1. Detector response and calibration of the cosmic-ray detector of the Sileye-3/Alteino experiment
- Author
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M. G. Korotkov, S. Avdeev, M. P. De Pascale, N. Zampa, V. Bonvicini, P. Picozza, P. Spillantini, A. Kolmykov, Eva Reali, V. Zaconte, E. Segreto, Walter G. Sannita, Victor Benghin, Andrea Vacchi, E. Rantucci, Marco Ricci, R. Scrimaglio, Vyacheslav Shurshakov, R. Vittori, C. Fuglesang, K.A. Trukhanov, V.P. Salnitskii, Gianluigi Zampa, N. Vavilov, V. Bidoli, A. M. Galper, G. Mazzenga, P. Carlson, A. Popov, M. Minori, O.I. Shevchenko, V.P. Petrov, Mirko Boezio, Livio Narici, and Marco Casolino
- Subjects
Atmospheric Science ,Silicon detector ,Physics::Instrumentation and Detectors ,Astrophysics::High Energy Astrophysical Phenomena ,Aerospace Engineering ,Cosmic ray ,Astrophysics ,Radiation ,Scintillator ,International Space Station ,Flash (photography) ,Optics ,Nuclear abundances ,Stack (abstract data type) ,Calibration ,Cosmic rays ,Physics ,business.industry ,Settore FIS/01 - Fisica Sperimentale ,Detector ,Astrophysics::Instrumentation and Methods for Astrophysics ,Astronomy and Astrophysics ,Settore FIS/07 - Fisica Applicata(Beni Culturali, Ambientali, Biol.e Medicin) ,Geophysics ,Space and Planetary Science ,General Earth and Planetary Sciences ,business - Abstract
The experiment Sileye-3/Alteino is constituted by a cosmic-ray silicon detector and an electroencephalograph. The main scientific aims include the investigation of the Light Flash phenomenon, the study of astronaut brain activity in space when subject to cosmic rays, the measurement of cosmic rays and the radiation environment inside the International Space Station. The experiment was operating on board the station from 27 April to 5 May 2002. The cosmic-ray detector is composed of eight silicon strip planes triggered by two scintillators placed on top and bottom of the stack. The detector is capable of identifying nuclei from B to As in the energy range above ≃60 MeV/n. Also protons and lighter particles are registered although with a reduced efficiency. The instrument was active in the Pirs module of the station for 130 h. In this work, we describe the silicon strip detector characteristics and its calibration performed using cosmic-ray nuclei.
- Published
- 2006