m-thesis-documentation/presentations/2023-06-01_step_up_interview/2023-STEP_UP.tex

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\title[STEP-UP: Interferometry in GRAND]{% and BEACON]{
{ \large STEP'UP Interview}\\
{
Investigating interferometry in\\%
GRAND\footnote{ Giant Radio Array for Neutrino Detection}
% and BEACON\footnote{Beam forming Elevated Array for COsmic Neutrinos}
}
}
\date{June, 2023}
\author[E.T. de Boone]{
E.T. de Boone
% \\
% \vspace{2em}
% Advisors: Olivier Martineau, LPNHE\\
% \quad\quad\quad\quad\quad\, Harm Schoorlemmer, IMAPP
}
\begin{document}
{
\setbeamertemplate{footline}{} % no page number here
\frame{ \titlepage }
}
\section{My Background}
\begin{frame}{My Background}
Studies @Radboud University, Nijmegen
\begin{itemize}
\item Master's Physics and Astronomy {\small (\textit{1yr courses + 1yr internship})}\\
\quad { \small Specialisation: Particle and Astrophysics }\\
\quad { \small Minor: Computational Data Science }\\
\vspace*{1em}
\item Master's Internship: \\
\quad {\small Supervisor: Harm Schoorlemmer, IMAPP, Radboud University}\\
\quad {\small ``Enhancing Timing Accuracy in Air Shower Radio Detectors'' }\\
\end{itemize}
\end{frame}
\note[itemize]{
\item Interests since Bachelor's, continued in Master's
\begin{itemize}
\item Ultra High Energy particles
\item Radio detection \& Hardware experimenting
\end{itemize}
\item Now wrapping up Master and full year's worth of internship
\item Why start internship? (Experimental)
}
% Cosmic Rays and Radio
%%%%%%%%%
\section{Radio and Airshowers}
\begin{frame}{Ultra High Energy particles}
\begin{figure}
\includegraphics[width=\textwidth]{grand/astroparticletypes_grand.jpg}%
\imagecite{GRAND:2018iaj}
\end{figure}
\end{frame}
\note[itemize]
{
\item Ultra High Energies (EeV $10^{18}$ eV) (Sources)
\item Propagation effects (Magnetic Field deflections, Horizons)
\item Multiple classes (Different combinations of effects)
}
%%
\begin{frame}{Air Showers: Atmospheric Depth \& Composition}
\begin{columns}
\begin{column}{0.45\textwidth}
\begin{figure}
\hspace*{-1em}
\includegraphics[width=\textwidth]{airshower/shower_development_depth_iron_proton_photon.pdf}%
\imagecredit{H. Schoorlemmer}
\end{figure}
\end{column}
\begin{column}{0.45\textwidth}
Enhanced Xmax measurement with Interferometry\\
$\mapsto$ particle identification\\
\begin{figure}
\centering
\includegraphics[width=\textwidth]{2006.10348/fig03_b.png}%
\imagecite{Schoorlemmer:2020low}
\end{figure}
\end{column}
\end{columns}
\end{frame}
\note[itemize]
{
\item Statistical discrimation: high Z at high altitudes
\item FD claims 20 g/cm2, Fe/p ~ 50 g/cm2
\item Radio Interferometry helps in Xmax measurement
}
\section{Radio Interferometry and Timing}
\begin{frame}{Effect of Timing Synchronisation}
%\vspace*{-2em}
Interferometry: Amplitude + Timing information of the $\vec{E}$-field\\
\vspace*{ 0.8em }
\begin{columns}
%\hfill
\begin{column}{0.4\textwidth}
\vfill
\hyperlink{fig:sine:repairments}{\includegraphics[width=1.1\textwidth]{radio_interferometry/trace_overlap/on-axis/dc_grid_power_time_fixes.py.repair_none.axis.trace_overlap.repair_none.pdf}}%
