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Latest results from PAMELA
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2009 (English)Conference paper, Published paper (Refereed)
Abstract [en]

The PAMELA experiment is a satellite-borne apparatus designed to study charged particles in the cosmic radiation, with a particular focus on antiparticles. The detector is housed on the Resurs-DK1 satellite and it is taking data since June 2006. The main parts of the apparatus are a magnetic spectrometer, which is equipped with a silicon-microstrip tracking system and which is used to measure the rigidity and the charge of particles, and a silicon/tungsten electromagnetic calorimeter which provides particle identification. The main results about the antiparticles component of cosmic rays obtained during the first 500 days of data taking are summarized here.

Place, publisher, year, edition, pages
2009. Vol. 194, p. 123-128
Series
Nuclear physics b-proceedings supplements, ISSN 0920-5632
Keywords [en]
SOLAR MINIMUM ACTIVITY, RAY ANTIPROTON FLUX, CALORIMETER, POSITRONS, ELECTRON
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-30390DOI: 10.1016/j.nuclphysbps.2009.07.011ISI: 000272247800023Scopus ID: 2-s2.0-71149087318OAI: oai:DiVA.org:kth-30390DiVA, id: diva2:401163
Conference
GGI--Dark Matter and Dark Energy 2009
Note

QC 20110301 Galileo-Galilei-Institute Conference on Dark Matter and Dark Energy, Florence, ITALY, JAN 19-MAR 12, 2009

Available from: 2011-03-01 Created: 2011-02-24 Last updated: 2016-05-18Bibliographically approved

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Pearce, Mark

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