mirror of
https://gitlab.science.ru.nl/mthesis-edeboone/m.internship-documentation.git
synced 2024-11-12 18:43:30 +01:00
Third round feedback, requires work on slide 7
This commit is contained in:
parent
8a5de083fe
commit
1c61564174
7 changed files with 151 additions and 49 deletions
BIN
figures/2006.10348/fig01_a.png
Normal file
BIN
figures/2006.10348/fig01_a.png
Normal file
Binary file not shown.
After Width: | Height: | Size: 77 KiB |
BIN
figures/grand/GRAND-detection-principle-1.png
Normal file
BIN
figures/grand/GRAND-detection-principle-1.png
Normal file
Binary file not shown.
After Width: | Height: | Size: 548 KiB |
Binary file not shown.
Binary file not shown.
Binary file not shown.
Binary file not shown.
|
@ -1,5 +1,9 @@
|
|||
\documentclass[showdate=false]{beamer}
|
||||
|
||||
|
||||
%%%%%%%%
|
||||
% Goal: show enthousiasm, knowledge and drive about the field
|
||||
|
||||
\usepackage[british]{babel}
|
||||
\usepackage{amsmath}
|
||||
\usepackage{hyperref}
|
||||
|
@ -19,41 +23,60 @@
|
|||
\setbeamerfont{page number in head/foot}{size=\normalsize}
|
||||
\setbeamertemplate{footline}[frame number]
|
||||
|
||||
\hypersetup{pdfpagemode=UseNone} % don't show bookmarks on initial view
|
||||
|
||||
|
||||
\title[]{Early contest STEP-UP}
|
||||
\date{March $13^{\text{\tiny{th}}}$, 2023}
|
||||
\author{E.T. de Boone}
|
||||
|
||||
\begin{document}
|
||||
\frame{\titlepage}
|
||||
{
|
||||
\setbeamertemplate{footline}{} % no page number here
|
||||
\frame{ \titlepage }
|
||||
}
|
||||
|
||||
\begin{frame}{About me}
|
||||
Studies (at Radboud University, Nijmegen):
|
||||
\begin{itemize}
|
||||
\item Bachelor from 2012 to 2020 \\
|
||||
\quad Minor: Astrophysics
|
||||
|
||||
\item Master from 2020 to 2023 (expected) \\
|
||||
\quad Specialisation: Particle and Astrophysics \\
|
||||
\quad Minor: Computational Data Science
|
||||
|
||||
\item Master's Internship (ongoing) \\
|
||||
\hfill ``Enhancing Timing Accuracy in Air Shower Radio Detectors''
|
||||
\end{itemize}
|
||||
|
||||
\vspace*{2em}
|
||||
|
||||
Interests:
|
||||
\begin{itemize}
|
||||
\item Hardware experimenting
|
||||
\item Ultra High Energy particles
|
||||
\item Radio detection
|
||||
\end{itemize}
|
||||
\end{frame}
|
||||
|
||||
% Context
|
||||
%%%%%%%%%
|
||||
\begin{frame}{Airshowers from Ultra High Energy particles}
|
||||
academic curriculum?
|
||||
|
||||
\begin{frame}{Ultra High Energy particles}
|
||||
\begin{figure}
|
||||
\includegraphics[width=\textwidth]{grand/astroparticletypes_grand.jpg}
|
||||
% \caption{
|
||||
% From: \cite{GRAND:2018ia}
|
||||
% }
|
||||
\end{figure}
|
||||
\end{frame}
|
||||
|
||||
\begin{frame}{Radio signals and Airshowers}
|
||||
\begin{columns}
|
||||
\begin{column}{0.4\textwidth}
|
||||
Airshower split into EM, Muon and Hadron
|
||||
\end{column}
|
||||
\begin{column}{0.5\textwidth}
|
||||
\begin{figure}
|
||||
\centering
|
||||
\includegraphics[width=\textwidth]{1607.08781/fig02a_airshower+detectors.png}
|
||||
% \caption{
|
||||
% \cite{Schroder:2016hrv}
|
||||
% }
|
||||
\end{figure}
|
||||
\end{column}
|
||||
\end{columns}
|
||||
\begin{figure}
|
||||
\centering
|
||||
\includegraphics<2>[width=\textwidth]{airshower/airshower_radio_polarisation.jpg}%
|
||||
\includegraphics[width=\textwidth]{grand/GRAND-detection-principle-1.png}
|
||||
% \caption{
|
||||
% From: \cite{GRAND:2018ia}
|
||||
% }
|
||||
\end{figure}
|
||||
\end{frame}
|
||||
|
||||
|
@ -96,16 +119,17 @@
|
|||
Required time accuracy $< 1 \mathrm{ns}$ not provided by GNSS $ \gtrsim 5 \mathrm{ns}$.
