source: JEM-EUSO/ICRC2013/EusoBalloonDetector/v0r0/icrc2013-EBDet-morettodagoret.tex @ 130

Last change on this file since 130 was 130, checked in by dagoret, 11 years ago

add first version of eusoballoon detector

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1%%
2% 33nd International Cosmic Ray Conference - 2013 - Rio de Janeiro, Brazil
3% Template adapted from the 2011 ICRC template.
4
5\documentclass[a4paper]{article}
6
7\usepackage{icrc2013}
8
9%The paper title
10\title{Detailed description of EUSO-BALLOON instrument}
11
12%The short title to appear at the header of the pages.
13\shorttitle{Instrumentation for JEM EUSO }
14
15%All paper authors
16\authors{
17
18C. Moretto$^{1}$, S. Dagoret-Campagne$^{1}$, J.H. Adams$^{19}$, P. von Ballmoos$^{2}$,P. Barrillon$^{1}$, J. Bayer$^{5}$, M. Bertaina$^{12}$, S. Blin-Bondil$^{1}$, F. Cafagna$^{7}$, M. Casolino$^{13,10,11}$, C. Catalano$^{2}$,P. Danto$^{4}$, A. Ebersoldt$^{6}$, T. Ebisuzaki$^{13}$, J. Evrard$^{4}$, Ph. Gorodetzky$^{3}$, A. Haungs$^{6}$, A. Jung$^{14}$, Y. Kawasaki$^{13}$, H. Lim$^{14}$, G. Medina-Tanco$^{15}$, H. Miyamoto$^{1}$, D. Monnier-Ragaigne$^{1}$, T. Omori$^{13}$, G. Osteria$^{9}$, E. Parizot$^3$, I.H. Park$^{14}$, P. Picozza$^{13,10,11}$, G. Pr\'ev\^ot$^{3}$,  H. Prieto$^{13,17}$, M. Ricci$^{8}$, M.D. Rodr’guez Fr’as$^{17}$, A. Santangelo$^{5}$, J. Szabelski$^{16}$, Y. Takizawa$^{13}$, K. Tsuno$^{13}$ 
19for the JEM-EUSO Collaboration$^{19}$.
20}
21
22%All the affiliations.
23\afiliations{
24$^1$ Laboratoire de lÕAcc\'el\'erateur Lin\'eaire, Univ Paris Sud-11, CNRS/IN2P3, Orsay, France\\
25$^2$ Institut de Recherche en Astrophysique et Plan\'etologie, Toulouse, France\\
26$^3$ AstroParticule et Cosmologie, Univ Paris Diderot, CNRS/IN2P3, Paris, France\\
27$^4$ Centre National d'Etudes Spatiales, Centre Spatial de Toulouse, France\\
28$^5$ Institute for Astronomy and Astrophysics, Kepler Center, University of TŸbingen, Germany\\
29$^6$ Karlsruhe Institute of Technology (KIT), Germany\\
30$^7$ Istituto Nazionale di Fisica Nucleare - Sezione di Bari, Italy\\
31$^8$ Istituto Nazionale di Fisica Nucleare - Laboratori Nazionali di Frascati, Italy\\
32$^9$ Istituto Nazionale di Fisica Nucleare - Sezione di Napoli, Italy\\
33$^{10}$ Istituto Nazionale di Fisica Nucleare - Sezione di Roma Tor Vergata, Italy\\
34$^{11}$ UniversitaÕ di Roma Tor Vergata - Dipartimento di Fisica, Roma, Italy\\
35$^{12}$ Dipartimento di Fisica dellÕ Universit`a di Torino and INFN Torino, Torino, Italy\\
36$^{13}$ RIKEN Advanced Science Institute, Wako, Japan\\
37$^{14}$ Sungkyunkwan University, Suwon-si, Kyung-gi-do, Republic of Korea\\
38$^{15}$ Universidad Nacional Aut—noma de MŽxico (UNAM), Mexico\\
39$^{16}$ National Centre for Nuclear Research, Lodz, Poland\\
40$^{17}$ Universidad de Alcal‡ (UAH), Madrid, Spain\\
41$^{18}$ University of Alabama in Huntsville, Huntsville, USA\\
42$^{19}$ http://jemeuso.riken.jp
43}
44
45%email address of the contact person
46\email{moretto@lal.in2p3.fr} 
47
48%The abstract.
49\abstract{EUSO-Balloon is a pathfinder prefiguring the future fluorescence space telescope JEM-EUSO that should be installed on-board of the Internal Space Station before the end of this decade.
50This telescope will be the payload of a stratospheric balloon operated by CNES, starting its flight campaign in 2014.
