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Simulations studies for the Mini-EUSO detector

Authors :
P. Gorodetzky
R. Bonino
Guillaume Prévôt
Francesco Fenu
F. Capel
L.W. Piotrowski
Toshikazu Ebisuzaki
P. Picozza
Matteo Battisti
P. Klimov
Marco Mignone
Alexander S. Belov
Christer Fugelsang
Francesca Bisconti
G. Suino
M. Bertaina
Naoto Sakaki
Raffaella Bonino
Dario Barghini
Gregorio Suino
Fumiyoshi Kajino
Mario E. Bertaina
A. Belov
Zbigniew Plebaniak
L. Marcelli
F. Bisconti
Jacek Szabelski
H. Miyamoto
J. Szabelski
M. Casolino
E. Parizot
Igor Churilo
G. Prevôt
Hiroko Miyamoto
G. Cambiè
I. Churilo
Laura Marcelli
C. Fuglesang
Kenji Shinozaki
Y. Takizawa
M. Mignone
Lech Piotrowski
Pavel Klimov
Marco Ricci
F. Kajino
N. Sakaki
M. Manfrin
Wlodzimierz Marszal
Marco Casolino
T. Ebisuzaki
Alessio Golzio
M. Ricci
A. Golzio
W. Marszal
D. Barghini
M. Battisti
K. Shinozaki
E. Reali
Enzo Reali
F. Fenu
Massimo Manfrin
Z. Plebaniak
Francesca Capel
Piergiorgio Picozza
Yoshiyuki Takizawa
Philippe Gorodetzky
Etienne Parizot
Giorgio Cambiè
AstroParticule et Cosmologie (APC (UMR_7164))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
JEM-EUSO
Source :
PoS, 37th International Cosmic Ray Conference, 37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.334, ⟨10.22323/1.395.0334⟩
Publication Year :
2021
Publisher :
arXiv, 2021.

Abstract

International audience; Mini-EUSO is a mission of the JEM-EUSO program flying onboard the International Space Station since August 2019. Since the first data acquisition in October 2019, more than 35 sessions have been performed for a total of 52 hours of observations. The detector has been observing Earth at night-time in the UV range and detected a wide variety of transient sources all of which have been modeled through Monte Carlo simulations. Mini-EUSO is also capable of detecting meteors and potentially space debris and we performed simulations for such events to estimatetheir impact on future missions for cosmic ray science from space. We show here examples of the simulation work done in this framework to analyze the Mini-EUSO data. The expected response of Mini-EUSO with respect to ultra high energy cosmic ray showers has been studied. The efficiency curve of Mini-EUSO as a function of primary energy has been estimated and the energy threshold for Cosmic Rays has been placed to be above $10^{21}$ eV. We compared the morphology of several transient events detected during the mission with cosmic ray simulations and excluded that they can be due to cosmic ray showers. To validate the energy threshold of the detector, asystem of ground based flashers is being used for end-to-end calibration purposes. We therefore implemented a parameterization of such flashers into the JEM-EUSO simulation framework and studied the response of the detector with respect to such sources.

Details

Database :
OpenAIRE
Journal :
PoS, 37th International Cosmic Ray Conference, 37th International Cosmic Ray Conference, Jul 2021, Berlin, Germany. pp.334, ⟨10.22323/1.395.0334⟩
Accession number :
edsair.doi.dedup.....dffd68ddfb1f9ee4b1c12e11df9c58dd
Full Text :
https://doi.org/10.48550/arxiv.2112.12150