Lithium and beryllium isotopes in the pamela-experiment
2015 (English)In: Proceedings of Science, Proceedings of Science (PoS) , 2015Conference paper (Refereed)
On the 15th of June 2006, the PAMELA satellite-borne experiment was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The apparatus comprises a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anti-coincidence system, a shower tail counter scintillator and a neutron detector. The scientific objectives addressed by the mission are the measurement of the antiprotons and positrons spectra in cosmic rays, the hunt for antinuclei as well as the determination of light nuclei fluxes from hydrogen to oxygen in a wide energy range and with very high statistics. In this paper the identification capability for lithium and beryllium isotopes for two different techniques are presented, combining the rigidity measurement from the magnetic spectrometer with the velocity information derived either with the time-of-flight or with multiple dE/dx measurements in the calorimeter. Preliminary results of the isotopic ratios will be presented.
Place, publisher, year, edition, pages
Proceedings of Science (PoS) , 2015.
IdentifiersURN: urn:nbn:se:kth:diva-194742ScopusID: 2-s2.0-84988692835OAI: oai:DiVA.org:kth-194742DiVA: diva2:1047383
34th International Cosmic Ray Conference, ICRC 2015, 30 July 2015 through 6 August 2015
QC 201611172016-11-172016-10-312016-11-17Bibliographically approved