|
||||
\vspace{ 2em }
|
||||
\begin{columns}
|
||||
\begin{column}{0.4\textwidth}
|
||||
Additional synchronisation
|
||||
using physics band
|
||||
\begin{column}{0.5\textwidth}
|
||||
\visible<2->{Additional synchronisation\\
|
||||
using physics band
|
||||
}
|
||||
\begin{itemize}
|
||||
\item Pulsed beacon
|
||||
\item Long period ($\sim 1 \mathrm{\mu s}$)% (AERA)
|
||||
\item<2-> Pulsed beacon
|
||||
\item<2-> Long period ($\sim 1 \mathrm{\mu s}$)% (AERA)
|
||||
\item<3-> Short period ($\lesssim 20 \mathrm{ns}$)
|
||||
\end{itemize}
|
||||
\end{column}
|
||||
\begin{column}{0.6\textwidth}
|
||||
\begin{column}{0.5\textwidth}
|
||||
\begin{figure}% Clock error fixes
|
||||
\includegraphics<1>[width=\textwidth]{radio_interferometry/trace_overlap/dc_grid_power_time_fixes.py.scale4d.best.trace_overlap.zoomed.repair_none.png}%
|
||||
\includegraphics<2>[width=\textwidth]{radio_interferometry/trace_overlap/dc_grid_power_time_fixes.py.scale4d.best.trace_overlap.zoomed.no_offset.png}%
|
||||
|
@ -116,46 +140,86 @@
|
|||
\end{columns}
|
||||
\end{frame}
|
||||
|
||||
\begin{frame}{Enhancing Timing Accuracy in Air Shower Radio Detectors}
|
||||
TODO: Relate GNSS stability to beacon synchronisation mechanisms\\
|
||||
|
||||
In-band mechanism affect physics data \\
|
||||
How often should we `resynchronise'?
|
||||
|
||||
\begin{columns}
|
||||
\begin{column}{0.5\textwidth}
|
||||
\includegraphics[width=\textwidth]{grand/split-cable/split-cable-delays-ch1ch4.pdf}
|
||||
\end{column}
|
||||
\begin{column}{0.5\textwidth}
|
||||
%\includegraphics[width=\textwidth]{grand/split-cable/split-cable-delay-ch1ch2-50mhz-200mVpp.pdf}
|
||||
\includegraphics[width=\textwidth]{fourier/04_signal_to_noise_fig04.png}
|
||||
\end{column}
|
||||
\end{columns}
|
||||
\end{frame}
|
||||
|
||||
% Towards GRAND
|
||||
%%%%%%%%%%%%%%%%%%%%
|
||||
\begin{frame}{Advantages of Radio Interferometry}
|
||||
\begin{columns}
|
||||
\begin{column}{0.4\textwidth}
|
||||
\begin{itemize}
|
||||
\item Trace longitudinal development of airshower
|
||||
\item Lower SNR threshold
|
||||
\item Measure depth of airshower
|
||||
\item Shower axis reconstruction
|
||||
\item Improved background rejection
|
||||
\end{itemize}
|
||||
\end{column}
|
||||
\begin{column}{0.6\textwidth}
|
||||
\begin{figure}
|
||||
\includegraphics[width=\textwidth]{2006.10348/fig01.png}
|
||||
% \caption{
|
||||
% \cite{Schoorlemmer:2020low}
|
||||
% From: \cite{Schoorlemmer:2020low}
|
||||
% }
|
||||
\end{figure}
|
||||
\end{column}
|
||||
\end{columns}
|
||||
\end{frame}
|
||||
|
||||
\begin{frame}{Physics Improvement of Radio Interferometry}
|
||||
composition measurement\\
|
||||
\vskip 1em
|
||||
\begin{frame}{Physics Improvement with Radio Interferometry}
|
||||
\begin{columns}
|
||||
\begin{column}{0.6\textwidth}
|
||||
Improved energy measurement (air-calorimetry)
|
||||
|
||||
direction reconstruction improved\\
|
||||
relevance for $\nu$s pointing back to sources
|
||||
\vskip 1em
|
||||
|
||||
