[ctsim.git] / doc / ctsim-gui.tex

\chapter{The Graphical User Interface}\label{ctsim}\index{ctsim}%
\setheader{{\it CHAPTER \thechapter}}{}{}{\ctsimheadtitle}{}{{\it CHAPTER \thechapter}}%
\ctsimfooter%


\section{Overview}\index{Graphical shell}
\ctsim\ is the graphical shell for the CTSim project. This shell uses
the \urlref{wxWindows}{http://www.wxwindows.org} library for
cross-platform compatibility. The graphical shell is compatible
with Microsoft Windows, \urlref{GTK}{http://www.gtk.org}, and
\urlref{Motif}{http://www.openmotif.org} graphical environments.

\usage \texttt{ctsim [files to open...]}

You can invoke \ctsim\ by itself on the command line, or include
any number of files that you want \ctsim\ to
automatically open. \ctsim\ can open projection files, image
files, phantom files, and plot files.


\section{File Types}\index{File types}

\subsection{Phantom}
Besides loading phantom files from the disk, the Herman and
Shepp-Logan phantoms are built-in to \ctsim. Phantom files can be
read and stored on the disk. Phantom files are stored in a simple
ASCII format. A text editor is required to
create and edit these files.

\subsection{Image}
Image files are 2-dimensional files that store 4-byte floating
point values. Images files can be either real or complex valued.
Typically, all images are real except for images that have been
processed by Fourier transforms. As you might expect,
complex-valued images are twice the size of real-valued images
since both a real and imaginary component need to be store. When
complex-valued images are viewed on the screen, only the real
component is displayed.

Images files can also store any number of text labels. \ctsim\ uses
these labels for storing history information regarding
the creation and modifications of images.

\subsection{Projection}
Projection files are created from phantom files during the
projection process. Numerous options are available for the
creation of the these files. The files are stored in a binary
format with cross-platform compatibility on little and big endian
architectures.

\subsection{Plot}
Plot files are created by \ctsim\ during analysis of image files.
They can be read and stored on the disk. They are stored as ASCII
files for easy cross-platform support and editing.

\section{Global Menu Commands}
These global commands are present on the menus of all windows.

\subsection{File - Create Phantom}\label{IDH_DLG_PHANTOM}\index{Dialog!Create phantom}
This command brings up a dialog box showing the phantoms that are preprogrammed
into \ctsim. After selecting one of these phantoms, the new window with that
phantom will be generated. The preprogrammed phantoms are:

\begin{twocollist}
\twocolitem{\textbf{Herman}}{The Herman head phantom\cite{HERMAN80}}
\twocolitem{\textbf{Shepp-Logan}}{The head phantom of Shepp \& Logan\cite{SHEPP74}}
\twocolitem{\textbf{Unit pulse}}{A phantom that has a value of \texttt{1} for the
center of the phantom and \texttt{0} everywhere else.}
\end{twocollist}

\subsection{File - Create Filter}\label{IDH_DLG_FILTER}\index{Dialog!Create filter}
This command brings up a dialog box showing the pre-programmed filters
of \ctsim. This command will create a 2-dimensional image of the selected filter.
The center of the filter is at the center of the image.

These filters can be created in their natural frequency domain or in their spatial domain.

\begin{twocollist}
\twocolitem{\textbf{Filter}}{Selects the filter to generate.}
\twocolitem{\textbf{Domain}}{Selects either the \texttt{Frequency} or \texttt{Spatial} domains. The filters have the
frequency domain as their natural domain.}
\twocolitem{\textbf{X Size}}{Number of columns in the output image.}
\twocolitem{\textbf{Y Size}}{Number of rows in the output image.}
\twocolitem{\textbf{Hamming Parameter}}{Sets the parameter for the Hamming filter.}
\twocolitem{\textbf{Bandwidth}}{Sets the bandwidth of the filter.}
\twocolitem{\textbf{Axis (input) Scale}}{Sets the scale for the filter input. By default, the input to the filter is
the distance in pixels from the center of the image. By changing this value, one can set a scale the input to the filter.
For example, if the output image is \texttt{101} pixels and thus the center of the image is at \texttt{(50,50)}, then a pixel
lying at point \texttt{100,50} would be 50 units from the center of the filter. By applying an \texttt{Axis scale} of
\texttt{0.1}, then that point would be scaled to 5 units from the center of the filter.}
\twocolitem{\textbf{Filter (output) Scale}}{Multiplies the output of the filter by this amount. By default, the filter has a maximum
value of \texttt{1}.}
\end{twocollist}

