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Cosmic–ray positron energy spectrum measured by PAMELA
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2013 (English)In: Proceedings of the 33rd International Cosmic Rays Conference, ICRC 2013, Sociedade Brasileira de Fisica , 2013Conference paper, Published paper (Refereed)
Abstract [en]

The PAMELA satellite borne experiment is designed to study cosmic rays with great accuracy in a wide energy range. One of PAMELA’s main goal is the study of the antimatter component of cosmic rays. The experiment, housed on board the Russian satellite Resurs–DK1, was launched on June 15th 2006 and it is still taking data. In this work we present the measurement of galactic positron energy spectrum in the energy range between 500 MeV and few hundred GeV. 

Place, publisher, year, edition, pages
Sociedade Brasileira de Fisica , 2013.
Keywords [en]
Cosmic–Rays, Neural Networks, PAMELA, Positrons, Cosmic rays, Electrons, Spectroscopy, Energy ranges, Positron energy, Satellite-borne experiment, Wide energy range, Cosmology
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-237203Scopus ID: 2-s2.0-85052290420ISBN: 9788589064293 OAI: oai:DiVA.org:kth-237203DiVA, id: diva2:1262190
Conference
33rd International Cosmic Rays Conference, ICRC 2013; Rio de Janeiro; Brazil; 2 July 2013 through 9 July 2013
Funder
Swedish Research Council
Note

QC 20181109

Available from: 2018-11-09 Created: 2018-11-09 Last updated: 2018-11-09Bibliographically approved

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Pearce, Mark

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