Composition measurement (Fe, p, $\gamma$, $\nu$) of primary particle
|
||||
% through airshower depth Fe high, p deep, gamma deeper, neutrino deepest
|
||||
|
||||
\vskip 1em
|
||||
\visible<2->{
|
||||
Improved direction reconstruction
|
||||
% through shower axis reconstruction
|
||||
%\; Relevant for $\nu$s pointing back to sources
|
||||
}
|
||||
|
||||
|
||||
\visible<3->{
|
||||
\vspace*{\fill}
|
||||
\begin{center}
|
||||
\begin{minipage}{.6\textwidth}
|
||||
\hrule
|
||||
\centering
|
||||
\vspace{ 2em }
|
||||
\textit{Thank you!}
|
||||
\end{minipage}
|
||||
\end{center}
|
||||
%\vspace{ 4em }
|
||||
}
|
||||
\end{column}
|
||||
\begin{column}{0.4\textwidth}
|
||||
\begin{figure}
|
||||
\includegraphics[width=\textwidth]{2006.10348/fig01_a.png}
|
||||
% \caption{
|
||||
% From: \cite{Schoorlemmer:2020low}
|
||||
% }
|
||||
\end{figure}
|
||||
\end{column}
|
||||
\end{columns}
|
||||
|
||||
% \visible<2->{
|
||||
% \vspace*{\fill}
|
||||
% \begin{center}
|
||||
% \begin{minipage}{.6\textwidth}
|
||||
% \hrule
|
||||
% \centering
|
||||
% \vspace{10pt}
|
||||
% \textit{Thank you!}
|
||||
% \end{minipage}
|
||||
% \end{center}
|
||||
% \vspace{\stretch{2}}
|
||||
% }
|
||||
\end{frame}
|
||||
|
||||
|
||||
|
@ -166,12 +230,41 @@
|
|||
\section{Supplemental material}
|
||||
\begin{frame}[c]
|
||||
\centering
|
||||
\Large {
|
||||
\textcolor{blue} {
|
||||
Supplemental material
|
||||
}
|
||||
}
|
||||
\end{frame}
|
||||
|
||||
\subsection{Radio Emission}
|
||||
\begin{frame}{Polarised Radio Emission}
|
||||
\begin{columns}
|
||||
\begin{column}{0.2\textwidth}
|
||||
\centering
|
||||
Geosynchrotron
|
||||
\end{column}
|
||||
\begin{column}{0.7\textwidth}
|
||||
\includegraphics[width=\textwidth]{airshower/airshower_radio_polarisation_geomagnetic.png}%
|
||||
\end{column}
|
||||
\end{columns}
|
||||
\vfill
|
||||
\begin{columns}
|
||||
\begin{column}{0.2\textwidth}
|
||||
\centering
|
||||
Askaryan
|
||||
\end{column}
|
||||
\begin{column}{0.7\textwidth}
|
||||
\includegraphics[width=\textwidth]{airshower/airshower_radio_polarisation_askaryan.png}%
|
||||
\end{column}
|
||||
\end{columns}
|
||||
% \vfill
|
||||
% From: \cite{Huege:2017bqv}
|
||||
\end{frame}
|
||||
|
||||
|
||||
%%%%%%%%%
|
||||
\subsection{Single frequency beacon synchronisation}
|
||||
|
||||
\begin{frame}{Short period beacon synchronisation}
|
||||
\begin{figure}
|
||||
\includegraphics<1>[width=\textwidth]{beacon/08_beacon_sync_timing_outline.pdf}%
|
||||
|
@ -225,8 +318,17 @@
|
|||
\end{figure}
|
||||
\end{frame}
|
||||
|
||||
|
||||
|
||||
\subsubsection{In the field}
|
||||
\begin{frame}{GNSS clock stability II}
|
||||
\begin{columns}
|
||||
\begin{column}{0.5\textwidth}
|
||||
\includegraphics[width=\textwidth]{images/IMG_20220819_154801.jpg}
|
||||
\end{column}
|
||||
\begin{column}{0.5\textwidth}
|
||||
\includegraphics[width=\textwidth]{images/IMG_20220815_161244.jpg}
|
||||
\end{column}
|
||||
\end{columns}
|
||||
\end{frame}
|
||||
|
||||
%%%%%%%%%%%%%%
|
||||
% Bibliography
|
||||
|
|
Loading…
Reference in a new issue