnitStepA
3
ÅÅÅÅ
2
- x1E - 12 x1 UnitStepA
3
ÅÅÅÅ
2
- x1E + 4 x12
UnitStepA
3
ÅÅÅÅ
2
- x1E +
UnitStepA-
1
ÅÅÅÅ
2
+ x1E - 4 x1 UnitStepA-
1
ÅÅÅÅ
2
+ x1E + 4 x12
UnitStepA-
1
ÅÅÅÅ
2
+ x1EN +
1
ÅÅÅÅÅ
4
J-UnitStepA
1
ÅÅÅÅ
2
- x1E + 4 x1 UnitStepA
1
ÅÅÅÅ
2
- x1E - 4 x12
UnitStepA
1
ÅÅÅÅ
2
- x1E -
UnitStepA
1
ÅÅÅÅ
2
+ x1E - 4 x1 UnitStepA
1
ÅÅÅÅ
2
+ x1E - 4 x12
UnitStepA
1
ÅÅÅÅ
2
+ x1EN +
1
ÅÅÅÅ
8
J-4 + UnitStepA-
1
ÅÅÅÅ
2
- x1E + 4 x1 UnitStepA-
1
ÅÅÅÅ
2
- x1E + 4 x12
UnitStepA-
1
ÅÅÅÅ
2
- x1E +
9 UnitStepA
3
ÅÅÅÅ
2
+ x1E + 12 x1 UnitStepA
3
ÅÅÅÅ
2
+ x1E + 4 x12
UnitStepA
3
ÅÅÅÅ
2
+ x1EN
We see that we get a result that begins to look more towards a Gaussian:

Plot@8h2, gauss@x1, .5D<, 8x1, -3, 3<, PlotRange -> All,
PlotStyle -> 8Dashing@8<D, Dashing@80.02, 0.02<D<, ImageSize -> 150D;
-3 -2 -1 1 2 3
0.2
0.4
0.6
0.8
Figure 3.14 Two times a convolution of a blockfunction with the same blockfunction gives a
function that rapidly begins to look like a Gaussian function. A Gaussian kernel with s = 0.5
is drawn (dotted) for comparison.
The real Gaussian is reached when we apply an infinite number of these convolutions with
the same function. It is remarkable that this result applies for the infinite repetition of any
convolution kernel. This is the central limit theorem.
Ú Task 3.1 Show the central limit theorem in practice for a number of other
arbitrary kernels.
3.10 Anisotropy
PlotGradientField@-gauss@x, 1D gauss@y, 1D,
8x, -3, 3<, 8y, -3, 3<, PlotPoints -> 20, ImageSize -> 140D;
Figure 3.15 The slope of an isotropic Gaussian function is indicated by arrows here. There are
circularly symmetric, i.e. in all directions the same, from which the name isotropic derives.
The arrows are in the direction of the normal of the intensity landscape, and are called
gradient vectors.
The Gaussian kernel as specified above is isotropic, which means that the behaviour of the
function is in any direction the same. For 2D this means the Gaussian function is circular, for
3D it looks like a fuzzy sphere.
It is of no use to speak of isotropy in 1-D. When the standard deviations in the different
dimensions are not equal, we call the Gaussian function anisotropic. An example is the
pointspreadfunction of an astigmatic eye, where differences in curvature of the cornea/lens in
different directions occur. This show an anisotropic Gaussian with anisotropy ratio of 2
Hsx êsy = 2L:
48 3.9 Central limit theorem

Unprotect@gaussD;
gauss@x_, y_, sx_, sy_D :=
1
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅ
2 p sx sy
ExpA-
i
k
jjjj
x2
ÅÅÅÅÅÅÅÅÅÅÅÅÅ
2 sx2
+
y2
ÅÅÅÅÅÅÅÅÅÅÅÅÅ
2 sy2
y
{
zzzzE;
sx = 2; sy = 1; Block@8$DisplayFunction = Identity<,
p1 = DensityPlot@gauss@x, y, sx, syD,
8x, -10, 10<, 8y, -10, 10<, PlotPoints -> 50D;
p2 = Plot3D@gauss@x, y, sx, syD, 8x, -10, 10<,
8y, -10, 10<, Shading -> TrueD;
p3 = ContourPlot@gauss@x, y, sx, syD, 8x, -5, 5<, 8y, -10, 10<DD;
Show@GraphicsArray@8p1, p2, p3<D, ImageSize -> 400D;
-4 -2 0 2 4
-10
-5
0
5
10
Figure 3.16 An anisotropic Gaussian kernel with anisotropy ratio sx ê sy = 2 in three
appearances. Left: DensityPlot, middle: Plot3D, right: ContourPlot.
3.11 The diffusion equation
The Gaussian function is the solution of several differential equations. It is the solution of
d y
ÅÅÅÅÅÅÅÅd x
=
yHm-xL
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅs2 , because
d y
ÅÅÅÅÅÅÅÅy
=
Hm-xL
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅs2 d x, from which we find by integration lnI
y
ÅÅÅÅÅÅÅy0
M = -
Hm-xL2
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅ2 s2
and thus y = y0 e-
Hx-mL2
ÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅÅ2 s2
.
It is the solution of the linear diffusion equation, ∑L
ÅÅÅÅÅÅÅ∑t
= ∑2 L
ÅÅÅÅÅÅÅÅÅÅ∑x2 + ∑2 L
ÅÅÅÅÅÅÅÅÅÅ∑y2 = D L.
This is a partial differential equation, stating that the first derivative of the (luminance)
function LHx, yL to the parameter t (time, or variance) is equal to the sum of the second order
spatial derivatives. The right hand side is also known as the Laplacian (indicated by D for
any dimension, we call D the Laplacian operator), or the trace of the Hessian matrix of
second order derivatives:
hessian2D =
i
k
jjj
Lxx Lxy
Lxy Lyy
y
{
zzz; Tr@hessian2DD
Lxx + Lyy
hessian3D =
i
k
jjjjjjjj
Lxx Lxy Lxz
Lyx Lyy Lyz
Lzx Lyz Lzz
y
{
zzzzzzzz
; Tr@hessian3DD
Lxx + Lyy + Lzz
The diffusion equation ∑u
ÅÅÅÅÅÅÅ∑t
= D u is one of some of the most famous differential equations in
physics. It is often referred to as the heat equation. It belongs in the row of other famous
equations like the Laplace equation D u = 0, the wave equation ∑2 u
ÅÅÅÅÅÅÅÅÅ∑t2 = D u and the
Schrödinger equation ∑u
ÅÅÅÅÅÅÅ∑t
= i D u.

