mirror of
https://gitlab.science.ru.nl/mthesis-edeboone/m.internship-documentation.git
synced 2024-11-22 23:13:35 +01:00
54 lines
1.1 KiB
TeX
54 lines
1.1 KiB
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}
|
|
Standalone devices,
|
|
\gls*{PA},
|
|
\gls*{GRAND}
|
|
|
|
\subsubsection{Time Synchronisation}
|
|
\label{sec:timesynchro}
|
|
The main method of synchronising multiple stations is by employing a \gls{GNSS}.
|
|
This system should deliver timing with an accuracy in the order of $50\ns$ (see Section~\ref{sec:grand:gnss}).
|
|
\\
|
|
|
|
Need reference system with better accuracy to constrain (Figure~\ref{fig:reference-clock}).
|
|
|
|
\begin{figure}
|
|
\centering
|
|
\includegraphics[width=\textwidth]{clocks/reference-clock.pdf}
|
|
\caption{
|
|
Using a reference clock to compare two other clocks.
|
|
}
|
|
\label{fig:reference-clock}
|
|
\todo{
|
|
redo figure with less margins,
|
|
remove spines,
|
|
rotate labels
|
|
}
|
|
\end{figure}
|
|
|
|
|
|
\subsection{Interferometry}
|
|
\label{sec:interferometry}
|
|
Requires $\sigma_t \lesssim 1\ns$
|
|
|
|
|
|
\end{document}
|