51Current technical development for JEM-EUSO are a challenge for a space project, have been implemented in EUSO-Balloon.
52In this poster, the complete design of this instrument will be presented. It consists of an advanced modular telescope structure including a set of three Fresnel lenses having an excellent focusing capability onto its pixelized focal surface of its UV Camera. This camera is very sensitive to single photons, with 6 orders of magnitude dynamic range thanks to an adaptive gain, and fast enough to observe speed-of-light phenomena. The camera is an array of multianodes photomultipliers, which dynodes are driven by Crockoft Walton HV generators capable of switching down the gain in few microseconds to protect the photodetectors against strongly luminous events.
53The analog signals at anodes are digitized continuously each time window (2.5 microsecond) by an ASIC, performing two kinds of signal measurements and readout by a FPGA applying a first level trigger algorithm.
54The Electronics is operated by a digital processing unit comprising a CPU associated to Clocks generators board and a GPS receiver, an event filtering board based on a FPGA and an House-Keeping unit for the instrument monitoring. The CPU controls both acquisition and the data storage.
55This processing unit is interfaced with the CNES telemetry system to receive commands from ground and to download samples of the event or monitoring data.
56The whole instrument operates autonomously with a battery package that drives a series of power supply boards that deliver the required voltage to each board.
57}
58
59%The keywords
60\keywords{JEM-EUSO, UHECR, space instrument, balloon experiment, instrumentation}
61
62
63\begin{document}
64\maketitle
65
66
67\section{Introduction}
68EUSO-Ballon is a reduced scaled telescope aiming at verifying the conceptual design as well as the technologies foreseen to be applied for the construction of the future space telescope JEM-EUSO mission~\cite{bib:EUSOperf}.
69The scientific and technical goals on its mission are reviewed in the reference~\cite{bib:EBpath}. This instrument is foreseen to be operated in a standalone mode, onboard of a stratospheric balloon.
70The instrument design had to be as close as possible to that of the JEM-EUSO. Nevertheless the special environmental conditions which are much more severe than in space required much precautions in the design
71and implied dedicated tests under the realisation of prototypes.
72The section~\ref{icdc}
73with Fresnel Since autumn 2011, the instrument has been designed to be operated onboard a stratospheric Balloon 
74d it is presently at the stage on the final assembly, integration and test.
75
76\section{The Instrument}
77
78\subsection{General characteristics and functions}
79
80\subsection{Optics}
81
82\subsection{Front-End Electronics}
83
84\subsection{Data acquisition}
85
86\subsection{Monitoring}
87
88\subsection{Power supply and electrical architecture}
89
90\subsection{Instrument mechanics}
91
92\section{Assembly and Tests}
93
94\section{Operation and Analysis}
95
96\section{Conclusion}
97
98
99\newpage
100
101\section{Latex instructions}
102
103\subsection{Equations}
104Equations can be introduced without numbering
105
106\begin{eqnarray*}
107 y=a \ddot x + b \dot x + c
108\end{eqnarray*}
109
110or with numbering
111
112\begin{equation}
113 \chi^{2}= \sum\limits_{i=0}^{n}\frac{(t_{i}-t_{0}-ax_{i}-by_{i}-
114 \alpha r_{i}/c)^{2}}{\sigma_{i}^{2}}
115\end{equation}
116
117The array environment can be used to introduce multiple-line
118equations not to numerate:
119
120\begin{eqnarray*}
121(x+y)(x-y) & = & x^2-xy+xy-y^2 \\
122           & = & x^2-y^2 \\
123   (x+y)^2 & = & x^2+2xy+y^2
124\end{eqnarray*}
125
126or partly to numerate:
127
128\begin{eqnarray}
129(x+y)(x-y) & = & x^2-xy+xy-y^2 \nonumber \\
130           & = & x^2-y^2 \\
131   (x+y)^2 & = & x^2+2xy+y^2
132\end{eqnarray}
133
134The array environment can be used for expression of the following
135type:
136
137\[ \left( \begin{array}{c}
138\left| \begin{array}{cc} x_{11} & x_{12} \\ x_{21} & x_{22}
139\end{array} \right| x \\y \end{array} \right) \]
140
141This is an example on show to add space:
142
143\begin{equation}
144f(n) = \left\{
145  \begin{array}{l l}
146    n/2 & \quad \textrm{if $n$ is even}\\
147    -(n+1)/2 & \quad \textrm{if $n$ is odd}
148  \end{array} \right.
149\end{equation}
150
151and how to remove space:
152
153\begin{equation}
154\left(\!\!
