Response function of a stacked GSO(Ce) spectrometer to cosmic-rays

H. Murohka, K. Anami, G. Wakabayashi, H. Yoshida, A. Nohtomi, Y. Uozumi, T. Sakae, M. Matoba, T. Maki, N. Koori

Research output: Contribution to journalArticlepeer-review

2 Citations (Scopus)

Abstract

The stacked GSO(Ce) spectrometer consists of three plastic scintillation detectors, three rectangular GSO(Ce) scintillators (43×43×43 mm3) and a large cylindrical GSO(Ce) (φ62× 120 mm3). It has been developed to measure proton emission spectra up to 450 MeV. As a preliminary test, γ-rays from 137Cs and cosmic-rays were measured. We compare the results of the stacked GSO(Ce) spectrometer and those of the stacked NaI(Tl) spectrometer. The performances of the stacked GSO(Ce) spectrometer in intermediate energy region are discussed.

Original languageEnglish
Pages (from-to)484-488
Number of pages5
JournalIEEE Transactions on Nuclear Science
Volume44
Issue number3 PART 1
DOIs
Publication statusPublished - 1997

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Nuclear Energy and Engineering
  • Electrical and Electronic Engineering

Fingerprint Dive into the research topics of 'Response function of a stacked GSO(Ce) spectrometer to cosmic-rays'. Together they form a unique fingerprint.

Cite this