From 10aa52bd526aee135059d2e5391172c037d603b4 Mon Sep 17 00:00:00 2001 From: Eric Teunis de Boone Date: Mon, 5 Sep 2022 18:21:13 +0200 Subject: [PATCH] fixup: b528735 --- documents/thesis/chapters/beacon_discipline.tex | 2 +- documents/thesis/chapters/introduction.tex | 2 +- 2 files changed, 2 insertions(+), 2 deletions(-) diff --git a/documents/thesis/chapters/beacon_discipline.tex b/documents/thesis/chapters/beacon_discipline.tex index 92689b1..15a2a41 100644 --- a/documents/thesis/chapters/beacon_discipline.tex +++ b/documents/thesis/chapters/beacon_discipline.tex @@ -232,7 +232,7 @@ In a static setup, these distance should be measured to such a degree to have a \bigskip If measuring the distances to the required accuracy is not possible, a different method must be found to obtain the correct number of periods. -The total time delay in \eqref{eq:phaes_diff_to_time_diff} contains a continuous term $\Delta t_\phase$ that can be determined from the beacon signal, and a discrete term $k T$ where $k$ is the unknown discrete quantity. +The total time delay in \eqref{eq:phase_diff_to_time_diff} contains a continuous term $\Delta t_\phase$ that can be determined from the beacon signal, and a discrete term $k T$ where $k$ is the unknown discrete quantity. \\ Since $k$ is discrete, the best time delay might be determined from the calibration signal by using a coherent sum diff --git a/documents/thesis/chapters/introduction.tex b/documents/thesis/chapters/introduction.tex index 78c83d1..570b521 100644 --- a/documents/thesis/chapters/introduction.tex +++ b/documents/thesis/chapters/introduction.tex @@ -12,7 +12,7 @@ \section{Cosmic Rays} -\label{sec:airshowers} +\label{sec:crs} \subsection{Airshowers} \label{sec:airshowers}