Merge branch '3.0.1' into developer

This commit is contained in:
Dhanya Maliakal 2017-11-28 11:18:43 +01:00
commit 130f3d2e6f
260 changed files with 48 additions and 22571 deletions

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<B> Next:</B> <A NAME="tex2html7"
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<P>
<H1 ALIGN="CENTER">Angular calibration wizard manual</H1>
<DIV>
<P ALIGN="CENTER"><STRONG>Anna Bergamaschi</STRONG></P>
<P ALIGN="CENTER"><STRONG>August 24, 2017</STRONG></P>
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<BR><HR>
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<LI><A NAME="tex2html9"
HREF="node2.html">Data acquisition</A>
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<LI><A NAME="tex2html10"
HREF="node2.html#SECTION00021000000000000000">Software</A>
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HREF="node3.html">Data analysis</A>
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<LI><A NAME="tex2html12"
HREF="node3.html#SECTION00031000000000000000">Software</A>
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<LI><A NAME="tex2html13"
HREF="node4.html">Setup calibration files</A>
<LI><A NAME="tex2html14"
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<ADDRESS>
Thattil Dhanya
2017-08-24
</ADDRESS>
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<B> Next:</B> <A NAME="tex2html7"
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<P>
<H1 ALIGN="CENTER">Angular calibration wizard manual</H1>
<DIV>
<P ALIGN="CENTER"><STRONG>Anna Bergamaschi</STRONG></P>
<P ALIGN="CENTER"><STRONG>August 24, 2017</STRONG></P>
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<LI><A NAME="tex2html9"
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<LI><A NAME="tex2html10"
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<LI><A NAME="tex2html12"
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<H1><A NAME="SECTION00010000000000000000">
Introduction</A>
</H1>
<P>
In order to convert from strip number to 2<IMG
WIDTH="12" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img1.png"
ALT="$\theta$">-angle, an accurate angular calibration of the detector must be performed (for details see the paper Bergamaschi, A. et al. (2010). J. Synchrotron Rad. 17, 653-668).
<BR>
<P>
For this purpose, a series of patterns of a powder standard with symmetric peaks (e.g. silicon) must acquired while shifting the detector by an angular step of the order of about 2% of the module size. During the measurement, a strong intensity peak (e.g. Si(111)) should pass through the field of view of every module such that it can be used as a reference angular position to perform the calibration of the modules position.
<BR>
<P>
In a first step, the peak is fitted with a Gaussian in order to determine its position <IMG
WIDTH="43" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img2.png"
ALT="$C_{peak}$"> in channel number for each of the acquired patterns.
<BR>
In a second step, for each module <IMG
WIDTH="10" HEIGHT="17" ALIGN="BOTTOM" BORDER="0"
SRC="img3.png"
ALT="$i$">, the encoder position <IMG
WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img4.png"
ALT="$\Theta_e$"> is fitted as a function of the peak position <IMG
WIDTH="43" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img2.png"
ALT="$C_{peak}$"> according to:
<BR>
<DIV ALIGN="RIGHT">
<!-- MATH
\begin{equation}
\Theta_e=\Theta_o^i-\arctan\Big(\frac{p \cdot (C_{peak}-C_{center}^i)}{R^i}\Big),
\end{equation}
-->
<TABLE WIDTH="100%" ALIGN="CENTER">
<TR VALIGN="MIDDLE"><TD ALIGN="CENTER" NOWRAP><A NAME="eq:angcal"></A><IMG
WIDTH="291" HEIGHT="41" BORDER="0"
SRC="img5.png"
ALT="\begin{displaymath}
\Theta_e=\Theta_o^i-\arctan\Big(\frac{p \cdot (C_{peak}-C_{center}^i)}{R^i}\Big),
\end{displaymath}"></TD>
<TD WIDTH=10 ALIGN="RIGHT">
(1)</TD></TR>
</TABLE>
<BR CLEAR="ALL"></DIV><P></P>
where the parameters <IMG
WIDTH="24" HEIGHT="36" ALIGN="MIDDLE" BORDER="0"
SRC="img6.png"
ALT="$\Theta_o^i$"> is the angular offset with respect to the diffractometer zero position, <!-- MATH
$C_{center}^{i}$
-->
<IMG
WIDTH="53" HEIGHT="36" ALIGN="MIDDLE" BORDER="0"
SRC="img7.png"
ALT="$C_{center}^{i}$"> is the central channel and <IMG
WIDTH="22" HEIGHT="16" ALIGN="BOTTOM" BORDER="0"
SRC="img8.png"
ALT="$R^i$"> is the distance of the module <IMG
WIDTH="10" HEIGHT="17" ALIGN="BOTTOM" BORDER="0"
SRC="img3.png"
ALT="$i$"> from the diffractometer center while <IMG
WIDTH="79" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img9.png"
ALT="$p=50~\mu m$"> is the strip pitch of the detector.
<BR>
Finally, the global offset of the detector system is precisely determined by refining a silicon pattern at a well-defined energy (i.e., knowing the position of the peak).
<P>
The same function of equation&nbsp;<A HREF="#eq:angcal">1</A>, with the parameters obtained from the calibration, is used in order to convert from channel number to 2<IMG
WIDTH="12" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img1.png"
ALT="$\theta$">-angle.
<P>
The parallax at the borders of the modules due to the thickness of the silicon sensor is a function of the X-ray energy (higher energy X-rays are absorbed deeper inside the sensor) and is of the order of 0.2&nbsp;mdeg at 12&nbsp;keV and 0.5&nbsp;mdeg at 30&nbsp;keV.
<BR>
The differences in pixel size due to the different portion of solid angle covered by the strips on the border of the modules and the higher efficiency due to the longer path of the X-rays in the sensor are removed by the flat field correction. This also normalizes additional differences in pixel size between channels which are also present because of mismatches in the strip sensor fabrication and in fluctuations of the channels threshold level.
<P>
Patterns acquired at different detector positions are generally merged together in order to fill the gaps between the modules and correct possibly bad functioning channels. In this procedure the data from different positions which are closer than 4&nbsp;mdeg (the average pixel size) are averaged and the new position is set to the mean of the positions of the original points.
<P>
The position and width of the peaks results from a fit over several detector channels. Geometrical distortions might disturb this determination mainly because of errors in the angular calibration, fluctuations in the encoder position, variations between channels and parallax effects.
<BR>
The resolution in locating the peak center and determining its width and integrated intensity has been estimated by acquiring several patterns of a LaB<IMG
WIDTH="12" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img10.png"
ALT="$_6$"> sample in a 300&nbsp;<IMG
WIDTH="14" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img11.png"
ALT="$\mu$">m capillary with the detector shifted in 5&nbsp;mdeg steps between 30.4 and 36.5 degrees. The 16&nbsp;peaks acquired have been fitted with a Gaussian function plus background and the fluctuations on the fitted parameters have been calculated. The resulting average resolutions are 0.63<IMG
WIDTH="17" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img12.png"
ALT="$\pm$">0.06&nbsp;mdeg for the peak center and 0.22<IMG
WIDTH="17" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img12.png"
ALT="$\pm$">0.05&nbsp;mdeg for the peak Full-Width at Half-Maximum (FWHM) for an average peak FWHM of 27.0<IMG
WIDTH="17" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img12.png"
ALT="$\pm$">2.5&nbsp;mdeg.
<BR>
These results show that the angular calibration allows a resolution in determining the peaks position and width which is appropriate for structural determination.
<P>
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<H1><A NAME="SECTION00020000000000000000">
Data acquisition</A>
</H1>
<P>
The angular calibration consists in acquiring a set of diffraction patterns of a well known powder standard (e.g. Silicon) at different encoder positions. In order to facilitate the procedure, the sample should not emit fluorescent light and should present relatively symmetric peaks.
<BR>
During the measurement, a strong intensity peak (e.g. Si(111)) should pass through the field of view of every module such that it can be used as a reference angular position to perform the calibration of the modules position. In general the highest peak will be used for the calibration, but this is not necessary in case there would be e.g. geometrical limitations for shifting the detector.
<BR><B>Do not forget to properly position the beam stopper if the detector is scanned in front of the direct beam.</B>
<BR>
The detector should be shifted of an angular step of the order of about 2% of the module size, such that about 50 patterns can contribute to the fitting of the 3 parameters necessary for the angular calibration.
<BR>
<P>
All the angular calibration procedure should be acquired using a trimmed detector with the threshold set at half of the X-ray energy (Assuming no fluorescent element in the standard). A flat field should also be acquired in order to precisely correct the data, while the X-ray intensity should be kept lower than about 100&nbsp;kHz per strip in order to avoid the need for rate corrections.
<P>
A rough angular conversion file starting from a previous calibration or from the geometric characteristics of the mechanics is an advantage. The angular conversion file should contain a line for each module of the detector with its module number <IMG
WIDTH="10" HEIGHT="17" ALIGN="BOTTOM" BORDER="0"
SRC="img3.png"
ALT="$i$">, center <!-- MATH
$C_{center}^{i}$
-->
<IMG
WIDTH="53" HEIGHT="36" ALIGN="MIDDLE" BORDER="0"
SRC="img7.png"
ALT="$C_{center}^{i}$"> and error, conversion radius <IMG
WIDTH="38" HEIGHT="36" ALIGN="MIDDLE" BORDER="0"
SRC="img13.png"
ALT="$p/R^i$"> and error, offset <IMG
WIDTH="24" HEIGHT="36" ALIGN="MIDDLE" BORDER="0"
SRC="img6.png"
ALT="$\Theta_o^i$"> and error:
<PRE>
module 0 center 639.5 +- 0 conversion 6.56E-05 +- 0 offset 0 +- 0
</PRE>
Also the <I>global offset</I> value of the beamline should be approximately known i.e. the angular position of channel 0 of module 0 when the motor is set at 0.
