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Anisotropy studies in the cosmic ray proton flux with the PAMELA experiment
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2013 (English)In: Proceedings of the 9th workshop on Science with the New Generation of High Energy Gamma-ray Experiments: From high energy gamma sources to cosmic rays, one century after their discovery, Elsevier, 2013, 123-128 p.Conference paper, Published paper (Refereed)
Abstract [en]

Using data taken by the Pamela experiment during 5 years of operation we studied the anisotropy in the arrival direction distribution of cosmic ray protons with rigidity above 40 GV. In this survey we used two different and independent techniques to investigate the large and medium anisotropy patterns in the proton spectrum. With both methods the observed distribution of arrival directions is consistent with the isotropic expectation and no significant evidence of strong anisotropies has been observed.

Place, publisher, year, edition, pages
Elsevier, 2013. 123-128 p.
Series
Nuclear Physics B - Proceedings Supplements, ISSN 0920-5632 ; 239-240
Keyword [en]
Cosmic rays, Pamela experiment
National Category
Physical Sciences
Identifiers
URN: urn:nbn:se:kth:diva-134129DOI: 10.1016/j.nuclphysbps.2013.05.020ISI: 000321940800021Scopus ID: 2-s2.0-84879872370OAI: oai:DiVA.org:kth-134129DiVA: diva2:665178
Conference
9th Workshop on Science with the New Generation of High Energy Gamma-Ray Experiments: From High Energy Gamma Sources to Cosmic Rays, One Century After Their Discovery, SciNeGHE 2012; Lecce; Italy; 20 June 2012 through 22 June 2012
Note

QC 20131118

Available from: 2013-11-19 Created: 2013-11-18 Last updated: 2015-12-03Bibliographically approved

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Pearce, Mark

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