WUotD: added first acronyms

This commit is contained in:
Eric Teunis de Boone 2022-09-05 19:21:51 +02:00
parent 10aa52bd52
commit c4e6aa3afd
3 changed files with 32 additions and 18 deletions

View file

@ -9,9 +9,8 @@
\begin{document} \begin{document}
\chapter{Disciplining by Beacon} \chapter{Disciplining by Beacon}
\label{sec:disciplining} \label{sec:disciplining}
The main method of synchronising multiple stations is by employing a GNSS. The time accuracy supplied by a \gls{GNSS} is not enough to do interferometry.
This system should deliver timing with an accuracy in the order of $50\ns$. In this chapter,
\section{Beacon} \section{Beacon}
@ -98,8 +97,8 @@ This slower timescale allows to count the ticks of the quicker signal.\todo{Exte
\begin{figure} \begin{figure}
\includegraphics[width=0.5\textwidth]{beacon/auger/1512.02216.figure2.beacon_beat.png} \includegraphics[width=0.5\textwidth]{beacon/auger/1512.02216.figure2.beacon_beat.png}
\caption{ \caption{
From Ref~\cite{PierreAuger:2015aqe} From Ref~\cite{PierreAuger:2015aqe}.
The beacon signal that the \PAObs\ employs. The beacon signal that the \acrlong*{PAObs} employs.
} }
\label{fig:beacon:pa} \label{fig:beacon:pa}
\end{figure} \end{figure}

View file

@ -19,18 +19,17 @@
\subsection{Detectors} \subsection{Detectors}
\label{sec:detectors} \label{sec:detectors}
Pierre Auger, Standalone devices,
GRAND \gls*{PA},
\gls*{GRAND}
\subsection{Interferometry} \subsubsection{Time Synchronisation}
\label{sec:interferometry}
Requires $\sigma_t \lesssim 1\ns$
\section{Time Synchronisation}
\label{sec:timesynchro} \label{sec:timesynchro}
Need reference system with better accuracy to constrain The main method of synchronising multiple stations is by employing a \gls{GNSS}.
See Section~\ref{sec:grand: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} \begin{figure}
\centering \centering
@ -39,5 +38,17 @@ See Section~\ref{sec:grand:gnss}.
Using a reference clock to compare two other clocks. Using a reference clock to compare two other clocks.
} }
\label{fig:reference-clock} \label{fig:reference-clock}
\todo{
redo figure with less margins,
remove spines,
rotate labels
}
\end{figure} \end{figure}
\subsection{Interferometry}
\label{sec:interferometry}
Requires $\sigma_t \lesssim 1\ns$
\end{document} \end{document}

View file

@ -30,6 +30,8 @@
\usepackage[english]{babel} % for proper word breaking at line ends \usepackage[english]{babel} % for proper word breaking at line ends
\usepackage[switch]{lineno} \usepackage[switch]{lineno}
\usepackage[acronym]{glossaries}
\glsdisablehyper
%\usepackage{listings} %\usepackage{listings}
\usepackage{csquotes} \usepackage{csquotes}
@ -99,6 +101,8 @@
% Names % Names
\newcommand{\PA}{Pierre~Auger} % Acronyms
\newcommand{\PAObs}{\PA\ Observatory} \newacronym{GNSS}{GNSS}{Global Navigation Satellite System}
\newcommand{\GRAND}{Giant Radio Array for Neutrino Detection} \newacronym{GRAND}{GRAND}{Giant Radio Array for Neutrino Detection}
\newacronym{PA}{PA}{Pierre~Auger}
\newacronym{PAObs}{PAO}{Pierre~Auger~Observatory}