<BR>
All the documentation assumes that the detector is oriented in the same direction as the encoder position i.e. large channel number at higher angles (both per module and absolute). If this is not the case, the <I>angular direction</I> should be set to -1.
<P>
<H2><A NAME="SECTION00021000000000000000">
Software</A>
</H2>
<P>
For the acquisition ot the data you need to install the slsDetector software package (please refere to separate documentation). The use of the GUI is optional and all operations can be performed also using the text client.
<BR>
<P>
Please make sure that you have edited the
<BR><I>slsDetectorSoftware/usersFunctions/angleFunction.h</I>
<BR>
in order to match the angular conversion for your geometry and
<BR><I>slsDetectorSoftware/usersFunctions/usersFunctions.cpp</I>
<BR>
in order to be able to move the detector and read out its position by using the slsDetector software.
<P>
In the following the command to acquire a dataset for the angular calibration with an exposure time of 1&nbsp;s, and position shift
<PRE>
#setup angular calibration log mode
&gt; sls_detector_put angcallog 1
#set exposure time to 1s
&gt; sls_detector_put exptime 1.
#setup threshold scan
&gt; sls_detector_put scan0script position
#setup the precision for the scan variable in the file name
&gt; sls_detector_put scan0prec 2
#set scan range between 20deg and -60deg, step of -0.1deg
# (at 12.4 keV the Si(111) peak is at approx 19deg
&gt; sls_detector_put scan0range 20 -60 -0.1
#acquire the data
&gt; sls_detector_acquire
#unset angular calibration log mode
&gt; sls_detector_put angcallog 0
</PRE>
<P>
With the GUI you can obtain the same results by clicking on the <I>Angular calibration</I> log button in the advanced tab (see figure&nbsp;<A HREF="#fig:guiangcallog">1</A>) and setting up the motor position scan in the Actions tab (see figure&nbsp;<A HREF="#fig:guiposscan">2</A>). The exposure time should also be set in the measurement tab.
<P>
Additional to the data files, the acquisition will produce a .angcal file containing an header and, for each step of the acquisition, the exect value of the motor position and the file name.
<BR>
In case you forgot to enable the angcallog flag in the software, you can produce the file with the syntax as follows, assuming that you know the exact values of your encoder for each frame:
<PRE>
type Mythen
maxmod 32
nmod 32
angconv /scratch/angcal20120422/ang.off
globaloff 5.088
fineoff 0.0
angdir 1
ffdir /scratch/angcal20120422/
flatfield flatfield_E12keV_T6keV_0.raw
badchannels /scratch/cal/bad.chans
19.99998 angcal_S20.00_0
19.90001 angcal_S19.90_0
19.79999 angcal_S19.80_0
19.70002 angcal_S19.70_0
......
</PRE>
<P>
<DIV ALIGN="CENTER"><A NAME="fig:guiangcallog"></A><A NAME="46"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 1:</STRONG>
Acquisition GUI window to enable the angular calibration log.</CAPTION>
<TR><TD><IMG
WIDTH="555" HEIGHT="603" ALIGN="BOTTOM" BORDER="0"
SRC="img14.png"
ALT="\includegraphics[width=\textwidth]{enable_angcal.eps}"></TD></TR>
</TABLE>
</DIV>
<P>
<DIV ALIGN="CENTER"><A NAME="fig:guiposscan"></A><A NAME="51"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 2:</STRONG>
Acquisition GUI window to setup the motor position scan.</CAPTION>
<TR><TD><IMG
WIDTH="555" HEIGHT="603" ALIGN="BOTTOM" BORDER="0"
SRC="img15.png"
ALT="\includegraphics[width=\textwidth]{position_scan.eps}"></TD></TR>
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<H1><A NAME="SECTION00030000000000000000">
Data analysis</A>
</H1>
<P>
The data analysis consists in fitting with a gaussian the selected peak of the powder pattern for each position in order to determine its position is channel number as a function of the encoder position.
<BR>
In a second step, for each module, the channel vs. encoder curve is fitted in order to extrapolate the three parameters necessary for the angular conversion and the result is written to file
<P>
<H2><A NAME="SECTION00031000000000000000">
Software</A>
</H2>
<P>
The software used for the angular calibration data analysis is based on root (see http://root.cern.ch).
<BR>
This can be downloaded as binary or installed from sources. The version of the software should not play an important role, but up to now everything has been implemented and tested using version 5.20.
<P>
To start the data analysis simply launch:
<PRE>
&gt; ./angularCalibrationWizard
</PRE>
<P>
<DIV ALIGN="CENTER"><A NAME="fig:setangcal"></A><A NAME="60"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 3:</STRONG>
Overview of the nagular calibration dataset.</CAPTION>
<TR><TD><IMG
WIDTH="555" HEIGHT="707" ALIGN="BOTTOM" BORDER="0"
SRC="img16.png"
ALT="\includegraphics[width=\textwidth]{setupAngcal.eps}"></TD></TR>
</TABLE>
</DIV>
<P>
To setup the angular calibration dataset, the .angcal file should be selected (or digited) and the load button should be pressed to confirm. The parameters of the angular calibration are then read to the file and the data loaded for a quick overview (see figure&nbsp;<A HREF="#fig:setangcal">3</A>).
<BR>
The software assumes that the data files (.raw) and the .encal file are in the same directory.
<BR>
A 2D color plot will show a rebinned overview of the dataset. The peak to be fitted should be visible as a high intensity diagonal line passing through all the channels.
<P>
<DIV ALIGN="CENTER"><A NAME="fig:peakfit"></A><A NAME="66"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 4:</STRONG>
Preview of the fitting of the Si(111) peak for one of the detector positions.</CAPTION>
<TR><TD><IMG
WIDTH="555" HEIGHT="707" ALIGN="BOTTOM" BORDER="0"
SRC="img17.png"
ALT="\includegraphics[width=\textwidth]{peakFit.eps}"></TD></TR>
</TABLE>
</DIV>
<P>
For a more detailed view of the data, one can select an angular calibration step from the combo box, select the plot mode (raw data or processed data as a function of channel number, processed angular converted data, flat field data, or again an overview of the whole dataset).
<BR>
By (right) clicking close to the axis you are able to zoom in/out, set the scale to logarithmic etc.
<BR>
<P>
If the bad channel list, angular conversion file or flat field file are changed compared to the acquisition, they can be reloaded by editing the correspondent text entries and pressing enter.
<P>
In particular, the angular converted data should be checked in order to view the position of the selected peak. In this case, the plot will be zoomed to the angular region slected in the minimum and maximum angle entries. By pressing fit, the fit of the peak in the selected angular range will be shown (see figure&nbsp;<A HREF="#fig:peakfit">4</A>). It is useful to check that it works properly in several positions such that then the sequential fitting on all steps can give good results.
<P>
To automatically fit all positions simply press <I>Proceed to Modules Calibration</I> and wait until all steps are fitted. This can take sometime, depending on the number of steps.
<P>
<DIV ALIGN="CENTER"><A NAME="fig:anglefit"></A><A NAME="73"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 5:</STRONG>
Window for fitting the angular calibration parameters of a module.</CAPTION>
<TR><TD><IMG
WIDTH="555" HEIGHT="707" ALIGN="BOTTOM" BORDER="0"
SRC="img18.png"
ALT="\includegraphics[width=\textwidth]{angleFit.eps}"></TD></TR>
</TABLE>
</DIV>
<P>
In the module calibration window (see figure&nbsp;<A HREF="#fig:anglefit">5</A>), you will be able to fit the channel number to encoder position curve to estimate the three angular calibration parameters for each module.
<BR>
The entries show the angular calibration parameters used for approximate angular conversion in the previous step of the calibration. These can be edited and will be used as start parameters for the fit.
By clicking on the check box next to the parameters, the selected parameter will be set and fixed during the fit. Often the center is used as a fix parameter.
<BR>
It is possible to navigate between modules by using the Previous and Next module buttons. To refit the current module (e.g. after changing one of the parameters) simply re-click on the module number.
<P>
After fitting all modules you can click on the <I>Write Angular Calibration</I> button, select the file name to write to and save the calibration angulat calibration data. Please note that the offset of module 0 will always be 0 and the other values will be rescaled to its value. Therefore the global offset of the steup will always need to be specified for a proper angular conversion unless the home of the encoder will not be redifined.
<P>
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Setup calibration files</A>
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To use the generated angular calibration files, using the text client:
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</PRE>
while for the GUI the file name should be specified in the configuration file (works also for the text client).
