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Measurement of Lithium and Beryllium cosmic-ray abundances by the PAMELA experiment
Vise andre og tillknytning
2015 (engelsk)Inngår i: Proceedings of Science, Proceedings of Science (PoS) , 2015Konferansepaper, Publicerat paper (Fagfellevurdert)
Abstract [en]

The PAMELA experiment is collecting particles along a low Earth semi-polar orbit on board of Resurs-DK1 satellite since June 2006. The combined information of a silicon tracking system and a scintillator hodoscope provides redundant light-element identification capabilities, via multiple ionization energy-loss measurements. The instrument design is not optimized for nuclei detection, whose high ionization signal progressively saturates the detectors. However, Li and Be nuclei can still be identified by using the full set of information, which allows to efficiently select the two elements against the background of more abundant elements. The main issues of the analysis aiming to optimize the Li and Be selection are discussed in this paper. Preliminary results on the elemental abundances will be presented at the conference.

sted, utgiver, år, opplag, sider
Proceedings of Science (PoS) , 2015.
HSV kategori
Identifikatorer
URN: urn:nbn:se:kth:diva-194747Scopus ID: 2-s2.0-84988719714OAI: oai:DiVA.org:kth-194747DiVA: diva2:1047282
Konferanse
34th International Cosmic Ray Conference, ICRC 2015, 30 July 2015 through 6 August 2015
Merknad

QC 20161117

Tilgjengelig fra: 2016-11-17 Laget: 2016-10-31 Sist oppdatert: 2016-11-17bibliografisk kontrollert

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