2004/03/31 by S. Haino, T. Sanuki, K. Abe +33 · 1 citation
Physics and Astronomy · #Astronomy #Astrophysics #COSMIC cancer database #Cosmic ray #Dark Matter and Cosmic Phenomena #Neutrino Physics Research #Nuclear physics #Optics #Particle Detector Development and Performance #Particle physics #Physics #Primary (astronomy) #Spectral line #Spectrometer #astro-ph
paper · pdf · doi:10.1016/j.physletb.2004.05.019
published as Phys.Lett.B594:35-46,2004 · 26 pages, 9 figures, 3 tables, Submitted to Phys. Lett. B
arxiv created 2004/03/31 · openalex publication_date 2004/06/16 · arxiv updated 2014/10/13 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Primary and atmospheric cosmic-ray spectra were precisely measured with the BESS-TeV spectrometer. The spectrometer was upgraded from BESS-98 to achieve seven times higher resolution in momentum measurement. We report absolute fluxes of primary protons and helium nuclei in the energy ranges, 1–540 GeV and 1–250 GeV/n, respectively, and absolute flux of atmospheric muons in the momentum range 0.6–400 GeV/c.