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Two years of flight of the Pamela experiment: Results and perspectives
Visa övriga samt affilieringar
2009 (Engelska)Ingår i: Journal of the Physical Society of Japan, ISSN 0031-9015, E-ISSN 1347-4073, Vol. 78, nr Suppl. A, s. 35-40Artikel i tidskrift (Refereegranskat) 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 antinuclei with a precision of the order of 10~8). The experiment, housed on board the Russian Resurs-DKl satellite, was launched on June, 15th 2006 in a 350 x 600 km orbit with an inclination of 70 degrees. In this work we describe the scientific objectives and the performance of PAMELA in its first two years of operation. Data on protons of trapped, secondary and galactic nature - as well as measurements of the December 13th 2006 Solar Particle Event - are also provided.

Ort, förlag, år, upplaga, sidor
2009. Vol. 78, nr Suppl. A, s. 35-40
Nyckelord [en]
Antimatter, Cosmic rays, Dark matter, Solar particle events, Trapped cosmic rays
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Identifikatorer
URN: urn:nbn:se:kth:diva-153600Scopus ID: 2-s2.0-66849106758OAI: oai:DiVA.org:kth-153600DiVA, id: diva2:753052
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QC 20141007

Tillgänglig från: 2014-10-07 Skapad: 2014-10-06 Senast uppdaterad: 2017-12-05Bibliografiskt granskad

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Pearce, Mark

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Hofverberg, PetterPearce, MarkCarlson, Per
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