Changeset 569 in ETALON

Timestamp:

Apr 27, 2016, 7:37:33 PM (8 years ago)

Author:

hodnevuc

Message:

 

Location:

papers/2016_IPAC/IPAC16_CLIO/poster

Files:

• conference_poster_3.log (modified) (8 diffs)
• conference_poster_3.pdf (modified) (previous)
• conference_poster_3.synctex.gz (modified) (previous)
• conference_poster_3.tex (modified) (4 diffs)

papers/2016_IPAC/IPAC16_CLIO/poster/conference_poster_3.log

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papers/2016_IPAC/IPAC16_CLIO/poster/conference_poster_3.tex

@@ -30 +30 @@
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 \begin{document}
@@ -73 +60 @@
 boxshade=plain,
 headerheight=0.17\textheight,
-%postertitlecolor=titlecolor
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 }
 {}
@@ -109 +96 @@
 
 \headerbox{Intro}{name=introduction,column=0,row=0}{
-CLIO is a Free Electron Laser based on a thermoionic electron gun.This accelerator can produce single electron bunches  with length of about 8~$\pm1$~ps~[1]  and energy up to 50~MeV. Experimental comparison of Coherent Smith-Purcell Radiation (CSPR)  and Coherent Transition Radiation (CTR) will take place at CLIO accelerator~[2].  To predict the spectrums of CTR and CSPR and optimise the CLIO parameters for the experiment, we have performed simulations of  of the accelerator using ASTRA~[3]. 
+CLIO is a Free Electron Laser based on a thermoionic electron gun. Experimental comparison of Coherent Smith-Purcell Radiation (CSPR)  and Coherent Transition Radiation (CTR) will take place at CLIO accelerator. To measure and optimize the bunch length at CLIO we plan to use install a bunch length monitor at the exit of the AC at CLIO.
 }
 
-\headerbox{Reference}{name=reference,column=0,row=0,below=introduction}{
-\begin{flushleft}
-\begin{itemize}
-\item{1}
-  F. Glotin a. o.
-  \emph{Bunch length measurments on CLIO}, NI\&MPResearch A 341 (1994) 49-53
-  
-\item{2}
- J.C.Bourdon a. o. 
-  \emph{CLIO: Free Electron Laser in ORSAY} Epac 88, Rome, Italy. World Scientific, pp.314-316, 1989
-  
-\item{3}
-  Klaus Floettmann,
-  \emph{A Space Charge Tracking Algorithm Version 3.0}, DESY, Germany, October 2011(Update April 2014)
- 
- \item{4}
-  R. Chaput a. o.
-  \emph{Optimisation of the FEL CLIO Linear Accelerator}
-   
-\item{5}
-  S. J. Smith and E. M. Purcell,   Phys. Rev. 92, 1069 ~1953!.
-   
-\item{6}
-J. H. Brownell, J. Walsh, G. Doucas
-  \emph{Spontaneous Smith-Purcell radiation described through induced surface currents},  Physical review E volume 57, number 1 January 1998
-  
-\item{7}
-  S. Casalbuoni a. o.
-  \emph{ Ultrabroadband terahertz source and beamline based on coherent transition radiation}, Phys. rev. AB, 030705 (2009)
-\end{itemize}
-\end{flushleft}
+\headerbox{CTR}{name=ctr,column=0,row=0,below=introduction}{
+\begin{center}
+\includegraphics[width=\linewidth]{../MOPMB005f8.pdf}\\
+\smaller \textit{CTR spectrums of the different bunch profiles from CLIO simulation}
+\end{center}
+Unlike the case of CSPR, CTR will only be used to estimate the bunch length and no detailed profile reconstruction will be attempted. %The discrimination between pulse length will therefore be based primarily on CTR intensity but to enhance this phenomena we will also use band-pass filters in THz wavelength. %
 }
 
