HEP Student seminar presetnation

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Eric Teunis de Boone 2023-03-08 12:20:23 +01:00
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Figure 2: Left: Simplified sketch of an air shower and possible detection techniques. Real air showers
contain more particle types than displayed, but most detection techniques (radio, air-Cherenkov and
fluorescence light) are only sensitive to electrons and positrons. Particle detectors also measure muons,
which generally reach further out than the electromagnetic component. Right: Longitudinal shower
profile for different particle types.

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From Harm

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\usepackage{hyperref} \usepackage{hyperref}
\usepackage[backend=bibtex,style=trad-plain]{biblatex} \usepackage[backend=bibtex,style=trad-plain]{biblatex}
\usepackage{graphicx} \usepackage{graphicx}
\graphicspath{{.}{../../figures/}} \graphicspath{{.}{./figures/}{../../figures/}}
\usepackage{todo} \usepackage{todo}
\usepackage{notes}
\addbibresource{../../../bibliotheca/bibliography.bib} \addbibresource{../../../bibliotheca/bibliography.bib}
@ -26,7 +27,7 @@
\setbeamerfont{page number in head/foot}{size=\normalsize} \setbeamerfont{page number in head/foot}{size=\normalsize}
\setbeamertemplate{footline}[frame number] \setbeamertemplate{footline}[frame number]
\title[]{} \title[]{HEP Student Seminar}
\date{March 08, 2023} \date{March 08, 2023}
\author{E.T. de Boone} \author{E.T. de Boone}
@ -37,66 +38,107 @@
%%%%% %%%%%
\section{Cosmic Rays} \section{Cosmic Rays}
\begin{frame}{Particles from space} \begin{frame}{Particles from space}
\includegraphics[width=\textwidth]{grand/astroparticletypes_grand.jpg}
\end{frame} \end{frame}
\begin{notes}
- Ultra energy, solid idea for source missing
\end{notes}
\begin{frame}{Airshowers} \begin{frame}{Airshowers}
\includegraphics[width=\textwidth]{1607.08781/fig02.png}
\end{frame} \end{frame}
\begin{notes} \note[itemize]{
- Coming into atmosphere, trying to measure particle debris \item Coming into atmosphere, trying to measure particle debris
through Cherenkov light. through Cherenkov light.
- FD/SD - FD/SD
\end{notes} }
\begin{frame}{Airshowers: Radio Detection} \begin{frame}{Airshowers: (Interferometric) Radio Detection}
\begin{columns}
\begin{column}{0.5\textwidth}
\includegraphics[width=\textwidth]{radio_interferometry/Schematic_RIT_extracted.png}
\end{column}
\begin{column}{0.5\textwidth}
\includegraphics[width=\textwidth]{2006.10348/fig01.png}
\end{column}
\end{columns}
\end{frame} \end{frame}
\begin{notes} \note[itemize]{
measurables of RD: EM
\end{notes}
\begin{frame}{Airshowers: Interferometric Radio Detection}
\end{frame}
\begin{notes}
Can reconstruct spatial distribution Can reconstruct spatial distribution
Requires sigma < 1 ns Requires sigma < 1 ns
\end{notes} }
%%%%% %%%%%
%%%%% %%%%%
\section{Experimental problem} \section{Experimental problem}
\begin{frame}{Experiments: Autonomous antennas} \begin{frame}{Experiments: Autonomous antennas}
\begin{columns}
\begin{column}{0.4\textwidth}
\includegraphics[width=\textwidth]{images/auger-astro-uchicageo.edu-watertank-080224-3_large.jpg}
\end{column}
\begin{column}{0.6\textwidth}
\includegraphics[width=\textwidth]{images/Layout-of-the-Pierre-Auger-Southern-Observatory-The-dots-represent-the-position-of-each.png}
\end{column}
\end{columns}
\end{frame} \end{frame}
\begin{notes} \note{
Introduce GRAND and Auger Introduce GRAND and Auger
\end{notes} }
\begin{frame}{Experiments: GNSS timing}
\end{frame}
\begin{notes}
Note timing accuracy obtained in Auger
\end{notes}
%%%%% %%%%%
%%%%% %%%%%
\section{Improving time synchronisation} \begin{frame}{Testing GNSS in GRAND: I}
\begin{frame}{Improving time synchronisation} \begin{columns}
\end{frame} \begin{column}{0.7\textwidth}
\be \includegraphics<1>[width=\textwidth]{grand/setup/channel-delay-setup.pdf}
\includegraphics<2->[width=\textwidth]{grand/setup/channel-delay-setup-inverse.pdf}
%%%%% \end{column}
\subsection{Can GNSS be improved} \begin{column}{0.3\textwidth}
% Hardware setups WR / GRAND \includegraphics[width=\textwidth]{grand/setup/antenna-to-adc.pdf}
\begin{frame}{Improving GNSS timing} \end{column}
\end{columns}
\end{frame} \end{frame}
%%%%% \begin{frame}{Filterchain delay}
\subsection{Other methods to improve timing} \includegraphics[width=\textwidth]{grand/split-cable/split-cable-delay-ch1ch2-50mhz-200mVpp.pdf}
% mixing clock information with physics \end{frame}
\begin{frame}{Beacon}
%%%%%%
\begin{frame}{Testing GNSS in GRAND: II}
\centering
\includegraphics[width=0.7\textwidth]{grand/setup/grand-gps-setup.pdf}
\end{frame}
\begin{frame}
\includegraphics[width=\textwidth]{images/IMG_20220712_164912.jpg}
\end{frame}
%%%%
\begin{frame}
\includegraphics[width=\textwidth]{images/IMG_20220812_114028.jpg}
\end{frame}
\begin{frame}
\includegraphics[width=\textwidth]{images/IMG_20220811_185348.jpg}
\end{frame}
\begin{frame}
\includegraphics[width=\textwidth]{images/IMG_20220811_220552.jpg}
\end{frame}
\begin{frame}
\includegraphics[width=\textwidth]{images/IMG_20220811_220539.jpg}
\end{frame}
%%% Real
\begin{frame}
\includegraphics[width=\textwidth]{images/IMG_20220819_154801.jpg}
\end{frame}
\begin{frame}
\includegraphics[width=\textwidth]{images/IMG_20220819_152900.jpg}
\end{frame}
\begin{frame}
\includegraphics[width=\textwidth]{images/IMG_20220815_161244.jpg}
\end{frame} \end{frame}
\end{document} \end{document}