\vspace*{\fill}
\hyperlink{fig:sine:grid_power}{\includegraphics[width=1.1\textwidth]{radio_interferometry/dc_grid_power_time_fixes.py.X400.repair_none.scale4d.pdf}}
\end{column}
\hfill
\begin{column}{0.4\textwidth}
\vfill
\hyperlink{fig:sine:repairments}{\includegraphics[width=1.1\textwidth]{radio_interferometry/trace_overlap/on-axis/dc_grid_power_time_fixes.py.repair_full.axis.trace_overlap.repair_full.pdf}}%
\vspace*{\fill}
\hyperlink{fig:sine:grid_power}{\includegraphics[width=1.1\textwidth]{radio_interferometry/dc_grid_power_time_fixes.py.X400.repair_all.scale4d.pdf}}%
\end{column}
\hfill
\end{columns}
\end{frame}
\note{
}
\begin{frame}{Timing Synchronisation: Beacon}
\begin{columns}
\begin{column}{0.6\textwidth}
\hspace*{1em}
Required time accuracy $\sim 1 \mathrm{ns}$\\
\vspace*{1em}
\hspace*{1em}
\visible<2->{
\textcolor{red}{GNSS}, in Auger $\gtrsim 5 \mathrm{ns}$\\
}
\hspace*{1em}
\vspace*{1em}
\visible<2->{
\textcolor{blue}{Beacon}: Pulse or Sine
}
\vspace*{\fill}
\begin{figure}
\hspace*{-2em}
\begin{tikzpicture}
\node[anchor=south west, inner sep=0] (image) at (0,0) {\includegraphics[width=\textwidth]{beacon/array_setup_gps_transmitter_cows.png}};
\begin{scope}[x={(image.south east)}, y={(image.north west)}]
%\draw[help lines,xstep=.1,ystep=.1] (0,0) grid (1,1);
%\foreach \x in {0,1,...,9} { \node [anchor=north] at (\x/10,0) {0.\x}; }
%\foreach \y in {0,1,...,9} { \node [anchor=east] at (0,\y/10) {0.\y}; }
\draw[red, ultra thick, visible on=<{2-}>] (0.85,0.87) circle [radius=8mm];
\draw[blue, ultra thick, visible on=<{2-}>] (0.23,0.32) circle [radius=8mm];
\end{scope}
\end{tikzpicture}
\imagecredit{H. Schoorlemmer}
\end{figure}
\end{column}
\begin{column}{0.5\textwidth}
\centering
\vspace*{\fill}
\onslide<3->{\hyperlink{fig:pulse:accuracy}{\includegraphics[width=\textwidth]{pulse/time_res_vs_snr_multiple_dt_small.pdf}}}%
\vspace*{\fill}
\onslide<3->{\hyperlink{fig:sine:accuracy}{\includegraphics[width=\textwidth]{beacon/time_res_vs_snr_f67.pdf}}}%
\vspace*{\fill}
\end{column}
\end{columns}
\end{frame}
\note{
Single frequency interest due to Auger (TV@67MHz)
}
\section{Radio Interferometry in GRAND}
\begin{frame}{Radio Interferometry in GRAND}
\begin{figure}
\centering
\vspace*{\fill}
\hspace*{-2em}
\includegraphics[width=1.13\textwidth]{grand/roadmap-per-2023-01-shortened.jpg}%
%\includegraphics<2->[width=0.5\textwidth]{grand/roadmap-per-2023-01-shortened.jpg}%
\imagesource{Adapted from \url{https://grand.cnrs.fr/overview/roadmap/}}
\end{figure}
\end{frame}
% GRAND
%%%%%%%%%%%%%%%
%\note[itemize]
%{
% \item GRAND radio-only, heavy development
% \item pathfinders upto 2026 (Auger reference, Europe testbed, China array)
% \item ultra high energy has low hits, need large area
%}
\begin{frame}{Radio Interferometry in GRAND in Conclusion}
\begin{columns}
\begin{column}{0.4\textwidth}
\hspace*{-1.2em}
\begin{figure}
\vspace*{\fill}
\vspace*{2.4em}
\includegraphics[width=1\textwidth]{grand/roadmap-per-2023-01-shortened-prototyping.jpg}%
