Changeset 571 in ETALON

Timestamp:

Apr 28, 2016, 11:45:47 AM (8 years ago)

Author:

malovyts

Message:

Edited the poster

Location:

papers/2016_IPAC/2016_IPAC_ModelComparison_Poster

Files:

• 2016_IPAC_ModelComparisonPoster.log (modified) (7 diffs)
• 2016_IPAC_ModelComparisonPoster.pdf (modified) (previous)
• 2016_IPAC_ModelComparisonPoster.synctex.gz (modified) (previous)
• 2016_IPAC_ModelComparisonPoster.tex (modified) (11 diffs)
• figures/Polar_SPESO_SEY.png (added)
• figures/WavelengthGrat.png (modified) (previous)

papers/2016_IPAC/2016_IPAC_ModelComparison_Poster/2016_IPAC_ModelComparisonPoster.log

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papers/2016_IPAC/2016_IPAC_ModelComparison_Poster/2016_IPAC_ModelComparisonPoster.tex

@@ -109 +109 @@
 {
 \begin{center}
+        \footnotesize
         Smith-Purcell radiation is a phenomenon observed, when a charged particle moves near a periodical grating\\[2pt]
         \fbox{\includegraphics[width=0.9\linewidth]{WavelengthGrat}}\\
@@ -116 +117 @@
 }
 
-\headerbox{Parameters}{name=parameters,column=0,row=0,below=introduction}
+\headerbox{Smith-Purcell SEY}{name=polar,column=0,row=0,below=introduction}
+{
+        {\scriptsize Prediction of the Smith-Purcell Radiation single electron yield for the SPESO parameters}
+        \begin{center}
+                \fbox{\includegraphics[width=0.9\linewidth]{Polar_SPESO_SEY.png}}\\
+        \end{center}    
+}
+
+\headerbox{Parameters}{name=parameters,column=0,row=0,below=polar}
 {
 \begin{center}
@@ -143 +152 @@
 
 }
-\headerbox{References}{name=reference,column=0,row=0,below=parameters}
-{
-        \footnotesize
-        {[}1{]} D.~V.~Karlovets and A.~P.~Potylitsyn.,
-        \emph{Phys. Rev. ST Accel. Beams}, vol. 9,
-        p. 080701, 2006. \\
-        {[}2{]} J.~H.~Brownell, J.~Walsh, G.~Doucas,
-        \emph{Phys. Rev. E} vol.~57,
-        pp.~1075--1080, 1998.\\
-        {[}3{]} D.~V.~Karlovets and A.~P.~Potylitsyn.,
-        \emph{JETP Letters}, vol. 84, no. 9,
-        pp. 489-–493, 2006. \\
-}
+
 %\headerbox{Contacts}{name=contacts,column=0,row=0,below=parameters}
 %{
@@ -165 +162 @@
 %----------------------------------------------------------------------------------------
 
