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Taccetti, F.; Adriani, O.; Bonechi, L.; Bongi, M.; Boscherini, M.; Castellini, G.; D'Alessandro, R.; Gabbanini, A.; Grandi, M.; Papini, P.; Piccardi, S.; Ricciarini, S.; Spillantini, P.; Straulino, S.; Tesi, M.; Vannuccini, E., E-mail: taccetti@iroe.fi.cnr.it2002
AbstractAbstract
[en] The Pamela apparatus will be launched at the end of 2002 on board of the Resurs DK Russian satellite. The tracking system, composed of six planes of silicon sensors inserted inside a permanent magnetic field was intensively tested during these last years. Results of tests have shown a good signal-to-noise ratio and an excellent spatial resolution, which should allow to measure the antiproton flux in an energy range from 80 MeV up to 190 GeV. The production of the final detector modules is about to start and mechanical and thermal tests on the tracking tower are being performed according to the specifications of the Russian launcher and satellite
Primary Subject
Source
S0168900202005351; Copyright (c) 2002 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.; Country of input: International Atomic Energy Agency (IAEA)
Record Type
Journal Article
Journal
Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment; ISSN 0168-9002; ; CODEN NIMAER; v. 485(1-2); p. 78-83
Country of publication
ANTIPROTON BEAMS, COSMIC RADIATION, COSMIC RAY DETECTION, DIELECTRIC TRACK DETECTORS, GEV RANGE 01-10, GEV RANGE 100-1000, GEV RANGE 10-100, MAGNETIC FIELDS, MEV RANGE 100-1000, MEV RANGE 10-100, PARTICLE TRACKS, PERFORMANCE TESTING, SATELLITES, SI SEMICONDUCTOR DETECTORS, SIGNAL-TO-NOISE RATIO, SPATIAL RESOLUTION
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