\imagesource{Adapted from \url{https://grand.cnrs.fr/overview/roadmap/}}
\vspace*{\fill}
\end{figure}
\end{column}
\hspace*{-2em}
\begin{column}{0.65\textwidth}
\begin{enumerate}
\item Timing Requirement in~Hardware\\
\quad test beacon at Auger/GP300
\vspace*{2em}
\item Setup Interferometric Analyses\\
\quad adapt to GRAND
\vspace*{2em}
\item Particle ID through Xmax\\
and Shower Axis reconstruction
\end{enumerate}
\vspace*{1em}
\end{column}
\end{columns}
\end{frame}
% \only<2-> {
% Timing Requirements:\\
% \quad synchronisation schemes investigated in internship,\\
% \quad opportunity to implement and test (e.g.~Nan\c{c}ay)\\
% }
%
% \only<3-> {
% \vspace*{1em}
% Interferometric Analyses:\\
% \quad enhances Xmax resolution\\
% }
%
% \vspace{\stretch{100}}
%\vspace*{2em}
%GRAND Goals:\\
% \quad Largest UHECR observatory, \\
% \quad Multi-messenger science case,\\
% \quad meaningful contribution to a new experiment\\
%\end{frame}
%\begin{frame}{Radio Interferometry in GRAND}
% \visible<2->{
% \vspace*{\fill}
% \begin{center}
% \begin{minipage}{.6\textwidth}
% \hrule
% \centering
% \vspace{ 2em }
% \textit{Thank you!}
% \end{minipage}
% \end{center}
% %\vspace{ 4em }
% }
%%%%%%%%%%%%%%%
% Backup slides
%%%%%%%%%%%%%%%
\appendix
\begin{frame}[c]
\centering
\Large {
\textcolor{blue} {
Supplemental material
}
}
\end{frame}
\section*{Table of Contents}
\begin{frame}{Table of Contents}
\tableofcontents
\end{frame}
\begin{frame}{GRAND}
\begin{figure}
\includegraphics[width=1\textwidth]{grand/GRAND-detection-principle-1.png}%
\imagecite{GRAND:2018iaj}
\end{figure}
\end{frame}
\section{Radio Emission}
\begin{frame}{Airshower development}
\begin{figure}
\includegraphics[width=0.9\textwidth]{1607.08781/fig02a_airshower+detectors.png}
\imagecite{Schroder:2016hrv}
\end{figure}
\end{frame}
\begin{frame}{Polarised Radio Emission}
\begin{columns}
\begin{column}{0.2\textwidth}
\centering
Geosynchrotron
\end{column}
\begin{column}{0.7\textwidth}
\centering
\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}
\centering
\includegraphics[width=\textwidth]{airshower/airshower_radio_polarisation_askaryan.png}%
\imagecite{Huege:2017bqv}
\end{column}
\end{columns}
% \vfill
\end{frame}
\section{Radio Interferometry}
\begin{frame}{Radio Interferometry: Concept}
\begin{columns}
\begin{column}{0.4\textwidth}
\begin{figure}
\includegraphics<1>[width=\textwidth]{radio_interferometry/rit_schematic_base.pdf}%
\includegraphics<2>[width=\textwidth]{radio_interferometry/rit_schematic_far.pdf}%
\includegraphics<3>[width=\textwidth]{radio_interferometry/rit_schematic_close.pdf}%
\includegraphics<4>[width=\textwidth]{radio_interferometry/rit_schematic_true.pdf}%
\end{figure}
\end{column}
\begin{column}{0.6\textwidth}
\vspace*{\fill}
\begin{itemize}
\item<1-> Measure signal $S_i(t)$ at antenna $\vec{a_i}$
\item<2-> Calculate light travel time \\[5pt]
\quad $\Delta_i(\vec{x}) = \frac{ \left| \vec{x} - \vec{a_i} \right| }{c} n_{eff}$
\item<2-> Sum waveforms accounting \\
for time delay \\[5pt]
\quad $S(\vec{x}, t) = \sum S_i( t + \Delta_i(\vec{x}) )$
\end{itemize}
