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Taddeüs Kroes
uva
Commits
3895c9fd
Commit
3895c9fd
authored
Oct 24, 2011
by
Taddeüs Kroes
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improc ass4: Updated separability section in report.
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improc/ass4/report/gauss_times_1d.pdf
improc/ass4/report/gauss_times_1d.pdf
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improc/ass4/report/gauss_times_2d.pdf
improc/ass4/report/gauss_times_2d.pdf
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improc/ass4/report/report.tex
improc/ass4/report/report.tex
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...
@@ -18,29 +18,145 @@
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@@ -18,29 +18,145 @@
\section
{
Analytical Local Structure
}
\section
{
Analytical Local Structure
}
\subsection
{
Derivatives
}
\subsection
{
Derivatives
}
\label
{
sub:derivatives
}
We have been given the following function:
We have been given the following function:
$$
f
(
x, y
)
=
A sin
(
Vx
)
+
B cos
(
Wy
)
$$
$$
f
(
x, y
)
=
A sin
(
Vx
)
+
B cos
(
Wy
)
$$
The partial derivatives
$
f
_
x, f
_
y, f
_{
xx
}
, f
_{
xy
}$
and
$
f
_{
yy
}$
can be derived as follows:
The partial derivatives
$
f
_
x, f
_
y, f
_{
xx
}
, f
_{
xy
}$
and
$
f
_{
yy
}$
can be
derived as follows:
\begin{table}
[H]
\begin{table}
[H]
\begin{tabular}
{
rl
}
\begin{tabular}
{
rl
}
$
f
_
x
$
&
$
=
A
\frac
{
\delta
}{
\delta
x
}
sin
(
Vx
)
+
B
\frac
{
\delta
}{
\delta
x
}
cos
(
Wy
)
$
\\
$
f
_
x
$
&
$
=
\frac
{
\delta
f
}{
\delta
x
}$
\\
&
$
=
A
\frac
{
\delta
}{
\delta
x
}
sin
(
Vx
)
+
B
\frac
{
\delta
}{
\delta
x
}
cos
(
Wy
)
$
\\
&
$
=
A cos
(
Vx
)
\cdot
V
+
B
\cdot
0
$
\\
&
$
=
A cos
(
Vx
)
\cdot
V
+
B
\cdot
0
$
\\
&
$
=
AV cos
(
Vx
)
$
\\
&
$
=
AV cos
(
Vx
)
$
\\
&
\\
&
\\
$
f
_
y
$
&
$
=
A
\frac
{
\delta
}{
\delta
y
}
sin
(
Vx
)
+
B
\frac
{
\delta
}{
\delta
y
}
cos
(
Wy
)
$
\\
$
f
_
y
$
&
$
=
\frac
{
\delta
f
}{
\delta
y
}$
\\
&
$
=
A
\frac
{
\delta
}{
\delta
y
}
sin
(
Vx
)
+
B
\frac
{
\delta
}{
\delta
y
}
cos
(
Wy
)
$
\\
&
$
=
A
\cdot
0
-
B sin
(
Wy
)
\cdot
W
$
\\
&
$
=
A
\cdot
0
-
B sin
(
Wy
)
\cdot
W
$
\\
&
$
=
-
BW sin
(
Wy
)
$
\\
&
$
=
-
BW sin
(
Wy
)
$
\\
&
\\
&
\\
$
f
_{
xx
}$
&
$
=
AV
\frac
{
\delta
}{
\delta
x
}
cos
(
Vx
)
$
\\
$
f
_{
xx
}$
&
$
=
\frac
{
\delta
f
_
x
}{
\delta
x
}$
\\
&
$
=
AV
\frac
{
\delta
}{
\delta
x
}
cos
(
Vx
)
$
\\
&
$
=
-
AV
^
2
sin
(
Vx
)
$
\\
&
$
=
-
AV
^
2
sin
(
Vx
)
$
\\
&
\\
&
\\
$
f
_{
xy
}$
&
$
=
AV
\frac
{
\delta
}{
\delta
y
}
cos
(
Vx
)
=
0
$
\\
$
f
_{
xy
}$
&
$
=
\frac
{
\delta
f
_
x
}{
\delta
y
}
=
AV
\frac
{
\delta
}{
\delta
y
}
cos
(
Vx
)
=
0
$
\\
&
\\
&
\\
$
f
_{
yy
}$
&
$
=
-
BW
\frac
{
\delta
}{
\delta
y
}
sin
(
Wy
)
$
\\
$
f
_{
yy
}$
&
$
=
\frac
{
\delta
f
_
y
}{
\delta
y
}$
\\
&
$
=
-
BW
\frac
{
\delta
}{
\delta
y
}
sin
(
Wy
)
$
\\
&
$
=
-
BW
^
2
cos
(
Wy
)
$
\\
&
$
=
-
BW
^
2
cos
(
Wy
)
$
\\
\end{tabular}
\end{tabular}
\end{table}
\end{table}
\pagebreak
\subsection
{
Plots
}
The following plots show
$
f
(
x, y
)
$
and its first and second derivatives. The
image on the left shows
$
f
_
x
$
and
$
f
_
y
$
. The image on the right shows
$
f
_{
xx
}$
and
$
f
_{
yy
}$
in a quiver plot over
$
f
(
x, y
)
$
. The arrows point towards the
largest increase of gray value, which means that the derivations in chapter
\ref
{
sub:derivatives
}
are correct.