@@ -153 +115 @@
 
 \headerbox{The CLIO accelerator}{name=results1,span=2,column=1,row=0}{ % To reduce this block to 1 column width, remove 'span=2'
-The CLIO free electron laser is an accelerator built in 1992. It is described in details in~[1] and it is shown on figure bellow. The CLIO accelerator consist of a thermionic gun, a subharmonic buncher (SHB), a fundamental buncher (FB) and an accelerating cavity (AC). The gun produce bunches about 1.5 ns long at an energy of 90 keV. These bunch are then compressed by the subharmonic buncher  to 200 ps or less  to make it suitable for further compression with the fundamental buncher. This fundamental buncher further compresses the beam to a few ps and accelerates bunch to several MeV, making the electrons relativistic. The bunches are then further accelerated in the accelerating cavity to the operation energy  (typically 15-50 MeV). \par
-
+  To predict the spectrums of CTR and CSPR and optimise the CLIO parameters for the experiment, we have performed simulations of  of the accelerator using ASTRA.%We simulate:
+ % \begin{itemize}
+ % \item thermionic gun $\rightarrow$ 1.5ns long bunch with 90keV energy
+  %\item subharmonic buncher (SHB) $\rightarrow$ compression to 200 ps
+ % \item fundamental buncher (FB) $\rightarrow$ further compression with acceleration
+ % \item accelerating cavity (AC) $\rightarrow$ acceleration (typically 15-50 MeV)
+ % \item solenoids $\rightarrow$ keep particles on orbit
+ % \end{itemize}
 \begin{center}
-    \includegraphics*[width=0.7\textwidth]{../MOPMB005f1.png}\\
-\smaller \textit{Layout of the CLIO accelerator (taken from [4]).}
+    \includegraphics*[width=1\textwidth]{../MOPMB005f1.png}\\
+\smaller \textit{Layout of the CLIO accelerator (taken from).}
 \end{center}
 
 \begin{center}
-  \includegraphics[width=0.45\linewidth]{../MOPMB005f3.pdf}
-    \includegraphics[width=0.45\linewidth]{../MOPMB005f4.pdf}
-  
+  \includegraphics[width=0.47\linewidth]{../MOPMB005f3.pdf}
+    \includegraphics[width=0.45\linewidth]{../MOPMB005f4.pdf}\\  
  \smaller \textit{Longitudinal bunch size at exit of gun (FWHM=800 ps), at the entrance of FB (FWHM=92 ps), at the entrance (FWHM=2.35ps) and at the exit (FWHM=2.29ps) of the AC at left figure and profile of the bunch at the exit of the acceleration cavity for different maximum fields of fundamental buncher (optimized) at right figure. }
   \end{center}
 }
 
-\headerbox{Bunch length measurements}{name=results2,span=2,column=1,below=results1}{ % To reduce this block to 1 column width, remove 'span=2'
-To measure and optimize the bunch length at CLIO we plan to use install a bunch length monitor at the exit of the AC at CLIO. This bunch length monitor will use two different radiative phenomenon:  Coherent Smith-Purcell Radiation (CSPR)~[5,6] and Coherent Transition Radiation (CTR)~[7]. 
+\headerbox{Bunch length measurements (CSPR)}{name=results2,span=3,column=0,below=ctr}{ % To reduce this block to 1 column width, remove 'span=2'
+ %The bunch length monitor will use two different radiative phenomenon:  Coherent Smith-Purcell Radiation (CSPR)~and Coherent Transition Radiation (CTR)~. 
+ Energy distribution of Coherent Smith-Purcell spectrum as a function of the observation angle for different maximum field in the FB at left. The grating used for these simulations is $40 mm\times180 mm$ with a pitch of $8mm$ and a blaze angle of $30^o$.
 \begin{center}
-\includegraphics[width=0.45\linewidth]{../MOPMB005f6.pdf}
-\includegraphics[width=0.45\linewidth]{../MOPMB005f8.pdf}\\
-\smaller \textit{Energy distribution of Coherent Smith-Purcell spectrum as a function of the observation angle for different maximum field in the FB at left. The grating used for these simulations has a pitch of 8~mm and a blaze angle of $30^o$. And on right CTR spectrums the different bunches profiles shown on figure up.}
+\includegraphics[width=0.40\linewidth]{../MOPMB005f6.pdf}
+\includegraphics[width=0.40\linewidth]{../MOPMB005f7.pdf}\\
+\smaller \textit{ CSPR spectrums with original (left) and normalized (right) amplitude}
 \end{center}
 
-Unlike the case of CSPR, CTR will only be used to estimate the bunch length and no detailed profile reconstruction will be attempted.%
+
 }