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Results from PAMELA
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2011 (English)In: NUCL PHYS B-PROC SUP, 2011, Vol. 217, 243-248 p.Conference paper, Published paper (Refereed)
Abstract [en]

The PAMELA satellite experiment was launched into low earth orbit on June 15(th) 2006. The combination of a permanent magnet silicon strip spectrometer and a silicon-tungsten imaging calorimeter allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV - several hundred GeV). A primary scientific goal is to search for dark matter particle annihilation by measuring the energy spectra of cosmic ray antiparticles. Latest results from the PAMELA experiment are presented with a particular focus on cosmic ray antiprotons and positrons.

Place, publisher, year, edition, pages
2011. Vol. 217, 243-248 p.
Series
Nuclear physics b-proceedings supplements, ISSN 0920-5632
Keyword [en]
SOLAR MINIMUM ACTIVITY, RAY ANTIPROTON FLUX, POSITRONS, ELECTRONS, ORBIT
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-47998DOI: 10.1016/j.nuclphysbps.2011.04.111ISI: 000295296500058Scopus ID: 2-s2.0-80051626170OAI: oai:DiVA.org:kth-47998DiVA: diva2:456749
Conference
Neutrino Oscillation Workshop (NOW), Otranto, ITALY, SEP 05-11, 2010
Note
QC 20111115Available from: 2011-11-15 Created: 2011-11-15 Last updated: 2011-11-15Bibliographically approved

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Pearce, Mark

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