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Measurements of cosmic-ray antiprotons with PAMELA
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.
2011 (English)In: Astrophysics and Space Sciences Transactions (ASTRA), ISSN 1810-6528, E-ISSN 1810-6536, Vol. 7, no 2, 225-228 p.Article in journal (Refereed) Published
Abstract [en]

The PAMELA experiment is a satellite-borne apparatus designed to study charged particles, and especially antiparticles, in the cosmic radiation. The apparatus is mounted on the Resurs DK1 satellite which was launched on 15 June 2006. PAMELA has been traveling around the earth along an elliptical and semi-polar orbit for almost five years. It mainly consists of a permanent magnetic spectrometer, a time of flight system and an electromagnetic imaging calorimeter, which allows antiprotons to be identified from a dominating cosmic-ray background. New measurements of the cosmic-ray antiproton flux and the antiproton-to-proton flux ratio between 60 MeV and 180 GeV are presented, employing data collected between June 2006 and December 2008. Compared to previous experiments, PAMELA extends the energy range of antiproton measurements and provides significantly higher statistics. The derived antiproton flux and antiproton-to-proton flux ratio indicates that the main source of cosmic-ray antiprotons is considered to be secondary production and no primary contribution has to be invoked.

Place, publisher, year, edition, pages
Copernicus Publications , 2011. Vol. 7, no 2, 225-228 p.
Keyword [en]
cosmic ray, antiproton, PAMELA
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-80704DOI: 10.5194/astra-7-225-2011Scopus ID: 2-s2.0-79959717961OAI: oai:DiVA.org:kth-80704DiVA: diva2:496674
Note
on behalf of PAMELA collaboration. QC 20120214Available from: 2012-02-14 Created: 2012-02-10 Last updated: 2017-12-07Bibliographically approved

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