155    \begin{array}{c}
156      n \\
157      r
158    \end{array}
159  \!\!\right) = \frac{n!}{r!(n-r)!}
160\end{equation}
161
162 \begin{figure*}[!t]
163  \centering
164  \includegraphics[width=\textwidth]{icrc2013-template-01}
165  \caption{Wide figure example. Conference webpage header.}
166  \label{wide_fig}
167 \end{figure*}
168
169
170
171\subsection{Lists}
172
173You may create an itemized list with the places to see in Rio de Janeiro:
174
175\begin{itemize}
176\item Copabacana Beach
177\item Corcovado
178\item Sugar Loaf
179\end{itemize}
180
181An enumerated list with the rhythms to listen:
182
183\begin{enumerate}
184\item Bossa Nova
185\item Choro
186\item Samba
187\end{enumerate}
188
189Or a customized list with the food and drinks to taste:
190
191\begin{itemize}
192\item[$\gamma$] Brigadeiro
193\item[$\beta$]  Caipirinha
194\item[$\alpha$] Feijoada
195\end{itemize}
196
197\subsection{Footnotes}
198
199Footnotes can be created with the footnote command\footnote{This is
200a footnote example.}.
201
202
203\subsection{Figures}
204
205Single column figures and images as in figure \ref{simp_fig}
206preferred. However, large figures can be made to span two columns. If you have to introduce two column
207figures(e.g., figure \ref{wide_fig}), please verify that they do not
208overflow the margins of the text.
209
210
211 \begin{figure}[t]
212  \centering
213  \includegraphics[width=0.4\textwidth]{icrc2013-template-02}
214  \caption{Simple figure example. Rio Scenarium Restaurant / Bar / Nightclub. Venue of the Conference Dinner.}
215  \label{simp_fig}
216 \end{figure}
217
218\subsection{Tables}
219
220Tables can be done at one (Table \ref{table_single}) and two columns. \\
221
222\begin{table}[h]
223\begin{center}
224\begin{tabular}{|l|c|c|}
225\hline Month & Temperature ($^\circ$C) & Precipitation (mm) \\ \hline
226June   & 22  & 81.3 \\ \hline
227July   & 22  & 55.9 \\ \hline
228August & 22  & 50.8 \\ \hline
229\end{tabular}
230\caption{Weather conditions in the city of Rio de Janeiro. Average temperature and precipitation in each month.}
231\label{table_single}
232\end{center}
233\end{table}
234
235
236
237\section{Conclusions}
238
239A list of references should be placed at the end of the paper. See
240the below example. The citation to the references can be written as
241\cite{bib:EUSOperf} or \cite{bib:EUSOperf,bib:schoenberg}.
242
243\vspace*{0.5cm}
244\footnotesize{{\bf Acknowledgment:}{This work was partially supported by CNES
245}
246
247\begin{thebibliography}{}
248
249\bibitem{bib:EUSOperf} J.H. Adams Jr. et al. - JEM-EUSO Collaboration, Astroparticle Physics 44 (2013) 76-90 http://dx.doi.org/10.1016/j.astropartphys.2013.01.008
250
251\bibitem{bib:EBpath} P. von Ballmoos et al. - EUSO-BALLOON: a pathfinder for observing UHECR's from space, this proceedings, paper 1171,
252
253\bibitem{bib:EBSimulation} T. Mernik et al. ESAF-Simulation of the EUSO-Balloon, this proceedings, paper 875,
254
255
256\bibitem{bib:Optics} Manufacturing of the TA-EUSO and EUSO-Balloon lenses, this proceedings, paper 1040,
257
258
259\bibitem{bib:ASIC } H. Miyamoto et al., Performance of the SPACIROC front-end ASIC for JEM-EUSO, this proceedings, paper 1089,
260\bibitem{bib:CCB} J. Bayer et al., Second level trigger and Cluster Control Board for the JEM-EUSO mission,this proceedings, paper 432,
261
262\bibitem{bib:FrontEndEl}P. Barrillon et al., The Front-End Electronics of the EUSO-Balloon UV camera,this proceedings, paper 765,
263
264\bibitem{bib:Calib} P. Gorodetzky et al., Absolute calibrations of JEM-EUSO,this proceedings, paper 858,
265\bibitem{bib: PMT} C. Blaksley, Photomultiplier Tube Sorting for JEM-EUSO and EUSO-Balloon, this proceedings, paper 628,
266
267\bibitem{bib:OffOnLineAna} L.W. Piotrowski et al. On-line and off-line data analysis for the TA-EUSO and BALLOON-EUSO experiments, this proceedings, paper 713,
268
269
270
271\end{thebibliography}
272
273\end{document}
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