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Cosmic ray study with the PAMELA experiment
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.ORCID iD: 0000-0001-7011-7229
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.
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Number of Authors: 62
2013 (English)In: Journal of Physics, Conference Series, ISSN 1742-6588, E-ISSN 1742-6596, Vol. 409, no 1Article in journal (Refereed) Published
Abstract [en]

In six years of data collection years in space, the experiment PAMELA has discovered very interesting features in cosmic rays, namely in the fluxes of protons, helium, electrons, that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the Galaxy. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. The continuous particle detection is allowing a constant monitoring of the solar activity and detailed study of the solar modulation for a long period, giving important improvements to the comprehension of the heliosphere mechanisms. PAMELA is also measuring the radiation environment around the Earth, and has recently discovered an antiproton radiation belt.

Place, publisher, year, edition, pages
2013. Vol. 409, no 1
Keyword [en]
Dark matter, Data collection, Heliospheres, Measurements of, Particle detection, Radiation environments, Solar activity, Solar modulation, Experiments, Galaxies, Protons, Radiation belts, Solar energy, Cosmic rays
National Category
Subatomic Physics
Identifiers
URN: urn:nbn:se:kth:diva-134684DOI: 10.1088/1742-6596/409/1/012003ISI: 000315408200003Scopus ID: 2-s2.0-84874296905OAI: oai:DiVA.org:kth-134684DiVA: diva2:676586
Conference
23rd European Cosmic Ray Symposium, ECRS 2012 and 32nd Russian Cosmic Ray Conference, 3 July 2012 through 7 July 2012, Moscow
Note

QC 20131206. Author count: 62

Available from: 2013-12-06 Created: 2013-11-27 Last updated: 2017-12-06Bibliographically approved

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Pearce, Mark

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