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<P ALIGN="CENTER"><STRONG>Anna Bergamaschi</STRONG></P>
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<P>
<H1 ALIGN="CENTER">Energy calibration wizard manual</H1>
<DIV>
<P ALIGN="CENTER"><STRONG>Anna Bergamaschi</STRONG></P>
<P ALIGN="CENTER"><STRONG>August 24, 2017</STRONG></P>
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<P>
<BR><HR>
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<LI><A NAME="tex2html11"
HREF="node1.html">Introduction</A>
<LI><A NAME="tex2html12"
HREF="node2.html">Data acquisition</A>
<UL>
<LI><A NAME="tex2html13"
HREF="node2.html#SECTION00021000000000000000">Software</A>
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<LI><A NAME="tex2html14"
HREF="node3.html">Data analysis</A>
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<LI><A NAME="tex2html15"
HREF="node3.html#SECTION00031000000000000000">Software</A>
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<BR>
<LI><A NAME="tex2html16"
HREF="node4.html">Setup calibration files</A>
<LI><A NAME="tex2html17"
HREF="node5.html">About this document ...</A>
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<BR><HR>
<ADDRESS>
Thattil Dhanya
2017-08-24
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<H1><A NAME="SECTION00010000000000000000">
Introduction</A>
</H1>
<P>
The choice of the level of the comparator threshold plays a very important role in counting systems since it influences the efficiency of the detector as well as its spatial resolution (for details see the paper Bergamaschi, A. et al. (2010). J. Synchrotron Rad. 17, 653-668).
<P>
Single-photon-counting detectors are sensitive to single photons and the only limitation on the fluctuations of the number of counts is given by the Poisson-like statistics of the X-ray quanta.
The digitized signal does not carry any information concerning the energy of the X-rays and all photons with an energy larger than the threshold are counted as one bit. This means that the choice of the correct comparator threshold level is critical in order to obtain good-quality data.
<BR>
Figure&nbsp;<A HREF="#fig:thrscanexpl">1</A> shows the expected number of counts as a function of the threshold energy for <IMG
WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img2.png"
ALT="$N_0$"> monochromatic X-rays of energy <IMG
WIDTH="23" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img1.png"
ALT="$E_0$">. This is often denominated S-curve and can be interpreted as the integral of the signal spectrum between the threshold level and infinity.
The dashed curve represents the behavior of an ideal counting system: nothing is counted for thresholds larger than the photon energy and all the <IMG
WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img2.png"
ALT="$N_0$"> X-rays are counted for thresholds lower than <IMG
WIDTH="23" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img1.png"
ALT="$E_0$">.
The thick solid line represents the physical curve which also takes into account the electronic noise and the charge sharing between channels.
<P>
The intrinsic noise on the electronic signal is defined by the Equivalent Noise Charge (<IMG
WIDTH="44" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img3.png"
ALT="$ENC$">). The <IMG
WIDTH="44" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img3.png"
ALT="$ENC$"> describes noise in terms of the charge at the detector input needed to create the same output at the end of the analog chain and is normally expressed in electrons. For silicon sensors, it can be converted into energy units by considering 1&nbsp;<IMG
WIDTH="23" HEIGHT="19" ALIGN="BOTTOM" BORDER="0"
SRC="img12.png"
ALT="$e^-$">=3.6&nbsp;eV.
The value of the <IMG
WIDTH="44" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img3.png"
ALT="$ENC$"> normally depends on the shaping settings of the analog chain and increases with shorter shaping times.
The resulting electronic signal spectrum is then given by a convolution between the radiation spectrum and the noise i.e., a Gaussian of standard deviation <IMG
WIDTH="44" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img3.png"
ALT="$ENC$">.
The S-curve for a monochromatic radiation beam is well described by a Gaussian cumulative distribution <IMG
WIDTH="18" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img13.png"
ALT="$D$"> with an additional increase at low threshold due to the baseline noise, as shown by the solid thin line.
<P>
Moreover, when a photon is absorbed in the region between two strips of the sensor, the generated charge is partially collected by the two nearest electronic channels. For this reason the physical S-curve is not flat but can be modeled by a decreasing straight line. The number of shared photons <IMG
WIDTH="27" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img5.png"
ALT="$N_S$"> is given by the difference between the number of counts and the number of X-rays whose charge is completely collected by the strip (shown by the dotted line).
<P>
The number of counts in the physical case is equal to that in the ideal case for a threshold set at half the photon energy. This defines the optimal threshold level <IMG
WIDTH="78" HEIGHT="32" ALIGN="MIDDLE" BORDER="0"
SRC="img14.png"
ALT="$E_t=E_0/2$">.
<BR>
The detector response <IMG
WIDTH="19" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img15.png"
ALT="$N$"> as a function of the threshold energy <IMG
WIDTH="22" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img10.png"
ALT="$E_t$"> is given by the sum of the noise counts <IMG
WIDTH="26" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img16.png"
ALT="$N_n$"> and the counts originating from photons <IMG
WIDTH="25" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img17.png"
ALT="$N_\gamma$">:
<BR>
<DIV ALIGN="RIGHT">
<!-- MATH
\begin{equation}
N_\gamma(E_t)=\frac{N_0}{2}\cdot\Big(1+C_s \frac{E_0-2E_t}{E_0}\Big)D \Big(\frac{E_0-E_t}{ENC} \Big),
\end{equation}
-->
<TABLE WIDTH="100%" ALIGN="CENTER">
<TR VALIGN="MIDDLE"><TD ALIGN="CENTER" NOWRAP><A NAME="eq:thrscan"></A><IMG
WIDTH="335" HEIGHT="41" BORDER="0"
SRC="img18.png"
ALT="\begin{displaymath}
N_\gamma(E_t)=\frac{N_0}{2}\cdot\Big(1+C_s \frac{E_0-2E_t}{E_0}\Big)D \Big(\frac{E_0-E_t}{ENC} \Big),
\end{displaymath}"></TD>
<TD WIDTH=10 ALIGN="RIGHT">
(1)</TD></TR>
</TABLE>
<BR CLEAR="ALL"></DIV><P></P>
where <IMG
WIDTH="23" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img19.png"
ALT="$C_s$"> is the fraction of photons which produce a charge cloud which is shared between neighboring strips (<IMG
WIDTH="83" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img20.png"
ALT="$N_s=C_s N_0$">).
<BR>
By assuming a noise of Gaussian type, and considering its bandwidth limited by the shaping time <IMG
WIDTH="18" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img21.png"
ALT="$\tau_s$">, the number of noise counts in the acquisition time <IMG
WIDTH="16" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img22.png"
ALT="$T$"> can be approximated as:
<BR>
<DIV ALIGN="RIGHT">
<!-- MATH
\begin{equation}
N_n(E_t) \sim \frac{T}{\tau_s} D \Big(\frac{-E_t}{ENC} \Big).
\end{equation}
-->
<TABLE WIDTH="100%" ALIGN="CENTER">
<TR VALIGN="MIDDLE"><TD ALIGN="CENTER" NOWRAP><A NAME="eq:noisescan"></A><IMG
WIDTH="169" HEIGHT="41" BORDER="0"
SRC="img23.png"
ALT="\begin{displaymath}
N_n(E_t) \sim \frac{T}{\tau_s} D \Big(\frac{-E_t}{ENC} \Big).
\end{displaymath}"></TD>
<TD WIDTH=10 ALIGN="RIGHT">
(2)</TD></TR>
</TABLE>
<BR CLEAR="ALL"></DIV><P></P>
<P>
The choice of the comparator threshold level <IMG
WIDTH="22" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img10.png"
ALT="$E_t$"> influences not only the counting efficiency and noise performances, but also the spatial resolution and the counting statistics of the detector.
If the threshold is set at values higher than the ideal value <IMG
WIDTH="78" HEIGHT="32" ALIGN="MIDDLE" BORDER="0"
SRC="img14.png"
ALT="$E_t=E_0/2$">, a fraction of the photons absorbed in the sensor in the region between two strips is not counted thus reducing the detector efficiency but improving its spatial resolution (narrower strip size). On the other hand, if the threshold is set at values lower than <IMG
WIDTH="22" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img10.png"
ALT="$E_t$">, part of the X-rays absorbed in the region between two strips are counted by both of them, resulting in a deterioration of the spatial resolution of the detector and of the fluctuations on the number of photons because of the increased multiplicity.
<P>
Furthermore, the threshold uniformity is particularly critical with regards to fluorescent radiation emitted by the sample under investigation. Since the emission of fluorescent light is isotropic, the data quality will be improved by setting the threshold high enough in order to discard the fluorescence background (see figure&nbsp;<A HREF="#fig:thrscanfluo">3</A>).
<BR>
Moreover, setting the threshold too close to the energy of the fluorescent light gives rise to large fluctuations between channels in the number of counts since the threshold sits on the steepest part of the threshold scan curve for the fluorescent background. These differences cannot be corrected by using a flat-field normalization since the fluorescent component is not present in the reference image. For this reason, it is extremely important that the threshold uniformity over the whole detector is optimized. The threshold level must be set at least <IMG
WIDTH="88" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img24.png"
ALT="$\Sigma&gt;3\,ENC$"> away from both the fluorescent energy level and the X-ray energy in order to remove the fluorescence background while efficiently count the diffracted photons.
<P>
The comparator threshold is given by a global level which can be set on a module basis and adds to a component which is individually adjustable for each channel. In order to optimize the uniformity of the detector response it is important to properly adjust the threshold for all channels.
<BR>
Since both the signal amplification stages and the comparator are linear, it is necessary to calibrate the detector offset <IMG
WIDTH="17" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img25.png"
ALT="$O$"> and gain <IMG
WIDTH="17" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img26.png"
ALT="$G$"> in order to correctly set its comparator threshold <IMG
WIDTH="19" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img27.png"
ALT="$V_t$"> at the desired energy <IMG
WIDTH="22" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img10.png"
ALT="$E_t$">:
<BR>
<DIV ALIGN="RIGHT">
<!-- MATH
\begin{equation}
V_{t}=O+G \cdot E_t.
