NUSES is a low Earth orbit pathfinder satellite for innovative particle detectors dedicated to the study of cosmic radiation, astrophysical neutrinos, Sun-Earth environment, space weather and magnetosphere-ionosphere-lithosphere coupling. The satellite will host two instruments: Terzina and Zirè. While Terzina will focus on space based detection of ultra high energy extensive air showers, Zirè will perform measurements of electrons, protons and light nuclei from few up to hundreds MeV, also testing new tools for the detection of cosmic MeV photons, and monitoring possible MILC signals. Zirè will consists of a scintillating fiber tracker, a stack of plastic scintillator counters and an array of LYSO crystals. An active veto system and a Low Energy Module (LEM) are also part of the payload. In this work we present the design of a novel tracker prototype based on plastic scintillating fibers coupled with SiPM linear arrays. The preliminary results obtained in a beam test with the prototype module will be discussed.

The light tracker based on scintillating fibers with SiPM readout of the Zirè instrument on board the NUSES space mission / Mazziotta, M. N.; Pillera, R.; Aloisio, R.; Altomare, C.; Barbato, F. C. T.; Battiston, R.; Bertaina, M.; Bissaldi, E.; Boncioli, D.; Burmistrov, L.; Cagnoli, I.; Casolino, M.; Cummings, A.; D'Ambrosio, N.; De Mitri, I.; De Robertis, G.; De Santis, C.; Di Giovanni, A.; Di Salvo, A.; Di Santo, M.; Di Venere, L.; Eser, J.; Fernandez Alonso, M.; Fontanella, G.; Fusco, P.; Garbolino, S.; Gargano, F.; Giampaolo, R. A.; Giliberti, M.; Guarino, F.; Heller, M.; Iuppa, R.; Krizmanic, J. F.; Lega, A.; Licciulli, F.; Loparco, F.; Lorusso, L.; Mariotti, M.; Mazziotta, M. N.; Mese, M.; Miyamoto, H.; Montaruli, T.; Nagai, A.; Nicolaidis, R.; Nozzoli, F.; Olinto, A. V.; Orlandi, D.; Osteria, G.; Palmieri, P. A.; Panico, B.; Panzarini, G.; Parenti, A.; Perrone, L.; Picozza, P.; Pillera, R.; Rando, R.; Rinaldi, M.; Rivetti, A.; Rizi, V.; Salamida, F.; Santero Mormile, E.; Scherini, V.; Scotti, V.; Serini, D.; Siddique, I.; Silveri, L.; Smirnov, A.; Sparvoli, R.; Tedesco, S.; Trimarelli, C.; Wu, L.; Zuccon, P.; Zugravel, S. C.. - In: POS PROCEEDINGS OF SCIENCE. - ISSN 1824-8039. - 444:(2024). (Intervento presentato al convegno 38th International Cosmic Ray Conference, ICRC 2023 tenutosi a jpn nel 2023) [10.22323/1.444.0083].

The light tracker based on scintillating fibers with SiPM readout of the Zirè instrument on board the NUSES space mission

Pillera R.;Bissaldi E.;Di Venere L.;Giliberti M.;Loparco F.;Mazziotta M. N.;Panzarini G.;Pillera R.;
2024-01-01

Abstract

NUSES is a low Earth orbit pathfinder satellite for innovative particle detectors dedicated to the study of cosmic radiation, astrophysical neutrinos, Sun-Earth environment, space weather and magnetosphere-ionosphere-lithosphere coupling. The satellite will host two instruments: Terzina and Zirè. While Terzina will focus on space based detection of ultra high energy extensive air showers, Zirè will perform measurements of electrons, protons and light nuclei from few up to hundreds MeV, also testing new tools for the detection of cosmic MeV photons, and monitoring possible MILC signals. Zirè will consists of a scintillating fiber tracker, a stack of plastic scintillator counters and an array of LYSO crystals. An active veto system and a Low Energy Module (LEM) are also part of the payload. In this work we present the design of a novel tracker prototype based on plastic scintillating fibers coupled with SiPM linear arrays. The preliminary results obtained in a beam test with the prototype module will be discussed.
2024
38th International Cosmic Ray Conference, ICRC 2023
The light tracker based on scintillating fibers with SiPM readout of the Zirè instrument on board the NUSES space mission / Mazziotta, M. N.; Pillera, R.; Aloisio, R.; Altomare, C.; Barbato, F. C. T.; Battiston, R.; Bertaina, M.; Bissaldi, E.; Boncioli, D.; Burmistrov, L.; Cagnoli, I.; Casolino, M.; Cummings, A.; D'Ambrosio, N.; De Mitri, I.; De Robertis, G.; De Santis, C.; Di Giovanni, A.; Di Salvo, A.; Di Santo, M.; Di Venere, L.; Eser, J.; Fernandez Alonso, M.; Fontanella, G.; Fusco, P.; Garbolino, S.; Gargano, F.; Giampaolo, R. A.; Giliberti, M.; Guarino, F.; Heller, M.; Iuppa, R.; Krizmanic, J. F.; Lega, A.; Licciulli, F.; Loparco, F.; Lorusso, L.; Mariotti, M.; Mazziotta, M. N.; Mese, M.; Miyamoto, H.; Montaruli, T.; Nagai, A.; Nicolaidis, R.; Nozzoli, F.; Olinto, A. V.; Orlandi, D.; Osteria, G.; Palmieri, P. A.; Panico, B.; Panzarini, G.; Parenti, A.; Perrone, L.; Picozza, P.; Pillera, R.; Rando, R.; Rinaldi, M.; Rivetti, A.; Rizi, V.; Salamida, F.; Santero Mormile, E.; Scherini, V.; Scotti, V.; Serini, D.; Siddique, I.; Silveri, L.; Smirnov, A.; Sparvoli, R.; Tedesco, S.; Trimarelli, C.; Wu, L.; Zuccon, P.; Zugravel, S. C.. - In: POS PROCEEDINGS OF SCIENCE. - ISSN 1824-8039. - 444:(2024). (Intervento presentato al convegno 38th International Cosmic Ray Conference, ICRC 2023 tenutosi a jpn nel 2023) [10.22323/1.444.0083].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11589/281440
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