Changeset 593 in ETALON for papers

Timestamp:

May 2, 2016, 1:40:10 PM (8 years ago)

Author:

delerue

Message:

Papier acceleration laser-plasma

Location:

papers/2016_IPAC

Files:

• IPAC16_SP_CTR/poster/conference_poster_SP_TR.synctex.aux (deleted)
• IPAC16_SP_CTR/poster/conference_poster_SP_TR.synctex.log (deleted)
• MOPMB002_SPESO/MOPMB002.tex (modified) (5 diffs)
• WEPMY003_Plasma_acceleration (added)
• WEPMY003_Plasma_acceleration/PHIL.png (added)
• WEPMY003_Plasma_acceleration/PHIL_and_Laserix.png (added)
• WEPMY003_Plasma_acceleration/WEPMY003.aux (added)
• WEPMY003_Plasma_acceleration/WEPMY003.pdf (added)
• WEPMY003_Plasma_acceleration/WEPMY003.tex (added)
• WEPMY003_Plasma_acceleration/electrons_z_0cm.png (added)
• WEPMY003_Plasma_acceleration/electrons_z_3cm.png (added)
• WEPMY003_Plasma_acceleration/electrons_z_m2cm.png (added)
• WEPMY003_Plasma_acceleration/electrons_z_m35cm.png (added)
• WEPMY003_Plasma_acceleration/electrons_z_m4cm.png (added)
• WEPMY003_Plasma_acceleration/energy_distribution.png (added)
• WEPMY003_Plasma_acceleration/energy_distribution_vs_theta.png (added)
• WEPMY003_Plasma_acceleration/jacow.cls (added)
• WEPMY003_Plasma_acceleration/plasma_density.png (added)
• WEPMY003_Plasma_acceleration/scheme_Laserix_LAL.png (added)

papers/2016_IPAC/MOPMB002_SPESO/MOPMB002.tex

@@ -124 +124 @@
 On the breadboard two sets of two rotary stage allow to control the direction of the detectors. A photo of the experimental apparatus can be seen on figure~\ref{fig:SPESO_linac}.
 
-\begin{figure}[!htb]
+\begin{figure}[htbp]
 %   \vspace*{-.5\baselineskip}
    \centering
@@ -135 +135 @@
 Two different detectors are used, one is sensitive to electromagnetic waves in the Q-band (33-50~GHz - 9.1 to 6~mm) and the other one is sensitive in the Ka-band (26.5-40~GHz - 11.3 to 5~mm). These detectors are based on zero-bias Schottky diodes to produce a signal proportional to the incoming radiation. The data coming from these detectors are acquired by an oscilloscope. A typical example of data is shown on figure~\ref{fig:SPESO_data}
 
-\begin{figure}[!htb]
+\begin{figure}[htbp]
 %   \vspace*{-.5\baselineskip}
    \centering
@@ -150 +150 @@
 During normal beam operations the experiment is running autonomously: each time there is a linac trigger the data from the oscilloscope are recorded. Every 30 minutes the detectors are moved to a different location. In each 30 minutes cycle the grating is inserted for about 25~minutes and retracted for 5 minutes to allow measurement of the background. The data are then analysed by a script that runs every hours for data quality check. A more advanced analysis is done off-line to extract physical information from the data. On figure~\ref{fig:data_trend} one can see the trend of data recorded over a day while the detectors where moving along the S-direction.
 
-\begin{figure}[!htb]
+\begin{figure}[htbp]
 %   \vspace*{-.5\baselineskip}
    \centering
@@ -163 +163 @@
 
 
-\begin{figure}[!htb]
+\begin{figure}[htbp]
 %   \vspace*{-.5\baselineskip}
    \centering
@@ -173 +173 @@
 \end{figure}
 
+
+\begin{figure}[htbp]
+%   \vspace*{-.5\baselineskip}
+   \centering
+   \includegraphics[width=250pt]{Signal.eps}
+   \caption{XXX Example of data recorded during one day. During that day the detectors were moving along the linac axis. The 3 different lines correspond to 3 different regimes: grating retracted (upper line, SPM and LPM).}
+   \label{fig:data_trend}
+%   \vspace*{-\baselineskip}
+\end{figure}
+
+
+
+
 \section{Bunch profile reconstruction}
 \section{Simulations}