Measurement of galactic cosmic-ray deuteron spectrum in the PAMELA experiment. Bulletin of the Russian Academy of Sciences: Physics Volume 77, Issue 5, May 2013, Pages 606-608
14 сентября 2018
207
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| Вид публикации | Статья |
| Контактные данные автора публикации | Koldobskiy, S.A.a , Formato, V.g, Adriani, O.d, Barbarino, G.C. et.al. |
| Ссылка на публикацию в интернете | www.scopus.com/record/display.url?origin=recordpage&eid=2-s2.0-84879103297&citeCnt=29&noHighlight=false&sort=plf-f&src=s&st1=MEPhI&nlo=&nlr=&nls=&sid=F0743CC1BB1CEC168410A18CB87C48A7.Vdktg6RVtMfaQJ4pNTCQ:20&sot=b&sdt=b&sl=31&s=AFFIL(MEPhI) AND PUB |
Аннотация
This work presents the results of measuring the deuteron spectrum of Galactic cosmic rays (GCRs) with the PAMELA experiment. The PAMELA is an international experiment. Its main objectives are to search for antimatter and measure proton, helium nuclei, electron, and positron spectra over a wide range of energies. In addition, the experimental setup allows the detection of deuterons and the reconstruction of their spectra at low energies. Cosmic ray deuteron spectrum and the deuteron-proton ratio measured in the PAMELA experiment in the energy range of 50-650 MeV/nucleon are presented below. © 2013 Allerton Press, Inc.
Indexed keywords
Energy ranges; Galactic cosmic rays; Helium nuclei
ПодробнееIndexed keywords
Energy ranges; Galactic cosmic rays; Helium nuclei
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