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Search for cosmic ray electron-positron anisotropies with the Pamela data
Ist Nazl Fis Nucl, Sez Naples, I-80126 Naples, Italy..
KTH, Skolan för teknikvetenskap (SCI), Fysik.
KTH, Skolan för teknikvetenskap (SCI), Fysik.
KTH, Skolan för teknikvetenskap (SCI), Fysik.ORCID-id: 0000-0001-7011-7229
Vise andre og tillknytning
2013 (engelsk)Inngår i: 23RD EUROPEAN COSMIC RAY SYMPOSIUM (AND 32ND RUSSIAN COSMIC RAY CONFERENCE), IOP PUBLISHING LTD , 2013, artikkel-id 012055Konferansepaper, Publicerat paper (Fagfellevurdert)
Abstract [en]

Using data taken by the Pamela experiment during 5 years of operation we studied the anisotropy in the arrival direction of cosmic ray electrons and positrons with energy above 40 GeV. We report on a study of anisotropy in the e(+/-) flux at different angular scales extending from 30 degrees up to 90 degrees, further more a directional analysis has been performed around the Sun direction. The observed distribution of arrival directions is consistent with the isotropic expectation at any angular scale used in this study and no significant evidence of strong anisotropies has been observed, also the analysis around the Sun direction did not show any significant excess.

sted, utgiver, år, opplag, sider
IOP PUBLISHING LTD , 2013. artikkel-id 012055
Serie
Journal of Physics Conference Series, ISSN 1742-6588 ; 409
HSV kategori
Identifikatorer
URN: urn:nbn:se:kth:diva-243828DOI: 10.1088/1742-6596/409/1/012055ISI: 000315408200055Scopus ID: 2-s2.0-84874302275OAI: oai:DiVA.org:kth-243828DiVA, id: diva2:1285945
Konferanse
23rd European Cosmic Ray Symposium (ECRS) / 32nd Russian Cosmic Ray Conference, JUL 03-07, 2012, Lomonosov Moscow State Univ, Moscow, RUSSIA
Merknad

QC 20190205

Tilgjengelig fra: 2019-02-05 Laget: 2019-02-05 Sist oppdatert: 2019-04-08bibliografisk kontrollert

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