mirror of
https://gitlab.science.ru.nl/mthesis-edeboone/m.internship-documentation.git
synced 2024-11-12 18:43:30 +01:00
43 lines
777 B
TeX
43 lines
777 B
TeX
\documentclass[../thesis.tex]{subfiles}
|
|
|
|
\graphicspath{
|
|
{.}
|
|
{../../figures/}
|
|
{../../../figures/}
|
|
}
|
|
|
|
\begin{document}
|
|
\chapter{Introduction}
|
|
\label{sec:introduction}
|
|
|
|
|
|
\section{Cosmic Rays}
|
|
\label{sec:crs}
|
|
|
|
\subsection{Airshowers}
|
|
\label{sec:airshowers}
|
|
|
|
\subsection{Detectors}
|
|
\label{sec:detectors}
|
|
Pierre Auger,
|
|
GRAND
|
|
|
|
\subsection{Interferometry}
|
|
\label{sec:interferometry}
|
|
Requires $\sigma_t \lesssim 1\ns$
|
|
|
|
|
|
\section{Time Synchronisation}
|
|
\label{sec:timesynchro}
|
|
Need reference system with better accuracy to constrain
|
|
See Section~\ref{sec:grand:gnss}.
|
|
|
|
\begin{figure}
|
|
\centering
|
|
\includegraphics[width=\textwidth]{clocks/reference-clock.pdf}
|
|
\caption{
|
|
Using a reference clock to compare two other clocks.
|
|
}
|
|
\label{fig:reference-clock}
|
|
\end{figure}
|
|
\end{document}
|