\end{equation}
-->
<TABLE WIDTH="100%" ALIGN="CENTER">
<TR VALIGN="MIDDLE"><TD ALIGN="CENTER" NOWRAP><A NAME="eq:encal"></A><IMG
WIDTH="111" HEIGHT="26" BORDER="0"
SRC="img28.png"
ALT="\begin{displaymath}
V_{t}=O+G \cdot E_t.
\end{displaymath}"></TD>
<TD WIDTH=10 ALIGN="RIGHT">
(3)</TD></TR>
</TABLE>
<BR CLEAR="ALL"></DIV><P></P>
This is initially performed by acquiring measurements while scanning the global threshold using different X-ray energies and calculating the median of the counts at each threshold value for each module <IMG
WIDTH="10" HEIGHT="17" ALIGN="BOTTOM" BORDER="0"
SRC="img29.png"
ALT="$i$">. The curves obtained for one of the detector modules at three energies are shown in figure&nbsp;<A HREF="#fig:modulecalibration">4</A>. The experimental data are then fitted according to equation&nbsp;<A HREF="#eq:thrscan">1</A> and for each module a linear relation is found between the X-ray energy and the estimated inflection point, as shown in the inset of figure&nbsp;<A HREF="#fig:modulecalibration">4</A>. The resulting offset <IMG
WIDTH="22" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img30.png"
ALT="$O_i$"> and gain <IMG
WIDTH="22" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img31.png"
ALT="$G_i$"> are used as a conversion factor between the threshold level and the energy.
<P>
<DIV ALIGN="CENTER"><A NAME="fig:thrscanexpl"></A><A NAME="116"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 1:</STRONG>
Expected counts as a function of a threshold energy for a monochromatic beam of energy <IMG
WIDTH="23" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img1.png"
ALT="$E_0$">=12&nbsp;keV. <IMG
WIDTH="24" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img2.png"
ALT="$N_0$">=10000 is the number of photons absorbed by the detector during the acquisition time. The dashed line represents the curve in an ideal case without electronic noise and charge sharing, the solid thin line with noise <IMG
WIDTH="44" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img3.png"
ALT="$ENC$">=1&nbsp;keV but without charge sharing and the solid thick line is the physical case with noise and <IMG
WIDTH="45" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img4.png"
ALT="$CS=$">22&nbsp;% charge sharing. <IMG
WIDTH="27" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img5.png"
ALT="$N_S$"> is the number of photons whose charge is shared between neighbouring strips (<!-- MATH
$CS=\frac{N_S}{N_0}$
-->
<IMG
WIDTH="71" HEIGHT="38" ALIGN="MIDDLE" BORDER="0"
SRC="img32.png"
ALT="$CS=\frac{N_S}{N_0}$">). The dotted line represents the number of photons whose charge is completely collected by a single strip.</CAPTION>
<TR><TD><IMG
WIDTH="556" HEIGHT="539" ALIGN="BOTTOM" BORDER="0"
SRC="img33.png"
ALT="\includegraphics[width=\textwidth]{fig4.eps}"></TD></TR>
</TABLE>
</DIV>
<P>
<DIV ALIGN="CENTER"><A NAME="fig:expthrscan"></A><A NAME="117"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 2:</STRONG>
Measured threshold scan at 12.5&nbsp;keV with the three different settings. In the inset the fit of the experimental data with the expected curve as in function&nbsp;<A HREF="#eq:thrscan">1</A> is shown in the region of the inflection point.</CAPTION>
<TR><TD><IMG
WIDTH="556" HEIGHT="539" ALIGN="BOTTOM" BORDER="0"
SRC="img34.png"
ALT="\includegraphics[width=\textwidth]{fig5.eps}"></TD></TR>
</TABLE>
</DIV>
<P>
<DIV ALIGN="CENTER"><A NAME="fig:thrscanfluo"></A><A NAME="53"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 3:</STRONG>
Number of counts as a function of the threshold measured from a sample containing iron (<IMG
WIDTH="25" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img7.png"
ALT="$E_f$">=5.9&nbsp;keV) when using X-rays of energy <IMG
WIDTH="23" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img1.png"
ALT="$E_0$">=12&nbsp;keV. In this case, setting the threshold at <IMG
WIDTH="39" HEIGHT="32" ALIGN="MIDDLE" BORDER="0"
SRC="img8.png"
ALT="$E_0/2$">, which is very close to <IMG
WIDTH="25" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img7.png"
ALT="$E_f$">, would give <IMG
WIDTH="35" HEIGHT="14" ALIGN="BOTTOM" BORDER="0"
SRC="img9.png"
ALT="$\Delta \sim $">10% counts from the fluorescense background. Therefore the threshold should be set at an intermediate level <IMG
WIDTH="22" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img10.png"
ALT="$E_t$"> between the two energy components with a distance of at least <IMG
WIDTH="85" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img11.png"
ALT="$\Sigma &gt;3ENC$"> from both <IMG
WIDTH="25" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img7.png"
ALT="$E_f$"> and <IMG
WIDTH="23" HEIGHT="30" ALIGN="MIDDLE" BORDER="0"
SRC="img1.png"
ALT="$E_0$">.</CAPTION>
<TR><TD><IMG
WIDTH="556" HEIGHT="553" ALIGN="BOTTOM" BORDER="0"
SRC="img35.png"
ALT="\includegraphics[width=\textwidth]{fig7.eps}"></TD></TR>
</TABLE>
</DIV>
Differences in gain and offset are present also between individual channels within a module and therefore the use of threshold equalization techniques (trimming) using the internal 6-bit DAC is needed in order to reduce the threshold dispersion.
Since both gain and offset have variations between channels, the optimal trimming should be performed as a function of the threshold energy.
Please not that trimming of the channels of the detector should be performed in advanced and is extremely important for a succeful energy calibration of the detector.
<P>
All energy calibration procedures should be applied to a trimmed detector and only an improvement of the existing trimbits can be performed afterwards, since it does not significatively affect the energy calibration.
<P>
<DIV ALIGN="CENTER"><A NAME="fig:modulecalibration"></A><A NAME="118"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 4:</STRONG>
Median of the number of counts as a function of the threshold for X-rays of 12.5, 17.5 and 25&nbsp;keV for one of the detector modules using <I>standard</I> settings. The solid line represents the fit of the experimental points with equation&nbsp;<A HREF="#eq:thrscan">1</A>. In the inset the linear fit between the X-ray energy and the position of the inflection point of the curves is shown.</CAPTION>
<TR><TD><IMG
WIDTH="556" HEIGHT="539" ALIGN="BOTTOM" BORDER="0"
SRC="img36.png"
ALT="\includegraphics[width=\textwidth]{fig8.eps}"></TD></TR>
</TABLE>
</DIV>
<P>
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<H1><A NAME="SECTION00020000000000000000">
Data acquisition</A>
</H1>
<P>
The energy calibration consists in acquiring threshold scans using the detector at at least 2 (better 3) energies. A monochromatic beam is ideal in this procedure, but beam obtained from some fluorescent sample is also good.
<BR>
Please note that the statistic is important to succesfully analyze the data. Normally the exposure time for each step should be chosen in order to achieve at least 1000 counts per step.
If this is not possible it is better to reduce the scan range or enlarge the scan step rather than acquiring data with a too low statics.
<P>
With a quick acquisition or threshold scan it is useful to define the range of the scan and the exposure time. It is important to start from a threshold high enough that (almost) all channels of the detector have a negligible number of counts and that the plateau of the S-curve is long enough to correctly estimate the number of photons.
<P>
<H2><A NAME="SECTION00021000000000000000">
Software</A>
</H2>
<P>
For the acquisition ot the data you need to install the slsDetector software package (please refere to separate documentation). The use of the GUI is optional and all operations can be performed also using the text client.
<BR>
<P>
In the following the command to acquire a dataset for the energy calibration with an exposure time of 1&nbsp;s, and threshold scan range between 200 and 850 with a setp of 1 DAC unit.
<PRE>
&gt; sls_detector_put encallog 1 #setup energy calibration
&gt; sls_detector_put exptime 1. #set exposure time to 1s
&gt; sls_detector_put scan0script threshold #setup threshold scan
&gt; sls_detector_put scan0range 200 850 1 #set scan range between 200 and 850, step of 1
&gt; sls_detector_acquire #acquire the data
&gt; sls_detector_put encallog 0 #unset energy calibration
</PRE>
<P>
With the GUI you can obtain the same results by clicking on the <I>Energy Calibration</I> log button in the advanced tab (see figure&nbsp;<A HREF="#fig:guiencallog">5</A>) and setting up the threshold scan in the Actions tab (see figure&nbsp;<A HREF="#fig:guithrscan">6</A>). the exposure time should also be set in the measurement tab.
<P>
This procedure should be executed at at least 2 (better 3) energies.
<P>
Additional to the data files, the acquisition will produce a .encal file containing an header and, for each step of the acquisition, the threshold value and the file name.
<BR>
In case you forgot to enable the encallog flag in the software, you can produce the file with the syntax as follows:
<PRE>
settings standard
type Mythen+
nmod 12
modulenumber:0 000
modulenumber:1 111
modulenumber:2 222
modulenumber:3 333
modulenumber:4 444
modulenumber:5 555
modulenumber:6 666
modulenumber:7 777
modulenumber:8 888
modulenumber:9 999
modulenumber:10 aaa
modulenumber:11 bbb
450 standard_12_4keV_S450_0
460 standard_12_4keV_S460_0
470 standard_12_4keV_S470_0
480 standard_12_4keV_S480_0
490 standard_12_4keV_S490_0
500 standard_12_4keV_S500_0
510 standard_12_4keV_S510_0
520 standard_12_4keV_S520_0
...