\vspace*{\fill}
\begin{figure}% Spatially
\includegraphics<1>[width=0.8\textwidth]{radio_interferometry/single_trace.png}%
\includegraphics<2>[width=0.8\textwidth]{radio_interferometry/trace_overlap_bad.png}%
\includegraphics<3>[width=0.8\textwidth]{radio_interferometry/trace_overlap_medium.png}%
\includegraphics<4>[width=0.8\textwidth]{radio_interferometry/trace_overlap_best.png}%
\end{figure}
\end{column}
\end{columns}
\end{frame}
\begin{frame}{Radio Interferometry: Image}
\begin{figure}
\centering
\includegraphics[width=0.7\textwidth]{2006.10348/fig01.png}%
\imagecite{Schoorlemmer:2020low}
\end{figure}
\end{frame}
\begin{frame}{Radio Interferometry: Xmax Resolution vs Timing Resolution}
\begin{figure}
\centering
\includegraphics[width=0.7\textwidth]{2006.10348/fig03_b.png}%
\imagecite{Schoorlemmer:2020low}
\end{figure}
\end{frame}
\section{Time Synchronisation}
\subsection{Expected Time Accuracies vs SNR}
\subsubsection{Sine}
\begin{frame}{Sine wave: Accuracy}
\begin{figure}
\includegraphics[width=\textwidth]{beacon/time_res_vs_snr.pdf}
\label{fig:sine:accuracy}
\end{figure}
\end{frame}
\begin{frame}{Sine wave: SNR}
\includegraphics[width=\textwidth]{ZH_simulation/signal_to_noise_definition.pdf}
\end{frame}
\subsubsection{Pulse}
\begin{frame}{Pulse Template}
\begin{figure}
\includegraphics[width=\textwidth]{pulse/time_res_vs_snr_multiple_dt.pdf}
\label{fig:pulse:accuracy}
\end{figure}
\end{frame}
\begin{frame}{Pulse Template: SNR}
\begin{columns}
\begin{column}{0.45\textwidth}
\centering
Signal to Noise
\includegraphics[width=\textwidth]{pulse/antenna_signal_to_noise_6.pdf}
\end{column}
\hfill
\begin{column}{0.45\textwidth}
\centering
Impulse Response
\includegraphics[width=\textwidth]{pulse/filter_response.pdf}
\end{column}
\end{columns}
\end{frame}
\begin{frame}{Pulse Template: Timing}
\begin{figure}
\includegraphics[width=\textwidth]{pulse/correlation_tdt0.2_zoom.pdf}
\label{fig:pulse:correlation}
\end{figure}
\end{frame}
%%%%%%%%%
\subsection{Single Frequency Beacon}
\begin{frame}{Short period beacon synchronisation}
\begin{figure}
%\centering
\hspace*{-5em}
\includegraphics<1>[width=1.3\textwidth]{beacon/08_beacon_sync_timing_outline.pdf}%
\includegraphics<2>[width=1.3\textwidth]{beacon/08_beacon_sync_synchronised_outline.pdf}%
\includegraphics<3>[width=1.3\textwidth]{beacon/08_beacon_sync_synchronised_period_alignment.pdf}%
\end{figure}
\end{frame}
\begin{frame}{Time resolving short period beacon: phase vs full}
\begin{columns}
\begin{column}{0.45\textwidth}
{ Phase reparation }
\includegraphics[width=\textwidth]{radio_interferometry/trace_overlap/on-axis/dc_grid_power_time_fixes.py.repair_phases.axis.trace_overlap.repair_phases.pdf}%
\vfill
\includegraphics[width=\textwidth]{radio_interferometry/dc_grid_power_time_fixes.py.X400.repair_phases.scale4d.pdf}%
\label{fig:sine:repairments}
\end{column}
\hfill
\begin{column}{0.45\textwidth}
{ Phase + Period reparation }
\includegraphics[width=\textwidth]{radio_interferometry/trace_overlap/on-axis/dc_grid_power_time_fixes.py.repair_full.axis.trace_overlap.repair_full.pdf}%
