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Timestamp:
Apr 22, 2016, 1:04:38 PM (8 years ago)
Author:
hodnevuc
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1 edited

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  • papers/2016_IPAC/IPAC16_CLIO/MOPMB005.tex

    r516 r518  
    171171\begin{figure}[!htb]
    172172  \centering
    173   \includegraphics[width=0.9\linewidth]{plots/FF2.eps}
     173  \includegraphics[width=0.9\linewidth]{plots/FF22.eps}
    174174  \caption{Form factor for the bunch profiles shown on figure~\ref{p123}. }
    175175  \label{fig:FF}
     
    177177
    178178\begin{figure}[!htb]
    179   \includegraphics[width=0.9\linewidth]{plots/SPpolar.eps}
     179  \includegraphics[width=0.9\linewidth]{plots/SP42.eps}
    180180  \caption{Coherent Smith-Purcell spectrum as function of observation angle for different maximum field in the FB. The grating used for these simulations has a pitch of 8 mm and a blaze angle of$30^o$.  }
    181181  \label{sp}
     
    185185\begin{figure}[!htb]
    186186  \centering
    187   \includegraphics[width=0.9\linewidth]{plots/SPnorm.eps}
     187  \includegraphics[width=0.9\linewidth]{plots/SPn.eps}
    188188  \caption{  Coherent Smith-Purcell spectrum normalized by maximum as function of observation angle for different maximum field in the FB. The grating used for these simulations has a pitch of 8 mm and a blaze angle of$30^o$. }
    189189  \label{sp-normalised}
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