...
</PRE>
<P>
<DIV ALIGN="CENTER"><A NAME="fig:guiencallog"></A><A NAME="73"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 5:</STRONG>
Acquisition GUI window to enable the energy calibration log.</CAPTION>
<TR><TD><IMG
WIDTH="555" HEIGHT="603" ALIGN="BOTTOM" BORDER="0"
SRC="img37.png"
ALT="\includegraphics[width=\textwidth]{GUI_Advanced.eps}"></TD></TR>
</TABLE>
</DIV>
<P>
<DIV ALIGN="CENTER"><A NAME="fig:guithrscan"></A><A NAME="78"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 6:</STRONG>
Acquisition GUI window to setup the threshold scan.</CAPTION>
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WIDTH="555" HEIGHT="603" ALIGN="BOTTOM" BORDER="0"
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Data analysis</A>
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<P>
The data analysis consists in fitting the S-curves obtained from the datasets acquired as above and then performing a linear fit between the energy values and the inflection points.
<P>
<H2><A NAME="SECTION00031000000000000000">
Software</A>
</H2>
<P>
The software used for the energy calibration data analysis is based on root (see http://root.cern.ch).
<BR>
This can be downloaded as binary or installed from sources. The version of the software should not play an important role, but up to now everything has been implemented and tested using version 5.20.
<P>
To start the data analysis simply launch:
<PRE>
&gt; ./energyCalibrationWizard
</PRE>
<P>
To add anew energy write the energy value and select (or digit) the name of the .encal file corresponding to that energy (see figure&nbsp;<A HREF="#fig:addenergy">7</A>).
<BR>
The software assumes that the data files (.raw) and the .encal file are in the same directory.
Press <I>Preview</I> and a 2D color plot will be displayed, showing the channel numbers on the X-axis, the threshold on the Y-axis, and the number of counts as a color scale.
By (right) clicking close to the axis you are able to zoom in/out, set the scale to logarithmic etc.
<BR>
If the plot corresponds to your expectations press <I>Add to list</I>. The energy value will be shown in the combo box on top and labels will display the settings of the detector, the number of modules, the number of channels per module and the modules serial numbers.
<P>
Add then all the other energies to the calibration always by editing the energy value and .encal file name, pressing <I>preview</I> and <I>add to list</I>.
<BR>
If the settings, number of modules or serial numbers do not match, you will not be llowed to add the energy.
<BR>
By using the <I>selected energy actions</I> you can navigate in the combo box with list of energies, view the plots and eventually remove the ones you don't want to use in your calibration.
<BR>
Once you have uploaded at least 2 energies, you will be allowed to <I>proceed to module calibration</I>.
<P>
<DIV ALIGN="CENTER"><A NAME="fig:addenergy"></A><A NAME="94"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 7:</STRONG>
Window to add energies to the calibration.</CAPTION>
<TR><TD><IMG
WIDTH="555" HEIGHT="694" ALIGN="BOTTOM" BORDER="0"
SRC="img39.png"
ALT="\includegraphics[width=\textwidth]{addEnergy.eps}"></TD></TR>
</TABLE>
</DIV>
<P>
In the module calibration window (see figure&nbsp;<A HREF="#fig:calibratemodule">8</A>), you are still able to look at the calibration summary, and eventually return to the previous windown by pressing <I>Back to energy setup</I>.
<BR>
The canvas will show the plot of the S-curves relative to the median of the selected module, fitted with equation&nbsp;<A HREF="node1.html#eq:thrscan">1</A> and the linear fit between the energy values and the fitted inflection points.
Normally the points lie on a straight line (although often not perfect), therefore it should be simple to spot if there are problems in the fitting of some of the data.
<BR>
If <I>Manual save</I> is unclicked, the calibration files will be saved locally, with the extension automatically generated by using the modules serial numbers, every time a linear fit is performed (i.e. if you mess up wiht the linear fit you overwrite a previous good file!). If you click the checkbox, you need to save the calibration by pressing <I>Write to file</I> for each module once you are happy with the fit.
<P>
To change the Y scale of the plot, edit the <I>Counts</I> entry. After clicking of the energy button (eventually twice) the maximum of the histogram will be set to three times the value.
<P>
To re-fit one energy with modified range or start parameters, you should press the central button with the energy value once the energy is selected. The text color tells you which curve you are referring to.
<BR>
<P>
You should set the range of the fit. In particular the maximum should be limited in order to avoid to enter the noise range (and can be pretty different for the various modules).
<BR>
Normally the data are acquired by collecting holes from the detector and therefore the <I>Invert axis</I> check button should be ckecked. Uncheck it in case your detector collects electrons (e.g. CdTe, Si n in p)
<P>
You can change the start values of the parameters of the fits by editing the number eneries. The label nearby will show you the actual value of the fitted parameters.
<BR>
By checking the checkboxes you can fix the values to the ones you specify.
<BR>
Normally it can be useful to fix the pedestal and pedestal slope to 0, unless you have a lot of 3rd armnonics contribution, primary beam background or similar.
<BR>
Changing the starting value of the inflection point or of the number of counts can often help the fit to converge.
<BR>
Normally it is not very useful to change the starting value for the noise or charge sharing slope.
<P>
The button <I>Finished</I> will be enebled only once the calibration files have been generated for all modules.
<P>
<DIV ALIGN="CENTER"><A NAME="fig:calibratemodule"></A><A NAME="107"></A>
<TABLE>
<CAPTION ALIGN="BOTTOM"><STRONG>Figure 8:</STRONG>
Window to calibrate the modules.</CAPTION>
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Setup calibration files</A>
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<P>
To use the genrated calibration files as default ones, copy them into your default <I>caldir/settings</I> renaming them calibration.snxxx, where snxxx is the extension that the genrated files already have, which corresponds to the module serial number.
<BR>
Fot this scope, a script as following can be used:
<PRE>
for i in $(ls newcal_standard.sn* | awk -F "." '{print $2}'); do \
mv newcal_standard.$i caldir/standard/calibration.$i; \
done
</PRE>
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By reloading the default detector settings, the calibration coefficients will be automatically loaded.
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<h1><a class="anchor" id="acquisition">Acquition commands </a></h1><p>Commands to control the acquisition</p>
<ul>
<li><b>acquire</b> blocking acquisition (like calling sls_detector_acquire). Starts receiver and detector, writes and processes the data, stops detector. Only get! <code>Returns</code> (string)<code>"acquire unsuccessful"</code> if fails, else "" for MYTHEN, <code>"Acquired (int)"</code> for others, where int is number of frames caught.</li>
</ul>
<ul>
<li><b>busy</b> returns <code>1</code> if the acquisition is active, <code>0</code> otherwise. Works when the acquisition is started in blocking mode. Only get! <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b> status [s] </b> starts or stops acquisition in detector in non blocking mode. <code>s:</code> [<code>start</code>, <code>stop</code>]. <code>Returns</code> the detector status: [<code>running</code>, <code>error</code>, <code>transmitting</code>, <code>finished</code>, <code>waiting</code>, <code>idle</code>]. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>data</b> gets all data from the detector (if any) processes them and writes them to file according to the preferences already setup (MYTHEN only). Only get!</li>
</ul>
<ul>
<li><b>frame</b> gets a single frame from the detector (if any) processes it and writes it to file according to the preferences already setup (MYTHEN only). Only get!</li>
</ul>
<ul>
<li><b>readctr </b> Reads the counters from the detector memory (analog detector returning values translated into number of photons - only GOTTHARD). Cannot put.</li>
</ul>
<ul>
<li><b>resetctr i </b> Resets counter in detector, restarts acquisition if i=1(analog detector returning values translated into number of photons - only GOTTHARD). Cannot put.</li>
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<ul>
<li><b>resmat i </b> sets/resets counter bit in detector.gets the counter bit in detector ???? </li>
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<h1><a class="anchor" id="actions">Actions </a></h1><p>Commands to define scripts to be executed during the acquisition flow</p>
<ul>
<li><b>positions [n [p0..pn-1]]</b> sets/gets number of angular position and positions to be acquired.. <code>Returns</code> <code></code>(int int..) n [p0..pn-1]</li>
</ul>
<ul>
<li><b>startscript [s]</b> sets/gets the script to be executed at the beginning of the acquisition. <code>none</code> unsets. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>startscriptpar [s]</b> sets/gets a string to be passed as a parameter to the startscript. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>stopscript [s]</b> sets/gets the script to be executed at the end of the acquisition. <code>none</code> unsets. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>stopscriptpar [s]</b> sets/gets a string to be passed as a parameter to the stopscript. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>scriptbefore [s]</b> sets/gets the script to be executed before starting the detector every time in the acquisition. <code>none</code> unsets. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>scriptbeforepar [s]</b> sets/gets a string to be passed as a parameter to the scriptbefore. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>scriptafter [s]</b> sets/gets the script to be executed after the detector has finished every time in the acquisition. <code>none</code> unsets. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>scriptafterpar [s]</b> sets/gets a string to be passed as a parameter to the scriptafter. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>headerafter [s]</b> sets/gets the script to be executed for logging the detector parameters. <code>none</code> unsets. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>headerbefore [s]</b> sets/gets the script to be executed for logging the detector parameters. <code>none</code> unsets. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>headerbeforepar [s]</b> sets/gets a string to be passed as a parameter to the headerbefore script. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>headerafterpar [s]</b> sets/gets a string to be passed as a parameter to the headerafter script. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>enacallog [i]</b> enables/disables logging of the parameters necessary for the energy calibration. 1 sets, 0 unsets. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>angcallog [i]</b> enables/disables logging of the parameters necessary for the angular calibration. 1 sets, 0 unsets. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>scan0script [s]</b> sets/gets the script to be executed for the scan 0 level. <code>none</code> unsets.</li>
