Abstract:The PAMELA experiment is a satellite-borne apparatus designed to study charged particles in the cosmic radiation with a particular focus on antiparticles. PAMELA is mounted on the Resurs DK1 satellite that was launched from the Baikonur cosmodrome on June 15 th 2006. The PAMELA apparatus comprises a time-of-flight system, a magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail catcher scintillator and a neutron detector. The combination of these devices… Show more
“…The Resurs-DK1 satellite, which hosts the apparatus, was launched into a semipolar (70 ∘ inclination) and elliptical (350-610 km altitude) orbit on 15 June 2006. The instrument consists of a magnetic spectrometer equipped with a silicon tracking system, a time-of-flight system shielded by an anticoincidence system, an electromagnetic calorimeter, and a neutron detector [Picozza et al, 2007]. Details about apparatus performance, proton selection, detector efficiencies, and experimental uncertainties can be found elsewhere [see, e.g., Adriani et al, 2013].…”
“…The Resurs-DK1 satellite, which hosts the apparatus, was launched into a semipolar (70 ∘ inclination) and elliptical (350-610 km altitude) orbit on 15 June 2006. The instrument consists of a magnetic spectrometer equipped with a silicon tracking system, a time-of-flight system shielded by an anticoincidence system, an electromagnetic calorimeter, and a neutron detector [Picozza et al, 2007]. Details about apparatus performance, proton selection, detector efficiencies, and experimental uncertainties can be found elsewhere [see, e.g., Adriani et al, 2013].…”
“…PAMELA is a satellite-borne experiment [1] built to detect charged particles in cosmic rays with particular attention to antiparticles. PAMELA is in orbit from June 15th 2006.…”
“…Other important scientific goals include: the study of solar physics and solar modulation during the 24 th solar minimum, and the study of the cosmic-ray electron energy spectrum up to several TeV, thereby allowing possible contributions from local sources to be identified [1]. Table 1 shows the design goals for PAMELA performance, presenting the cosmic-ray components and energy ranges over which PAMELA will give new results.…”
Section: Introductionmentioning
confidence: 99%
“…PAMELA is installed inside a pressurized container mounted onboard the Russian Resurs DK-1 earth-observation satellite that was launched into space by a Soyuz-U rocket on June 15 th , 2006 from the Baikonur cosmodrome (Kazakhstan) [1]. The satellite orbit is elliptical and quasi-polar, with an inclination of 70.4º and an altitude varying between 350 and 610 km.…”
, and, since then, it is in continuous data taking. The calorimeter of the PAMELA apparatus has been designed to identify antiprotons from an electron background and positrons from a background of protons with high efficiency and rejection power. It is a sampling silicon-tungsten imaging calorimeter, which comprises 44 single-sided silicon sensor planes (380 µm thick) interleaved with 22 plates of tungsten absorber (0.74 X 0 each). It is the first silicon-tungsten calorimeter to be launched in space. In this work we present the in-orbit performance of the calorimeter, including the measured identification capabilities. The calorimeter provides a proton rejection factor of ~10 5 while keeping a high efficiency in selecting electrons and positrons, thus fulfilling the identification power needed to reach the primary scientific objectives of PAMELA. We show also that, after almost two years of operation in space, the calorimeter is still performing nominally.
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