\subsection{File - Preferences}\label{IDH_DLG_PREFERENCES}\index{Dialog!Preferences}
This command displays a dialog box that allows users to control
the behavior of \ctsim. These options are saved across \ctsim\ sessions.
Under Microsoft Windows environments, they are stored in the registry.
On UNIX and Linux environments, they are stored in the user's home
directory with the filename of \texttt{.ctsim}.

\begin{twocollist}
\twocolitem{\textbf{Advanced options}}{By default, this is turned off in new installations.
These advanced options are not required for normal simulations. When \texttt{Advanced
Options} is set, \ctsim\ will display more options during scanning of phantoms and
the reconstruction of projections.}

\twocolitem{\textbf{Ask before deleting new documents}}{By default, this is turned on in
new installations. With this option set, \ctsim\ will ask before closing
documents that have been modified or never saved on disk. By turning off
this option, \ctsim\ will never ask if you want to save a file -- you'll
be responsible for saving any files that you create.}

\end{twocollist}

\subsection{File - Open}
This command opens a file section dialog box. Of special consideration
is the \texttt{File Type} combo box on the bottom of the dialog. You need
to set the \texttt{File Type} combo box to to the type of file that you wish to open.

\subsection{File - Save}
This command saves the contents of the active window. If the window hasn't
been named, a dialog box will open asking for the file name to use.

\subsection{File - Close}
As one would expect, this closes the active window.

\subsection{File - Save As}
Allows the saving of the contents of a window to any filename.

\subsection{Help - Contents}
This command displays the online help.

\subsection{Help - About}
This command shows the version number of \ctsim.


\section{Phantom Menus}

\subsection{Properties}
Displays the properties of a phantom which includes:

\begin{itemize}\itemsep=0pt
\item Overall dimensions of a phantom
\item A list of all component phantom elements
\end{itemize}

\subsection{Rasterize Dialog}\label{IDH_DLG_RASTERIZE}\index{Dialog!Rasterize}
This creates an image file from a phantom. Technically, it
converts the phantom from a vector (infinite resolution) object
into a 2-dimension array of floating-point pixels. The parameters
to set are:

\begin{twocollist}
\twocolitem{\textbf{X size}}{Number of columns in image file}
\twocolitem{\textbf{Y size}}{Number of rows in image file}
\twocolitem{\textbf{Samples per pixel}}{Numbers of samples taken
per pixel in both the x and y directions. For example, if the
\texttt{Samples per pixel} is set to \texttt{3}, then for every
pixel in the image file 9 samples \latexonly{($3\times3$)}\latexignore{(3 x 3)}
are averaged.}
\end{twocollist}

\subsection{Projection Dialog}\label{IDH_DLG_PROJECTIONS}\index{Dialog!Projections}
This creates a projection file from a phantom. The options
available when collecting projections are:

\begin{twocollist}
\twocolitem{\textbf{Geometry}}{Selects the scanner geometry.
  \begin{itemize}\itemsep=0pt
    \item \texttt{Parallel}
    \item \texttt{Equiangular}
    \item \texttt{Equilinear}
  \end{itemize}}
\twocolitem{\textbf{Number of detectors}}{Sets the number of
detectors in the detector array.}

\twocolitem{\textbf{Number of views}}{Sets the number of views
collected}

\twocolitem{\textbf{Samples per detector}}{Sets the number of
samples collected for each detector}