</ul>
<ul>
<li><b>scan0par [s]</b> sets/gets a string to be passed as a parameter to the scan0script</li>
</ul>
<ul>
<li><b>scan0prec [i]</b> sets/gets number of digits to be used for the scan0 variable in the file name.</li>
</ul>
<ul>
<li><b>scan0steps [i [s0..sn-1]]</b> sets/gets number of steps (int) of the scan0 level and their values (float).</li>
</ul>
<ul>
<li><b>scan0range [smin smax sstep]</b> sets scan0 min, max and step, returns the number of steps and their values as scan0steps.</li>
</ul>
<ul>
<li><b>scan1script [s]</b> sets/gets the script to be executed for the scan1 level. <code>none</code> unsets.</li>
</ul>
<ul>
<li><b>scan1par [s]</b> sets/gets a string to be passed as a parameter to the scan1script</li>
</ul>
<ul>
<li><b>scan1prec [i]</b> sets/gets number of digits to be used for the scan1 variable in the file name.</li>
</ul>
<ul>
<li><b>scan1steps [i [s0..sn-1]]</b> sets/gets number of steps (int) of the scan1 level and their values (float).</li>
</ul>
<ul>
<li><b>scan1range [smin smax sstep]</b> sets scan1 min, max and step, returns the number of steps and their values as scan1steps. </li>
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<h1><a class="anchor" id="advanced">Advanced Usage </a></h1><p>This page is for advanced users. Make sure you have first read the introduction. </p>
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<h1><a class="anchor" id="config">Configuration commands </a></h1><p>Commands to configure the detector. these commands are often left to the configuration file.</p>
<ul>
<li><a class="el" href="config.html#configstructure">Data Structure</a>: commands to configure detector data structure</li>
<li><a class="el" href="config.html#configstatus">Status</a>: commands to configure detector status</li>
<li><a class="el" href="config.html#configsize">Data Size</a>: commands to configure detector data size</li>
<li><a class="el" href="config.html#configflags">Flags</a>: commands to configure detector flags</li>
<li><a class="el" href="config.html#configchip">Chip</a>: commands to configure chip of the detector</li>
<li><a class="el" href="config.html#configversions">Versions</a>: commands to check version of each subsytem</li>
<li><a class="el" href="config.html#configspeed">Speed</a>: commands to configure speed of detector</li>
<li><a class="el" href="config.html#configsettings">Detector Parameters</a>: commands to configure/retrieve configuration of detector</li>
</ul>
<h2><a class="anchor" id="configstructure">
Data Structure</a></h2>
<p>commands to configure detector data structure</p>
<ul>
<li><b> externalgui </b>sets/gets external gui flag. 1 sets and enables the 0MQ data stream (0MQ threads created) from receiver to client, while 0 unsets and disables. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>free</b> Free shared memory on the control PC</li>
</ul>
<ul>
<li><b>add</b> Adds a detector at the end of the multi-detector structure. <code>put</code> argument is the hostname or IP adress. Returns the chained list of detector hostnames.</li>
</ul>
<ul>
<li><b>remove i</b> Removes controller <code>i</code> from the multi-detector structure. Can be used for partial readout of the detector.</li>
</ul>
<ul>
<li><b>type</b> Sets/gets detector type. <code>Returns</code> <code></code>(string). Normally not used. Using hostname is enough.</li>
</ul>
<ul>
<li><b>hostname</b> <code>put</code> adds the hostname (ot IP adress) at the end of the multi-detector structure. If used for a single controlled (i:) replaces the current hostname. Returns the list of the hostnames of the multi-detector structure. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>id[:i]</b> Returns the id of the detector structure. i is the detector position in a multi detector system. If used a <code>put</code>, configures the id of the detector structure. i is the detector position in a multi detector system and l is the id of the detector to be added.</li>
</ul>
<ul>
<li><b>master i</b> <code>put</code> sets the position of the master of the acquisition (-1 if none). Returns the position of the master of the detector structure (-1 if none).</li>
</ul>
<ul>
<li><b>sync</b> Sets/gets the synchronization mode of the detectors in the multi-detector structure. Can be: <code>none</code>, <code>gating</code>, <code>trigger</code>, <code>complementary</code>. Mainly used by MYTHEN/GOTTHARD.</li>
</ul>
<h2><a class="anchor" id="configstatus">
Status</a></h2>
<p>commands to configure detector status</p>
<ul>
<li><b>online [i]</b> sets the detector in online (1) or offline (0) mode. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>checkonline</b> returns the hostnames of all detectors without connecting to them. <code>Returns</code> (string) "All online" or "[list of offline hostnames] : Not online".</li>
</ul>
<ul>
<li><b>activate</b> Activates/Deactivates the detector. Deactivated detector does not send data. Used for EIGER only. <code>Returns</code> <code></code>(int)</li>
</ul>
<h2><a class="anchor" id="configsize">
Data Size</a></h2>
<p>commands to configure detector data size</p>
<ul>
<li><b>nmod [i]</b> sets/gets the number of modules of the detector. Used for MYTHEN only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>maxmod </b> Gets the maximum number of modules of the detector. Used for MYTHEN only. Cannot put! <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>dr [i]</b> sets/gets the dynamic range of detector. Mythen [4,8,16,24]. Eiger [4,8,16,32]. Others cannot put! <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>roi [i] [xmin] [xmax] [ymin] [ymax] </b> sets region of interest of the detector, where i is number of rois;i=0 to clear rois. Used for GOTTHARD only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>detsizechan [xmax] [ymax]</b> sets the maximum number of channels in each dimension for complete detector set; -1 is no limit. Use for multi-detector system as first command in config file. <code>Returns</code> <code></code>("int int")</li>
</ul>
<ul>
<li><b>roimask [i]</b> ?? <code>Returns</code> <code></code>(int) in hexadecimal</li>
</ul>
<ul>
<li><b>flippeddatax [i]</b> enables/disables data being flipped across x axis. 1 enables, 0 disables. Used for EIGER only. 1 for bottom half-module, 0 for top-half module. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>tengiga [i]</b> enables/disables 10GbE in system (detector &amp; receiver). 1 enabled 10GbE, 0 enables 1GbE. Used in EIGER only. <code>Returns</code> <code></code>(int)</li>
</ul>
<h2><a class="anchor" id="configflags">
Flags</a></h2>
<p>commands to configure detector flags</p>
<ul>
<li><b>flags [flag]</b> sets/gets the readout flags to mode. Options: none, storeinram, tot, continous, parallel, nonparallel, safe, digital, analog_digital, unknown. Used for MYTHEN and EIGER only. <code>Returns</code> <code></code>(string). put takes one string and <code>returns</code> concatenation of all active flags separated by spaces.</li>
</ul>
<ul>
<li><b>extsig:[i] [flag]</b> sets/gets the mode of the external signal i. Options: <code>off</code>, <code>gate_in_active_high</code>, <code>gate_in_active_low</code>, <code>trigger_in_rising_edge</code>, <code>trigger_in_falling_edge</code>, <code>ro_trigger_in_rising_edge</code>, <code>ro_trigger_in_falling_edge</code>, <code>gate_out_active_high</code>, <code>gate_out_active_low</code>, <code>trigger_out_rising_edge</code>, <code>trigger_out_falling_edge</code>, <code>ro_trigger_out_rising_edge</code>, <code>ro_trigger_out_falling_edge</code>. <br/>
Used in MYTHEN, GOTTHARD, PROPIX only. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>programfpga [file]</b> programs the FPGA with file f (with .pof extension). Used for JUNGFRAU, MOENCH only. Only put! <code>Returns</code> <code></code>("successful", "unsuccessful")</li>
</ul>
<ul>
<li><b>resetfpga [f]</b> resets FPGA, where f can be any value. Used for JUNGFRAU only. Only put! <code>Returns</code> <code></code>("successful", "unsuccessful")</li>
</ul>
<h2><a class="anchor" id="configchip">
Chip</a></h2>
<p>commands to configure chip of the detector</p>
<ul>
<li><b>powerchip [i]</b> Powers on/off the chip. 1 powers on, 0 powers off. Can also get the power status. Used for JUNGFRAU only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>led [i]</b> sets/gets the led status. 1 on, 0 off. Used for MOENCH only ?? <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>pulse [n] [x] [y]</b> pulses pixel at coordinates (x,y) n number of times. Used in EIGER only. Only put! <code>Returns</code> <code></code>("successful", "unsuccessful")</li>
</ul>
<ul>
<li><b>pulsenmove [n] [x] [y]</b> pulses pixel n number of times and moves relatively by x value (x axis) and y value(y axis). Used in EIGER only. Only put! <code>Returns</code> <code></code>("successful", "unsuccessful")</li>
</ul>
<ul>
<li><b>pulsechip [n]</b>pulses chip n number of times, while n=-1 will reset it to normal mode. Used in EIGER only. Only put! <code>Returns</code> <code></code>("successful", "unsuccessful")</li>
</ul>
<h2><a class="anchor" id="configversions">
Versions</a></h2>
<p>Commands to check versions of each subsystem</p>
<ul>
<li><b>moduleversion:[i]</b> Gets the firmware version of module i. Used for MYTHEN only. Only get! <code>Returns</code> <code></code>(long int) in hexadecimal or "undefined module number"</li>
</ul>
<ul>
