Changeset 552 in ETALON for papers/2016_IPAC/IPAC16_SP_CTR/MOPMB003.tex
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papers/2016_IPAC/IPAC16_SP_CTR/MOPMB003.tex
r551 r552 33 33 \title{Comparison of Coherent Smith-Purcell radiation and Coherent Transition Radiation\thanks{The authors are grateful for the funding received from the French ANR (contract ANR-12-JS05-0003-01) and the IDEATE International Associated Laboratory (LIA) between France and Ukraine.}} 34 34 35 \author{Vitalii Khodnevych~\thanks{hodnevuc@lal.in2p3.fr} (LAL, Orsay; Taras Shevchenko National University of Kyiv, Kyiv),\\ Nicolas Delerue~\thanks{delerue@lal.in2p3.fr} (LAL, Orsay), Oleg Bezshyyko ( Taras Shevchenko National University of Kyiv, Kyiv) } 35 \author{Vitalii Khodnevych\textsuperscript{1}\thanks{hodnevuc@lal.in2p3.fr}, Nicolas Delerue~\thanks{delerue@lal.in2p3.fr} 36 \\(LAL, Orsay), 37 \\ Oleg Bezshyyko 38 \\ ( Taras Shevchenko National University of Kyiv, Kyiv) 39 \\ \textsuperscript{1}also at National Taras Shevchenko University of Kyiv, Kyiv, Ukraine 40 } 41 42 43 44 36 45 \maketitle 37 46 … … 84 93 \begin{figure}[htb] 85 94 \centering 86 \includegraphics[width=0.9\linewidth]{plots/SEY 2.eps}87 \caption{Single electron yield for TR and SP. The screen diameter for TR is 40mm. SP SEY is presented for different beam-grating separation (3,6,9 mm). The grating used here is $40\mbox{mm}\times180\mbox{mm}$with 8 mm pitch and $30^o$ blaze angle. }95 \includegraphics[width=0.9\linewidth]{plots/SEY1488.eps} 96 \caption{Single electron yield for TR and SP. The screen diameter for TR is 40mm. SP SEY is presented for different beam-grating separation (3,6,9 mm). The grating used here is $40\times180$ \si{mm^2}with 8 mm pitch and $30^o$ blaze angle. } 88 97 \label{sey} 89 98 \end{figure} … … 93 102 \centering 94 103 \includegraphics[width=0.9\linewidth]{plots/SP2d.eps} 95 \caption{SEY for SP effect. Grating $40mm\times180mm$with 8~mm pitch and $30^o$ blaze angle. }104 \caption{SEY for SP effect. Grating $40\times180$ \si{mm^2} with 8~mm pitch and $30^o$ blaze angle. } 96 105 \label{sey2d} 97 106 \end{figure} … … 134 143 \centering 135 144 \includegraphics[width=0.9\linewidth]{plots/MAE.eps} 136 \caption{Maximum angle of emission for SP effect as function of pulsewidth and grating pitch. Grating $40mm\times180mm$with $30^o$ blaze angle. The beam-grating separation is 3~mm.}145 \caption{Maximum angle of emission for SP effect as function of pulsewidth and grating pitch. Grating $40\times180$ \si{mm^2} with $30^o$ blaze angle. The beam-grating separation is 3~mm.} 137 146 \label{mae} 138 147 \end{figure} … … 152 161 \centering 153 162 \includegraphics[width=0.9\linewidth]{plots/TE.eps} 154 \caption{Total energy for SP effect presented as function of pulsewidth and grating pitch. Grating is $40mm\times180mm$with $30^o$ blaze angle. }163 \caption{Total energy for SP effect presented as function of pulsewidth and grating pitch. Grating is $40\times180$ \si{mm^2} with $30^o$ blaze angle. } 155 164 \label{Epp} 156 165 \end{figure} … … 197 206 \begin{figure}[!htb] 198 207 \centering 199 \includegraphics[width=0.9\linewidth]{plots/SP .eps}208 \includegraphics[width=0.9\linewidth]{plots/SP1488.eps} 200 209 \caption{CSPR and CTR energy density as function of wavelength. The CSPR spectrum is presented for beam-grating separations of \SIlist{3;6;9}{mm}. The grating dimensions are $40\times180$ \si{mm^2} with \SI{8}{mm} pitch and \ang{30} blaze angle. The screen diameter for TR is \SI{40}{mm}. The signal is measured as integrated with a \SI{50}{mm} diameter parabolic mirror located \SI{300}{mm} from the beam axis.} 201 210 \label{spctr}
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