\twocolitem{\textbf{View Ratio}}{Sets the field of view as a ratio
of the diameter of the phantom.  For normal scanning, use a value of
\texttt{1.0}.}

\twocolitem{\textbf{Scan Ratio}}{Sets the length of scanning as a
ratio of the view diameter. For normal scanning, use a value of \texttt{1.0}.}

\twocolitem{\textbf{Focal length ratio}}{Sets the distance between the
radiation source and the center of the phantom as a
ratio of the radius of the phantom. For parallel geometries, a value
of \texttt{1.0} is optimal. For other
geometries, this should be at least \texttt{2.0} to avoid artifacts.}
\end{twocollist}

\textbf{Advanced Options}

\begin{twocollist}
\twocolitem{\textbf{Rotation Angle}}{Sets the rotation amount as a
multiple of \latexonly{$\pi$.}\latexignore{pi.} For parallel geometries use a rotation angle of \texttt{1}
and for equilinear and equiangular geometries use a rotation angle
of \texttt{2}. Using any other rotation angle will lead to artifacts.}
\end{twocollist}



\section{Image Menus}
\subsection{File - Properties}
Properties of image files include
\begin{itemize}\itemsep=0pt
  \item Whether the image is real or complex valued
  \item Numeric statistics (minimum, maximum, mean, median, mode, and standard deviation)
  \item History labels (text descriptions of the processing for this image)
\end{itemize}

\subsection{File - Export}\label{IDH_DLG_EXPORT}\index{Image!Export}
This command allows for exporting image files to a standard
graphics file format. This is helpful when you want to take an
image and import it into another application. The current
\helprefn{intensity scale}{intensityscale} is used when exporting
the file. The supported graphic formats are:

\begin{twocollist}
\twocolitem{\textbf{PNG}}{Portable Network Graphics format. This uses 8-bits or
256 shades of gray.}
\twocolitem{\textbf{PNG-16}}{This is a 16-bit version of PNG which allows for
65536 shades of gray.}
\twocolitem{\textbf{PGM}}{Portable Graymap format. This is a common format used on
UNIX systems.}
\twocolitem{\textbf{PGM}}{ASCII version of PGM.}
\end{twocollist}


\subsection{View}\label{intensityscale}\index{Intensity Scale}
These commands are used change the intensity scale for viewing the image.
These commands do not change the image data. When the minimum intensity is
set, then the color pure black is assigned to that image intensity. Similarly,
when the maximum intensity is set, the the color pure white is assigned to that
image value.

Changing the intensity scale is useful when examining different image features.
In clinical medicine, the intensity scale is often changed to examine bone
(high intensity) verses soft-tissue (medium intensity) features.

\subsubsection{Set}\label{IDH_DLG_MINMAX}
This command displays a dialog box that allows you to set the lower
and upper intensities to display.

\subsubsection{Auto}\label{IDH_DLG_AUTOSCALE}
This command displays a dialog box that allows \ctsim\ to automatically
make an intensity scale. The parameters that \ctsim\ needs to make this
automatic scale are:

\begin{twocollist}
\twocolitem{\textbf{Center}}{This sets the center of the intensity scale. Currently,
\ctsim\ allows you to use either the mean, mode, or median of the image
as the center of the intensity scale.}

\twocolitem{\textbf{Width}}{This sets the half-width of the intensity scale. The width
is specified as a ratio of the standard deviation.}
\end{twocollist}

As an example, if \texttt{median} is selected as the center and
\texttt{0.5} is selected as the width, the the minimum intensity will
be \latexonly{$median - 0.5 \times standardDeviation$}\latexignore{\emph{median - 0.5 x standardDeviation}}
and the maximum will be \latexonly{$median + 0.5 \times standardDeviation$.}\latexignore{\emph{
median + 0.5 x standardDeviation}.}

\subsubsection{Full}
This command resets the intensity scale to the full scale of the image.

\subsection{Image}
These commands create a new image based upon the current image,
and for some commands, also upon a comparison image.