<li><b>detectornumber</b> Gets the serial number or MAC of detector. Only get! <code>Returns</code> <code></code>(long int) in hexadecimal</li>
</ul>
<ul>
<li><b>modulenumber:[i]</b> Gets the serial number of module i. Used for MYTHEN only. Only get! <code>Returns</code> <code></code>(long int) in hexadecimal or "undefined module number"</li>
</ul>
<ul>
<li><b>detectorversion</b> Gets the firmware version of detector. Only get! <code>Returns</code> <code></code>(long int) in hexadecimal</li>
</ul>
<ul>
<li><b>softwareversion</b> Gets the software version of detector server. Only get! <code>Returns</code> <code></code>(long int) in hexadecimal</li>
</ul>
<ul>
<li><b>thisversion</b> Gets the software version of this client software. Only get! <code>Returns</code> <code></code>(long int) in hexadecimal</li>
</ul>
<ul>
<li><b>receiverversion</b> Gets the software version of receiver. Only get! <code>Returns</code> <code></code>(long int) in hexadecimal</li>
</ul>
<ul>
<li><b>framesl</b> gets number of frames left. Used in MYTHEN, GOTTHARD only. Only get! <code>Returns</code> <code></code>(double with 9 decimal digits)</li>
</ul>
<h2><a class="anchor" id="configspeed">
Speed</a></h2>
<p>commands to configure speed of detector</p>
<ul>
<li><b>clkdivider [i]</b> sets/gets the readout clock divider. EIGER, JUNGFRAU [0(fast speed), 1(half speed), 2(quarter speed)]. MYTHEN[???]. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>setlength [i]</b> sets/gets length of set/reset signals (in clock cycles). Used in MYTHEN only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>waitstates [i]</b> sets/gets waitstates of the bus interface (in clock cycles). Used in MYTHEN only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>totdivider [i]</b> sets/gets clock divider in tot mode. Used in MYTHEN only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>totdutycycle [i]</b> sets/gets duty cycle of the tot clock. Used in MYTHEN only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>phasestep [i]</b> Only put for gotthard. Moves the phase of the ADC clock.<code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>oversampling [i]</b> Sets/gets the number of adcsamples per clock. For the new chiptestboard.<code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>adcclk [i]</b> sets/gets the ADC clock frequency in MHz. For the new chiptestboard!<code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>adcphase [i]</b> Sets/gets the ADC clock frequency in MHz. For the new chiptestboard!<code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>adcpipeline [i]</b> Sets/gets the pipeline of the ADC. For the new chiptestbaord!<code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>dbitclk [i]</b> Sets/gets the clock frequency of the latching of the digital bits in MHz. For the new chiptestboard!<code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>dbitphase [i]</b> Sets/gets the phase of the clock for latching of the digital bits. For the new chiptestboard!?<code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>dbitpipeline [i]</b> Sets/gets the pipeline of the latching of the digital bits. For the new chiptestbaord!<code>Returns</code> <code></code>(int)</li>
</ul>
<h2><a class="anchor" id="configsettings">
Detector Parameters</a></h2>
<p>commands to configure/retrieve configuration of detector</p>
<ul>
<li><b>config [fname]</b> sets/saves detector/receiver to configuration contained in fname. Same as executing sls_detector_put for every line. Normally a one time operation. <code>Returns</code> <code></code>(string) fname</li>
</ul>
<ul>
<li><b>rx_printconfig</b> prints the receiver configuration. Only get! <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>parameters [fname]</b> sets/saves detector parameters contained in fname. Normally once per different measurement. <code>Returns</code> <code></code>(string) fname</li>
</ul>
<ul>
<li><b>setup [fname]</b> sets/saves detector complete setup contained in fname (extensions automatically generated), including trimfiles, ff coefficients etc. <code>Returns</code> <code></code>(string) fname </li>
</ul>
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<h1><a class="anchor" id="ctb">Chiptest board </a></h1><p>Commands specific for the new chiptest board as pattern generator</p>
<ul>
<li><b>adcinvert [mask]</b> Sets/gets ADC inversion mask (8 digits hex format)</li>
</ul>
<ul>
<li><b>adcdisable [mask]</b> Sets/gets ADC disable mask (8 digits hex format)</li>
</ul>
<ul>
<li><b>pattern fn</b> loads binary pattern file fn</li>
</ul>
<ul>
<li><b>patword addr [word]</b> sets/gets 64 bit word at address addr of pattern memory. Both address and word in hex format. Advanced!</li>
</ul>
<ul>
<li><b>patioctrl [word]</b> sets/gets 64 bit mask defining input (0) and output (1) signals. hex format.</li>
</ul>
<ul>
<li><b>patclkctrl [word]</b> sets/gets 64 bit mask defining if output signal is a clock and runs. hex format. Unused at the moment.</li>
</ul>
<ul>
<li><b>patlimits [addr1 addr2]</b> sets/gets the start and stop limits of the pattern to be executed. hex format. Advanced!</li>
</ul>
<ul>
<li><b>patloop0 [addr1 addr2]</b> sets/gets the start and stop limits of the level 0 loop. hex format. Advanced!</li>
</ul>
<ul>
<li><b>patnloop0 [n]</b> sets/gets the number of cyclesof the level 0 loop (int).</li>
</ul>
<ul>
<li><b>patwait0 [addr]</b> sets/gets the address of the level 0 wait point. hex format. Advanced!</li>
</ul>
<ul>
<li><b>patwaittime0 [n]</b> sets/gets the duration of the witing of the 0 waiting point in clock cycles (int).</li>
</ul>
<ul>
<li><b>patloop1 [addr1 addr2]</b> sets/gets the start and stop limits of the level 1 loop. hex format. Advanced!</li>
</ul>
<ul>
<li><b>patnloop1 [n]</b> sets/gets the number of cyclesof the level 1 loop (int).</li>
</ul>
<ul>
<li><b>patwait1 [addr]</b> sets/gets the address of the level 1 wait point. hex format. Advanced!</li>
</ul>
<ul>
<li><b>patwaittime1 [n]</b> sets/gets the duration of the witing of the 1 waiting point in clock cycles (int).</li>
</ul>
<ul>
<li><b>patloop2 [addr1 addr2]</b> sets/gets the start and stop limits of the level 2 loop. hex format. Advanced!</li>
</ul>
<ul>
<li><b>patnloop2 [n]</b> sets/gets the number of cyclesof the level 2 loop (int).</li>
</ul>
<ul>
<li><b>patwait2 [addr]</b> sets/gets the address of the level 2 wait point. hex format. Advanced!</li>
</ul>
<ul>
<li><b>patwaittime2 [n]</b> sets/gets the duration of the waiting of the 2 waiting point in clock cycles (int).</li>
</ul>
<ul>
<li><b>dut_clk [i]</b> sets/gets the signal to be used as a clock for the digital data coming from the device under test. Advanced! </li>
</ul>
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<h1><a class="anchor" id="data">Data processing commands </a></h1><p>Commands to setup the data processing (mainly MYTHEN related)</p>
<ul>
<li><b>flatfield [fn]</b> <code>put</code> sets flatfield file to <code>fn</code> (relative to <code>ffdir</code>). returns the flatfield file name relative to <code>ffdir</code> (string). If</li>
</ul>
<ul>
<li><b>ffdir [d]</b> Sets/gets the directory in which the flat field file is located. <code>Returns</code> <code></code>(string) ffdir</li>
</ul>
<ul>
<li><b>ratecorr [ns]</b> Returns the dead time used for rate correections in ns (int). <code>put</code> sets the deadtime correction constant in ns, -1 will set it to default tau of settings (0 unset). <code>Returns</code> <code></code>(double with 9 decimal digit precision)</li>
</ul>
<ul>
<li><b>badchannels [fn]</b> <code>put</code> sets the badchannels file to <code>fn</code> . returns the bad channels file name. If</li>
</ul>
<ul>
<li><b>angconv [fn]</b> <code>put</code> sets the angular conversion file to <code>fn</code> . returns the angular conversion file name. If</li>
</ul>
<ul>
<li><b>globaloff [f]</b> Sets/gets the beamline angular global offset (float).</li>
</ul>
<ul>
<li><b>fineoff [f]</b> Sets/gets the angular fine offset of the measurement (float).</li>
</ul>
<ul>
<li><b>binsize [f]</b> Sets/gets the bin size used for the angular conversion (float).</li>
</ul>
<ul>
<li><b>angdir [i]</b> Sets/gets the angular direction. 1 means increasing channels number as increasing angle, -1 increasing channel number decreasing angle.</li>
</ul>
<ul>
<li><b>moveflag [i]</b> Sets/gets the flag for physically moving the detector during the acquisition of several positions. 1 sets (moves), 0 unsets.</li>
</ul>
<ul>
<li><b>samplex [f]</b> Sets/gets the sample displacement in th direction parallel to the beam in um. Unused!</li>
</ul>
<ul>
<li><b>sampley [f]</b> Sets/gets the sample displacement in th direction orthogonal to the beam in um. Unused!</li>
</ul>
<ul>
<li><b>threaded [i]</b> Sets/gets the data processing threaded flag. 1 is threaded, 0 unthreaded.</li>
</ul>
<ul>
<li><b>darkimage fn</b> Loads the dark image to the detector from file fn (pedestal image). Cannot get.</li>
</ul>
<ul>
<li><b>gainimage fn</b> Loads the gain image to the detector from file fn (gain map for translation into number of photons of an analog detector). Cannot get. </li>
</ul>
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<h1>Introduction</h1><p>This program is intended to control the SLS detectors via command line interface. This is the only way to access all possible functionality of the detectors, however it is often recommendable to avoid changing the most advanced settings, rather leaving the task to configuration files, as when using the GUI or the API provided.</p>
<p>The command line interface consists in four main functions:</p>
<ul>
<li><b>sls_detector_acquire</b> to acquire data from the detector</li>
<li><b>sls_detector_put</b> to set detector parameters</li>
<li><b>sls_detector_get</b> to retrieve detector parameters</li>
<li><b>sls_detector_help</b> to get help concerning the text commands Additionally the program slsReceiver should be started on the machine expected to receive the data from the detector.</li>
</ul>
<p>If you need control a single detector, the use of the command line interface does not need any additional arguments.</p>
<p>For commands addressing a single controller of your detector, the command cmd should be called with the index i of the controller:</p>
<p><b>sls_detector_clnt i:cmd</b></p>
<p>where <b>sls_detector_clnt</b> is the text client (put, get, acquire, help).</p>
<p>In case more than one detector is configured on the control PC, the command cmd should be called with their respective index j:</p>