ÅÅÅÅÅÅÅ∑t
= D u is one of some of the most famous differential equations in
physics. It is often referred to as the heat equation. It belongs in the row of other famous
equations like the Laplace equation D u = 0, the wave equation ∑2
u
ÅÅÅÅÅÅÅÅÅ∑t2 = D u and the
Schrödinger equation ∑u
ÅÅÅÅÅÅÅ∑t
= i D u.
ÅÅÅÅÅÅÅ∑t
= D u is a linear equation. It consists of just linearly combined
derivative terms, no nonlinear exponents or functions of derivatives.
The diffused entity is the intensity in the images. The role of time is taken by the variance
t = 2 s2 . The intensity is diffused over time (in our case over scale) in all directions in the
same way (this is called isotropic). E.g. in 3D one can think of the example of the intensity
of an inkdrop in water, diffusing in all directions.
The diffusion equation can be derived from physical principles: the luminance can be
considered a flow, that is pushed away from a certain location by a force equal to the
gradient. The divergence of this gradient gives how much the total entity (luminance in our
case) diminishes with time.
<< Calculus`VectorAnalysis`
SetCoordinates@Cartesian@x, y, zDD;
Div@ Grad@L@x, y, zDDD
LH0,0,2L
@x, y, zD + LH0,2,0L
@x, y, zD + LH2,0,0L
@x, y, zD
A very important feature of the diffusion process is that it satisfies a maximum principle
[Hummel1987b]: the amplitude of local maxima are always decreasing when we go to
coarser scale, and vice versa, the amplitude of local minima always increase for coarser
scale. This argument was the principal reasoning in the derivation of the diffusion equation
as the generating equation for scale-space by Koenderink [Koenderink1984a].
3.12 Summary of this chapter
The normalized Gaussian kernel has an area under the curve of unity, i.e. as a filter it does
not multiply the operand with an accidental multiplication factor. Two Gaussian functions
can be cascaded, i.e. applied consecutively, to give a Gaussian convolution result which is
equivalent to a kernel with the variance equal to the sum of the variances of the constituting
Gaussian kernels. The spatial parameter normalized over scale is called the dimensionless
'natural coordinate'.
The Gaussian kernel is the 'blurred version' of the Delta Dirac function, the cumulative
Gaussian function is the Error function, which is the 'blurred version' of the Heavyside
stepfunction. The Dirac and Heavyside functions are examples of generalized functions.
The Gaussian kernel appears as the limiting case of the Pascal Triangle of binomial
coefficients in an expanded polynomial of high order. This is a special case of the central
limit theorem. The central limit theorem states that any finite kernel, when repeatedly
convolved with itself, leads to the Gaussian kernel.
50 3.11 The diffusion equation

Anisotropy of a Gaussian kernel means that the scales, or standard deviations, are different
for the different dimensions. When they are the same in all directions, the kernel is called
isotropic.
The Fourier transform of a Gaussian kernel acts as a low-pass filter for frequencies. The cut-
off frequency depends on the scale of the Gaussian kernel. The Fourier transform has the
same Gaussian shape. The Gaussian kernel is the only kernel for which the Fourier transform
has the same shape.
The diffusion equation describes the expel of the flow of some quantity (intensity,
temperature) over space under the force of a gradient. It is a second order parabolic
differential equation. The linear, isotropic diffusion equation is the generating equation for a
scale-space. In chapter 21 we will encounter a wealth on nonlinear diffusion equations.

03 the gaussian kernel

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03 the gaussian kernel