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\title[]{}
\date{March 08, 2023}
\author{E.T. de Boone}

\begin{document}
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\section{Cosmic Rays}
\begin{frame}{Particles from space}
\end{frame}
\begin{notes}
	- Ultra energy, solid idea for source missing
\end{notes}

\begin{frame}{Airshowers}
\end{frame}
\begin{notes}
	- Coming into atmosphere, trying to measure particle debris
	  through Cherenkov light.
	- FD/SD
\end{notes}

\begin{frame}{Airshowers: Radio Detection}
\end{frame}
\begin{notes}
	measurables of RD: EM
\end{notes}

\begin{frame}{Airshowers: Interferometric Radio Detection}
\end{frame}
\begin{notes}
	Can reconstruct spatial distribution
	Requires sigma < 1 ns
\end{notes}


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\section{Experimental problem}
\begin{frame}{Experiments: Autonomous antennas}
\end{frame}
\begin{notes}
	Introduce GRAND and Auger
\end{notes}

\begin{frame}{Experiments: GNSS timing}
\end{frame}
\begin{notes}
	Note timing accuracy obtained in Auger
\end{notes}


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\section{Improving time synchronisation}
\begin{frame}{Improving time synchronisation}
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\be

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\subsection{Can GNSS be improved}
% Hardware setups WR / GRAND
\begin{frame}{Improving GNSS timing}
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\subsection{Other methods to improve timing}
% mixing clock information with physics
\begin{frame}{Beacon}
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