<p><b>sls_detector_clnt j-cmd</b></p>
<p>where <b>sls_detector_clnt</b> is the text client (put, get, acquire, help).</p>
<p>To address a specific controller i of detector j use:</p>
<p><b>sls_detector_clnt j-i:cmd</b></p>
<p>For additional questions concerning the indexing of the detector, please refer to the SLS Detectors FAQ documentation.</p>
<p>The commands are sudivided into different pages depending on their functionalities:</p>
<ul>
<li><a class="el" href="acquisition.html">Acquisition</a>: commands to start/stop the acquisition and retrieve data</li>
<li><a class="el" href="config.html">Configuration</a>: commands to configure the detector</li>
<li><a class="el" href="timing.html">Timing</a>: commands to configure the detector timing</li>
<li><a class="el" href="data.html">Data postprocessing</a>: commands to process the data - mainly for MYTHEN except for rate corrections.</li>
<li><a class="el" href="settings.html">Settings</a>: commands to define detector settings/threshold.</li>
<li><a class="el" href="output.html">Output</a>: commands to define output file destination and format</li>
<li><a class="el" href="actions.html">Actions</a>: commands to define scripts to be executed during the acquisition flow</li>
<li><a class="el" href="network.html">Network</a>: commands to setup the network between client, detector and receiver</li>
<li><a class="el" href="receiver.html">Receiver</a>: commands to configure the receiver</li>
<li><a class="el" href="ctb.html">Chiptest board</a>: commands specific for the new chiptest board as pattern generator</li>
<li><a class="el" href="test.html">Developer</a>: commands to be used only for software debugging. Avoid using them! </li>
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<h1><a class="anchor" id="network">Network </a></h1><p>Commands to setup the network between client, detector and receiver</p>
<ul>
<li><b>rx_hostname [s]</b> sets/gets the receiver hostname or IP address, configures detector mac with all network parameters and updates receiver with acquisition parameters. Normally used for single detectors (Can be multi-detector). <code>none</code> disables. If used, use as last network command in configuring detector MAC. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>rx_udpip [ip]</b> sets/gets the ip address of the receiver UDP interface where the data from the detector will be streamed to. Normally used for single detectors (Can be multi-detector). Used if different from eth0. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>rx_udpmac [mac]</b> sets/gets the mac address of the receiver UDP interface where the data from the detector will be streamed to. Normally used for single detectors (Can be multi-detector). <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>rx_udpport [port]</b> sets/gets the port of the receiver UDP interface where the data from the detector will be streamed to. Use single-detector command. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>rx_udpport2 [port]</b> sets/gets the second port of the receiver UDP interface where the data from the second half of the detector will be streamed to. Use single-detector command. Used for EIGER only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>detectormac [mac]</b> sets/gets the mac address of the detector UDP interface from where the detector will stream data. Use single-detector command. Normally unused. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>detectorip [ip]</b> sets/gets the ip address of the detector UDP interface from where the detector will stream data. Use single-detector command. Keep in same subnet as rx_udpip (if rx_udpip specified). <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>txndelay_left [delay]</b> sets/gets the transmission delay of first packet in an image being streamed out from the detector's left UDP port. Use single-detector command. Used for EIGER only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>txndelay_right [delay]</b> sets/gets the transmission delay of first packet in an image being streamed out from the detector's right UDP port. Use single-detector command. Used for EIGER only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>txndelay_frame [delay]</b> sets/gets the transmission frame period of entire frame being streamed out from the detector for both ports. Use single-detector command. Used for EIGER only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>flowcontrol_10g [delay]</b> Enables/disables 10 GbE flow control. 1 enables, 0 disables. Used for EIGER only. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>zmqport [port]</b> sets/gets the 0MQ (TCP) port of the receiver from where data is streamed to the client. Use single-detector command to set individually or multi-detector command to calculate based on <code>port</code> for the rest. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>configuremac [i]</b> configures the MAC of the detector with these parameters: detectorip, detectormac, rx_udpip, rx_udpmac, rx_udpport, rx_udpport2 (if applicable). This command is already included in <code>rx_hsotname</code>. Only put!. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>rx_tcpport [port]</b> sets/gets the port of the client-receiver TCP interface. Use single-detector command. Is different for each detector if same <code>rx_hostname</code> used. Must be first command to communicate with receiver. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>port [port]</b> sets/gets the port of the client-detector control server TCP interface. Use single-detector command. Default value is 1952 for all detectors. Normally not changed. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>stopport [port]</b> sets/gets the port of the client-detector stop server TCP interface. Use single-detector command. Default value is 1953 for all detectors. Normally not changed. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>lock [i]</b> Locks/Unlocks the detector to communicate with this client. 1 locks, 0 unlocks. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>lastclient </b> Gets the last client communicating with the detector. Cannot put!. <code>Returns</code> <code></code>(string) </li>
</ul>
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<h1><a class="anchor" id="output">Output settings </a></h1><p>Commands to setup the file destination and format</p>
<ul>
<li><b>outdir [dir]</b> Sets/gets the file output directory. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>fname [fn]</b> Sets/gets the root of the output file name <code>Returns</code> <code></code>(string)</li>
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<ul>
<li><b>index [i]</b> Sets/gets the current file index. <code>Returns</code> <code></code>(int)</li>
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<li><b>enablefwrite [i]</b> Enables/disables file writing. 1 enables, 0 disables. <code>Returns</code> <code></code>(int)</li>
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<li><b>overwrite [i]</b> enables(1) /disables(0) file overwriting. <code>Returns</code> <code></code>(int)</li>
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<ul>
<li><b>currentfname</b> gets the filename for the data without index and extension. MYTHEN only. <code>Returns</code> <code></code>(string)</li>
</ul>
<ul>
<li><b>fileformat</b> sets/gets the file format for data in receiver. Options: [ascii, binary, hdf5]. Ascii is not implemented in Receiver. <code>Returns</code> <code></code>(string) </li>
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<h1>Related Pages</h1>Here is a list of all related documentation pages:<ul>
<li><a class="el" href="test.html">Developer</a>
</li>
<li><a class="el" href="acquisition.html">Acquition commands</a>
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<h1><a class="anchor" id="receiver">Receiver commands </a></h1><p>Commands to configure the receiver. Not used in MYTHEN.</p>
<ul>
<li><b>receiver [s]</b> starts/stops the receiver to listen to detector packets. Options: [ <code>start</code>, <code>stop</code>]. <code>Returns</code> <code></code>(string) status of receiver[ <code>idle</code>, <code>running</code>].</li>
</ul>
<ul>
<li><b>r_online [i]</b> sets/gets the receiver in online/offline mode. 1 is online, 0 is offline. Get is from shared memory. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>r_checkonline</b> Checks the receiver if it is online/offline mode. Only get! <code>Returns</code> (string) "All online" or "[list of offline hostnames] : Not online".</li>
</ul>
<ul>
<li><b>framescaught</b> gets the number of frames caught by receiver. Average of all for multi-detector command. Only get! <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>resetframescaught [i]</b> resets the number of frames caught to 0. i can be any number. Use this if using status start, instead of acquire (this command is included). Only put! <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>frameindex [i]</b> gets the current frame index of receiver. Average of all for multi-detector command. Only get! <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>r_lock [i]</b> locks/unlocks the receiver to communicate with only this client. 1 locks, 0 unlocks. <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>r_lastclient</b> gets the last client communicating with the receiver. Only get! <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>r_readfreq [i]</b> sets/gets the stream frequency of data from receiver to client. i &gt; 0 is the nth frame being streamed. 0 sets frequency to a default timer (200ms). <code>Returns</code> <code></code>(int)</li>
</ul>
<ul>
<li><b>rx_fifodepth [i]</b> sets/gets receiver fifo (between Listener and Writer Threads) depth to i number of frames. Can improve listener packet loss (loss due to packet processing time in Listener threads), not if limited by writing. <code>Returns</code> <code></code>(int) </li>
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<html><head><title></title>
<meta http-equiv="Content-Type" content="text/xhtml;charset=UTF-8"/>
<link rel="stylesheet" type="text/css" href="search.css"/>
<script type="text/javascript" src="search.js"></script>
</head>
<body class="SRPage">
<div id="SRIndex">
<div class="SRStatus" id="NoMatches">No Matches</div>
</div>
</body>
</html>

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