\subsubsection{Add, Subtract, Multiply, Divide}
These are simple arithmetic operations. \ctsim\ will display a dialog
box showing all of the currently opened image files that are the
same size as the active image. After the selection of a compatible image,
\ctsim\ will perform the arithmetic operation on the two images and
make a new result image.

\subsubsection{Image Size}
This command will generate a new image based on the current image. The new
image can be scaled to any size. A dialog
appears asking for the size of the new image. Bilinear interpolation
is used when calculating the new image.

\subsubsection{3-D Conversion}
Generates a 3-dimensional view of the current phantom. This view can be
rotated in three dimensions. The left and right arrow control the z-axis
rotation, the up and down arrows control the x-axis rotation. The y-axis
rotation is controlled by the \texttt{T} and \texttt{Y} keys. Other options
are presented on the \texttt{View} menu and include:

\begin{itemize}
\item Surface plot versus wireframe plot.
\item Smooth shading versus flat shading.
\item Lighting on or off.
\item Color scale on or off.
\end{itemize}

\subsection{Filter}\index{Image filter}
These commands filter and modify the image

\subsubsection{Arithmetic}
These commands operate on the image on a pixel-by-pixel basis. The commands
support both real and complex-valued images. The available arithmetic commards are:

\begin{twocollist}
  \twocolitem{\textbf{Invert}}{Negate pixel values.}
  \twocolitem{\textbf{Log}}{Take natural logrithm of pixel values.}
  \twocolitem{\textbf{Exp}}{Take natural exponent of pixel values.}
  \twocolitem{\textbf{Square}}{Take square of pixel values.}
  \twocolitem{\textbf{Square root}}{Take square root of pixel values.}
\end{twocollist}


\subsubsection{Frequency Based}
This commands allow the Fourier and inverse Fourier transformations of
images. By default, the transformations will automatically convert
images between Fourier to natural orders as expected. For example, \texttt{2-D FFT}
will transform the points into natural order after the Fourier transform.
Similarly the inverse, \texttt{2-D IFFT}, will reorder the points from
natural order to Fourier order before applying the inverse Fourier transformation.

As you would expect, images that undergo frequency filtering will be complex-valued
images. Normally, only the real component is shown by \ctsim. However, \ctsim\ does
have options for converting a complex-valued image into a real-valued image via
the \texttt{Magnitude} and \texttt{Phase} filtering commands.

\subsection{Analyze}
These commands are used for analyzing an image.

\subsubsection{Plotting}
The commands plot rows and columns of images. There are also commands
that perform FFT and IFFT transformations prior to plotting.

\subsubsection{Image Comparison}\label{IDH_DLG_COMPARISON}\index{Image!Comparison}
This command performs statistical comparisons between two images. An option
also exists for generating a difference image from the two input images.

There are also commands for comparison plotting of rows and columns from two images.
 This is quite helpful when comparing a phantom to a reconstruction.

\section{Projection Menus}

\subsection{File - Properties}
The displayed properties include:

\begin{itemize}
\item Number of detectors in the projections
\item Number of views
\item The variables used when generating the projections from the phantom
\end{itemize}

\subsection{Process - Convert Polar Dialog}\label{IDH_DLG_POLAR}\index{Polar conversion}
Creates an image file with the polar conversion of the projection data. The options to set are:

\begin{twocollist}
\twocolitem{\textbf{xsize}}{Number of columns in output image.}
\twocolitem{\textbf{ysize}}{Number of rows in output image.}
\twocolitem{\textbf{interpolation}}{Selects the interpolation method.
Currently, the \texttt{bilinear} option provides the highest
quality interpolation.}
\end{twocollist}

\subsection{Process - Convert FFT Polar Dialog}
The parameters for this option are the same as \helprefn{Convert
Polar Dialog}{convertpolardialog}. For this command, though, the
projections are Fourier transformed prior to conversion to polar
image.