\begin{figure}
[H]
\hspace
{
-2cm
}
\includegraphics
[scale=.8]
{
samples.pdf
}
\caption
{
Plots of
$
f
(
x, y
)
$
and its first and second derivatives.
}
\end{figure}
\section
{
Gaussian Convolution
}
\subsection
{
Implementation
}
All Gaussian functions are implemented in the file
\emph
{
gauss.py
}
. The
\texttt
{
Gauss
}
function fills a 2D array with the values of the 2D Gaussian
function
\footnote
{
\label
{
footnote:gaussian-filter
}
\url
{
http://en.wikipedia.org/wiki/Gaussian
_
filter
}}
:
$$
g
_{
2
D
}
(
x, y
)
=
\frac
{
1
}{
2
\pi
\sigma
^
2
}
e
^{
-
\frac
{
x
^
2
+
y
^
2
}{
2
\sigma
^
2
}}$$
This function converges to zero, but never actually equals zero. The filter's
size is therefore chosen to be
$
\lceil
6
*
\sigma
\rceil
$
in each direction by
convention (since values for
$
x,y >
3
*
\sigma
$
are negligible). Finally,
because the sum of the filter should be equal to 1, it is divided by its own
sum.
The result of the
\texttt
{
Gauss
}
function is shown in figure
\ref
{
fig:gauss-diff
}
. The subplots respectively show the original image, the
Gaussian kernel and the convolved image.
\begin{figure}
[H]
\label
{
fig:gauss-diff
}
\hspace
{
-5cm
}
\includegraphics
[scale=.6]
{
gauss
_
diff
_
5.pdf
}
\caption
{
The result of
\texttt
{
python gauss.py diff 5
}
.
}
\end{figure}
\subsection
{
Measuring Performance
}
We've timed the runtime of the
\texttt
{
Gauss
}
function for
$
\sigma
=
1
,
2
,
3
,
5
,
7
,
9
,
11
,
15
,
19
$
, the results are in figure
\ref
{
fig:times-2d
}
. The graph shows a computational complexity of
$
\mathcal
{
O
}
(
\sigma
^
2
)
$
.
\begin{figure}
[H]
\label
{
fig:times-2d
}
\center
\includegraphics
[scale=.5]
{
gauss
_
times
_
2d.pdf
}
\caption
{
The result of
\texttt
{
python gauss.py timer 2d 5
}
(so, each
timing has been repeated 5 times and then averaged).
}
\end{figure}
\section
{
Separable Gaussian Convolution
}
\subsection
{
Implementation
}
The
\texttt
{
Gauss1
}
function uses the 1D Gaussian
function
\ref
{
footnote:gaussian-filter
}
:
$$
g
_{
1
D
}
(
x
)
=
\frac
{
1
}{
\sqrt
{
2
\pi
}
\cdot
\sigma
}
e
^{
-
\frac
{
x
^
2
}{
2
\sigma
^
2
}}$$
This function returns a 1D array of kernel values, which is used by the
function
\texttt
{
convolve1d
}
. Using the separability property, the following
code snippets produce the same result:
\begin{verbatim}
W = Gauss1(s)
G = convolve1d(F, W, axis=0, mode='nearest')
G = convolve1d(G, W, axis=1, mode='nearest')
\end{verbatim}
as opposed to:
\begin{verbatim}
G = convolve(F, Gauss(s), mode='nearest')
\end{verbatim}
The timing results of the first code snippet are displayed in figure
\ref
{
fig:times-1d
}
. The graphs shows that
\texttt
{
Gauss1
}
has a computational
complexity of
$
\mathcal
{
O
}
(
\sigma
)
$
, which is much faster than the 2D
convolution (certainly for higher scales).
\begin{figure}
[H]
\label
{
fig:times-1d
}
\center
\includegraphics
[scale=.5]
{
gauss
_
times
_
1d.pdf
}
\caption
{
The result of
\texttt
{
python gauss.py timer 1d 50
}
.
}
\end{figure}
\section
{
Gaussian Derivatives
}
\subsection
{
Separability
}
We can show analytically that all derivatives of the 2D Gaussian function
are separable as well:
\begin{table}
[H]
\begin{tabular}
{
rl
}
$
$
&
$
=
$
\\
\end{tabular}
\end{table}
\end{document}
\end{document}
\ No newline at end of file
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