\vfill
\includegraphics[width=\textwidth]{radio_interferometry/dc_grid_power_time_fixes.py.X400.repair_all.scale4d.pdf}%
\end{column}
\end{columns}
\end{frame}
\begin{frame}{Time resolving short period beacon}
\begin{figure}
\centering
\includegraphics<1>[width=\textwidth]{radio_interferometry/dc_grid_power_time_fixes.py.X400.repair_none.scale4d.pdf}
\includegraphics<2>[width=\textwidth]{radio_interferometry/dc_grid_power_time_fixes.py.X400.repair_phases.scale4d.pdf}
\includegraphics<3>[width=\textwidth]{radio_interferometry/dc_grid_power_time_fixes.py.X400.repair_all.scale4d.pdf}
\includegraphics<4>[width=\textwidth]{radio_interferometry/dc_grid_power_time_fixes.py.X400.no_offset.scale4d.pdf}
\label{fig:sine:grid_power}
\end{figure}
\end{frame}
%%%%%%%%%%
\section{GNSS clock stability}
\begin{frame}{GNSS clock stability I}
\begin{columns}
\begin{column}{0.4\textwidth}
\begin{figure}
\centering
\includegraphics[width=0.8\textwidth]{grand/setup/antenna-to-adc.pdf}
\caption{
GRAND Digitizer Unit's ADC to antennae
}
\end{figure}
\end{column}
\hfill
\begin{column}{0.5\textwidth}
\begin{figure}
\includegraphics[width=\textwidth]{grand/setup/channel-delay-setup.pdf}%
\caption{
Channel filterchain delay experiment
}
\end{figure}
\end{column}
\end{columns}
\end{frame}
\begin{frame}{GNSS filterchain delay experiment}
\begin{columns}
\begin{column}{0.5\textwidth}
\centering
Pulse
\includegraphics[width=\textwidth]{grand/split-cable/split-cable-delays-ch1ch4.pdf}
\end{column}
\begin{column}{0.5\textwidth}
\centering
50MHz Sinewave
\includegraphics[width=\textwidth]{grand/split-cable/split-cable-delay-ch1ch2-50mhz-200mVpp.pdf}
%\includegraphics[width=\textwidth]{fourier/04_signal_to_noise_fig04.png}
Delay $ \lesssim 150\mathrm{ps}$
\end{column}
\end{columns}
\end{frame}
\begin{frame}{GNSS clock stability II}
\begin{figure}
\centering
\includegraphics[width=0.7\textwidth]{grand/setup/grand-gps-setup.pdf}
\caption{
GNSS stability experiment
}
\end{figure}
\end{frame}
\subsection{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}
\subsection{White Rabbit}
\begin{frame}{White Rabbit: GNSS}
\begin{figure}
\includegraphics<1>[width=0.85\textwidth]{gnss/phase-delocked-gps-white-rabbit-setup-colored.pdf}%
\includegraphics<2>[width=0.8\textwidth]{gnss/phase-locked-gps-white-rabbit-setup-colored.pdf}%
\end{figure}
\end{frame}
\begin{frame}{White Rabbit: Precision Time Protocol}
\begin{figure}
\includegraphics[height=0.8\textheight]{white-rabbit/protocol/wrptpMSGs_1.pdf}
\imagecite{WRPTP}
\end{figure}
\end{frame}
\begin{frame}{White Rabbit: Delay model}
\begin{figure}
\includegraphics[width=\textwidth]{white-rabbit/protocol/delaymodel.pdf}
\imagecite{WRPTP}
\end{figure}
\end{frame}
\begin{frame}{White Rabbit: Clocks Reference}
\begin{figure}
\centering
\hspace*{-5em}
\includegraphics[width=1.35\textwidth]{clocks/wr-clocks.pdf}
\end{figure}
\end{frame}
%%%%%%%%%%%%%%
% Bibliography
%%%%%%%%%%%%%%
\section*{References}
\begin{frame}[allowframebreaks]
\frametitle{References}
\printbibliography
\end{frame}
\end{document}