-\headerbox{Models}{name=results1,column=1,span=2,row=0}
-{
-\scriptsize
-        The models, that were used:
-         \textbf{R}esonance \textbf{D}iffraction \textbf{R}adiation (\textbf{\footnotesize RDR})~[1],
-         \textbf{S}urface \textbf{C}urrent (\textbf{\footnotesize SC, GFW})[1,2],
-         \textbf{R}esonance \textbf{R}eflection \textbf{R}adiation (\textbf{\footnotesize RRR}) [3].\\
-         By SC  we mean the Surface current model, with the assumption, that the width of the grating is infinite, whether the GFW model takes it into account.
-\normalsize
-%\larger
-%Surface Current (SC,GFW)\\
-%\normalsize
-%\begin{tabular}{l  m{7cm}|}
-%       \begin{minipage}{5cm}
-%               \fbox{\includegraphics[width=1\linewidth]{SC_model.png}}
-%       \end{minipage}
-%        & {adasd}\\
-%\end{tabular}
-%\\[0.3cm]
-%\larger
-%Resonance Diffraction Radiation (RDR)\\
-%\normalsize
-%\begin{tabular}{l  m{7cm}|}
-%       \begin{minipage}{5cm}
-%               \fbox{\includegraphics[width=1\linewidth]{RDR_model.png}}
-%       \end{minipage}
-%       & {adasd}\\
-%\end{tabular}
-%\\[0.3cm]
-%\larger
-%Resonant Refraction Radiation (RRR)    \\
-%\normalsize
-%\begin{tabular}{l  m{7cm}|}
-%       \begin{minipage}{5cm}
-%               \fbox{\includegraphics[width=1\linewidth]{RRR_model.png}}
-%       \end{minipage}
-%       & {adasd}\\
-%\end{tabular}
-%\\
-}
+
 %\headerbox{Pre-wave zone effect}{name=results2,column=1,span=2,below=results1}
 %{
@@ -220 +178 @@
 %       \end{center}
 %}
-\headerbox{Width dependance}{name=results3,column=1,span=2,below=results1}
+\headerbox{Width dependance}{name=results3,column=1,span=2}
 {
 \scriptsize
-With the increase of the grating width, the RRR model tends to be like the SC and RDR models.\\
+With the increase of the grating width, the RRR model tends to have same distribution as the SC and RDR models. 
 The parameters are from the SPESO experiment.
 \normalsize
 \begin{center}
-                \begin{minipage}{0.3\linewidth}
+                \begin{minipage}{0.32\linewidth}
                 \centering
                 \fbox
@@ -234 +192 @@
                 \end{minipage}
 %               \caption{SPESO parameters, M=20mm}
-                \begin{minipage}{0.3\linewidth}
+                \begin{minipage}{0.32\linewidth}
                 \centering
                 \fbox
@@ -241 +199 @@
                 \end{minipage}
 %               \caption{SPESO parameters, M=200mm}
-                \begin{minipage}{0.3\linewidth}
+                \begin{minipage}{0.32\linewidth}
                 \centering
                 \fbox
@@ -257 +215 @@
         \normalsize
         \begin{center}
-                \begin{minipage}{0.3\linewidth}
+                \begin{minipage}{0.32\linewidth}
                 \centering
                 \fbox
@@ -264 +222 @@
                 \end{minipage}  
 %               \caption{E203 parameters, d=50$\mu m$, $\theta=40\deg$}
-                \begin{minipage}{0.3\linewidth}
+                \begin{minipage}{0.32\linewidth}
                 \centering
                 \fbox
@@ -271 +229 @@
                 \end{minipage}  
 %               \caption{E203 parameters, d=50$\mu m$, $\theta=40\deg$}
-                \begin{minipage}{0.3\linewidth}
+                \begin{minipage}{0.32\linewidth}
                 \centering
                 \fbox
@@ -284 +242 @@
 {
         \begin{center}
-                \fbox
-                {\includegraphics[width=0.48\linewidth]{MOPMB004f2}}
-%               \caption{SPESO parameters}
-                \fbox
-                {\includegraphics[width=0.48\linewidth]{MOPMB004f3}}
-%               \caption{E203 parameters}
+                \begin{minipage}{0.48\linewidth}
+                \centering
+                \fbox
+                {\includegraphics[width=\linewidth]{MOPMB004f2}}
+                {\footnotesize SPESO experiment parameters, d=10mm}
+                \end{minipage}  
+                \begin{minipage}{0.48\linewidth}
+                \centering
+                \fbox
+                {\includegraphics[width=\linewidth]{MOPMB004f3}}
+                {\footnotesize E203 experiment parameters, d=0.25~mm}
+                \end{minipage}  
         \end{center}
-}
-
-%\headerbox{Angle dependance}{name=results6,column=1,span=2,below=results5}
-%{
-%       \begin{center}
-%               \fbox
-%               {\includegraphics[width=0.3\linewidth]{d005_th40_M120.png}}
-%               \fbox
-%               {\includegraphics[width=0.3\linewidth]{d005_th90_M120.png}}
-%               \fbox
-%               {\includegraphics[width=0.3\linewidth]{d005_th140_M120.png}}
-%       \end{center}    
-%}
+        \footnotesize \textbf{Conclusions:} The simulation shows that the SC and RDR models are in agreement within experimental errors. The RRR model is also close to the RDR and SC, but more detailed explanation on the constant is required. More detailed consideration of the grating profile in the GFW simulation gives the intensity 10 times bigger.
+        The ratios between the models are not changing much with the parameters~(except the observation angle), which means that it is possible to introduce a parameter-independent model correction factor.
+}
+
+\headerbox{References}{name=reference,column=1,row=0,below=results5}
+{
+        \footnotesize
+        {[}1{]} D.~V.~Karlovets and A.~P.~Potylitsyn.,
+        \emph{Phys. Rev. ST Accel. Beams}, vol. 9,
+        p. 080701, 2006. \\
+        {[}2{]} J.~H.~Brownell, J.~Walsh, G.~Doucas,
+        \emph{Phys. Rev. E} vol.~57,
+        pp.~1075--1080, 1998.\\
+        {[}3{]} D.~V.~Karlovets and A.~P.~Potylitsyn.,
+        \emph{JETP Letters}, vol. 84, no. 9,
+        pp. 489-–493, 2006. \\
+}
+\headerbox{Models}{name=results1,column=2,span=1,row=0, below=results5}
+{
+        \scriptsize
+        The models, that were used:
+        \textbf{R}esonance \textbf{D}iffraction \textbf{R}adiation (\textbf{\footnotesize RDR})~[1],
+        \textbf{S}urface \textbf{C}urrent (\textbf{\footnotesize SC, GFW})[1,2],
+        \textbf{R}esonance \textbf{R}eflection \textbf{R}adiation (\textbf{\footnotesize RRR}) [3].\\
+        By SC  we mean the Surface current model, with the assumption, that the width of the grating is infinite, whether the GFW model takes it into account.
+        \normalsize
+}
 \end{poster}
-
 \end{document}