Changeset 550 in ETALON

Timestamp:

Apr 26, 2016, 3:16:27 PM (8 years ago)

Author:

hodnevuc

Message:

 

Location:

papers/2016_IPAC/IPAC16_SP_CTR

Files:

• MOPMB003.aux (modified) (1 diff)
• MOPMB003.log (modified) (9 diffs)
• MOPMB003.pdf (modified) (previous)
• MOPMB003.synctex.gz (modified) (previous)
• MOPMB003.tex (modified) (3 diffs)

papers/2016_IPAC/IPAC16_SP_CTR/MOPMB003.aux

@@ -31 +31 @@
 \@writefile{lof}{\contentsline {figure}{\numberline {4}{\ignorespaces Maximum angle of emission for SP effect as function of pulsewidth and grating pitch. Grating $40mm\times 180mm$ with $30^o$ blaze angle. The beam-grating separation is 3~mm.\relax }}{2}}
 \newlabel{mae}{{4}{2}}
-\@writefile{lof}{\contentsline {figure}{\numberline {5}{\ignorespaces Total energy for SP effect presented as function of pulsewidth and grating pitch. Grating is $40\times 180$mm with $30^o$ blaze angle. \relax }}{2}}
+\@writefile{lof}{\contentsline {figure}{\numberline {5}{\ignorespaces Total energy for SP effect presented as function of pulsewidth and grating pitch. Grating is $40mm\times 180mm$ with $30^o$ blaze angle. \relax }}{2}}
 \newlabel{Epp}{{5}{2}}
 \bibcite{GF}{1}

papers/2016_IPAC/IPAC16_SP_CTR/MOPMB003.log

@@ -1 @@
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 **E:/2016_IPAC/IPAC16_SP_CTR/MOPMB003.tex
@@ -1412 +1412 @@
 
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@@ -1471 +1469 @@
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+eps-converted-to.pdf>]
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papers/2016_IPAC/IPAC16_SP_CTR/MOPMB003.tex

@@ -49 +49 @@
 \label{eq:eq2}
 \end{equation}
-where $q_0$ is electron charge, c is the speed of light, $\beta$  is relativistic velocity and $\Theta$ is
+where $q_0$ is electron charge, $\epsilon_0$ -- vacuum permittivity, c is the speed of light, $\beta$  is relativistic velocity and $\Theta$ is
 the observation angle.
 
@@ -152 +152 @@
   \centering
   \includegraphics[width=0.9\linewidth]{plots/TE.eps}
-  \caption{Total energy for SP effect presented as function of pulsewidth and grating pitch. Grating is $40\times180$mm with  $30^o$ blaze angle. }
+  \caption{Total energy for SP effect presented as function of pulsewidth and grating pitch. Grating is $40mm\times180mm$ with  $30^o$ blaze angle. }
   \label{Epp}
 \end{figure}
@@ -203 +203 @@
 
 \section{Conclusion}
-We have studied both CSPR and CTR and studied how to optimize the experimental parameters. Using the CLIO parameters we expect a signal (in the range 0.3-3 THz [ 0.1 - 1 mm]) of 5.3e-7 J for CSPR and 1.86e-06 J for CTR   with 50 mm parabolic mirror at distance 300mm from grating.\par
+We have studied both CSPR and CTR and studied how to optimize the experimental parameters. Using the CLIO parameters we expect a signal (in the range 0.03-3 THz [ 0.1 - 10 mm]) of 8.37e-7 J for CSPR and 7.35e-08 J for CTR.\par