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Launch of the space experiment PAMELA
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2008 (English)In: Advances in Space Research, ISSN 0273-1177, E-ISSN 1879-1948, Vol. 42, no 3, 455-466 p.Article in journal (Refereed) Published
Abstract [en]

PAMELA is a satellite borne experiment designed to study with great accuracy cosmic rays of galactic, solar, and trapped nature in a wide energy range (protons 80 MeV-700 GeV, electrons 50 MeV-400 GeV). Main objective is the study of the antimatter component: antiprotons (80 MeV-190 GeV), positrons (50 MeV-270 GeV) and search for antimatter with a precision of the order of 10-8. The experiment, housed on board the Russian Resurs-DK I satellite, was launched on June 15th, 2006 in a 350 x 600 km orbit with all inclination of 70'. The detector is composed of a series of scintillator counters arranged at the extremities of a permanent magnet spectrometer to provide charge, time-of-flight, and rigidity information. Lepton/hadron identification is performed by a silicon-tungsten calorimeter and a neutron detector placed at the bottom of the device. An anticounter system is used offline to reject false triggers coming from the satellite. In self-trigger mode the calorimeter, the neutron detector, and a shower tail catcher are capable of an independent measure of the lepton component up to 2 TeV. In this work we describe the experiment, its scientific objectives, and the performance in the first months after launch.

Place, publisher, year, edition, pages
Elsevier, 2008. Vol. 42, no 3, 455-466 p.
Keyword [en]
cosmic rays, antimatter, satellite borne experiment
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-33157DOI: 10.1016/j.asr.2007.07.023ISI: 000257684300009Scopus ID: 2-s2.0-44849118875OAI: oai:DiVA.org:kth-33157DiVA: diva2:413679
Note

QC 20110429

Available from: 2011-04-29 Created: 2011-04-29 Last updated: 2017-12-11Bibliographically approved

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Pearce, Mark

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Carlson, PerHofverberg, PetterLund, JensOrsi, SilvioPearce, Mark
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