\subsection{Reconstruct - Filtered Backprojection Dialog}\label{IDH_DLG_RECONSTRUCTION}\index{Dialog!Reconstruction}
This dialog sets the parameters for reconstructing an image from projections
using the Filtered Backprojection technique.


\begin{twocollist}
\twocolitem{\textbf{Filter}}{Selects which filter to apply to each
projection. To properly reconstruct an image, this filter should
be consist of the the absolute value of distance from zero
frequency optionally multiplied by a smoothing filter. The optimal
filters to use are:
\begin{itemize}\itemsep=0pt
\item \texttt{abs\_bandlimit}
\item \texttt{abs\_cosine}
\item \texttt{abs\_hamming}
\end{itemize}
} \twocolitem{\textbf{Hamming parameter}}{Sets the alpha level for
Hamming   window. At setting of 0.54, this equals the Hanning
window.}

\twocolitem{\textbf{Filter Method}}{Selects the filtering method.
For large numbers of detectors, \texttt{rfftw} is optimal. For
smaller numbers of detectors, \texttt{convolution} might be a bit
faster.
\begin{itemize}\itemsep=0pt
\item \texttt{convolution}
\item \texttt{fourier} - Uses simple Fourier transform.
\item \texttt{fourier-table} - Optimizes Fourier transform by precalculating trigometric functions.
\item \texttt{fftw} - Uses complex-valued Fourier transform with the \emph{fftw} library.
\item \texttt{rfftw} - Uses optimized real/half-complex Fourier transform.
\end{itemize}
}

\twocolitem{\textbf{Interpolation}}{Interpolation technique.
\texttt{cubic} is optimal when the
data is smooth. Smooth data is obtained by taking many projections and/or
using a smoothing filter. In the absence of smooth data, \texttt{linear} gives better results and
is many times faster than cubic interpolation.

\begin{itemize}\itemsep=0pt
\item nearest
\item linear
\item cubic
\end{itemize}
}
\end{twocollist}

\textbf{Advanced Options}

These options are only visible if \emph{Advanced Options} has been
selected in the \texttt{File - Preferences} dialog. These parameters
default to optimal settings and don't need to be adjusted except
by expert users.

\begin{twocollist}
\twocolitem{\textbf{Backprojection}}{Selects the backprojection
technique. A setting of \texttt{idiff} is optimal.
\begin{itemize}\itemsep=0pt
\item \texttt{trig} - Use trigometric functions at each image point.
\item \texttt{table} - Use precalculated trigometric tables.
\item \texttt{diff} - Use difference method to iterate within image.
\item \texttt{idiff} - Use integer iteration math.
\end{itemize}
}

\twocolitem{\textbf{Filter Generation}}{Selects the filter
generation. With convolution, \texttt{direct} is the proper method
to select. With any of the frequency methods,
\texttt{inverse-fourier} is the best method.
\begin{itemize}\itemsep=0pt
\item \texttt{direct}
\item \texttt{inverse-fourier}
\end{itemize}
}

\twocolitem{\textbf{Zeropad}}{Zeropad factor when using
frequency-based filtering. A setting of \texttt{1} is optimal whereas
a setting of \texttt{0} disables zero padding.}

\end{twocollist}

\section{Plot Menus}
\subsection{File - Properties}
The displayed properties include:

\begin{itemize}\itemsep=0pt
\item the number of curves in the plot and the number of points per curve.
\item the EZPlot commands used to format the plot are displayed.
\item history labels from the originating image(s) and the plot function
\end{itemize}

\subsection{View Menu}
These commands set the scaling for the y-axis. They are analogous
to the options used for setting the intensity scale for images.

\subsubsection{Set}
This command sets the upper and lower limits for the y-axis.

\subsubsection{Auto}
This command automatically sets the upper and lower limits for the
y-axis. Please refer to the \texttt{View - Auto} documentation for
image files for the details.

\subsubsection{Full}
The command resets the upper and lower limits of the y-axis to the
minimum and maximum values of the curves.