Chemical composition of primary cosmic rays with energies from 1015 to 1016.5 eV

Y. ShirasakiF. KakimotoS. OgioN. GirondaM. TakedaT. KanekoH. YoshiiToshihiko BabaSakae SanoK. Nishi2026-03-222026-03-22200110.1016/s0927-6505(00)00166-3https://doi.org/10.1016/s0927-6505(00)00166-3https://andeanlibrary.org/handle/123456789/53857Citaciones: 10enCosmic rayPhysicsPrimary (astronomy)SupernovaAstrophysicsMonte Carlo methodStarsChemical compositionNuclear physicsChemical composition of primary cosmic rays with energies from 1015 to 1016.5 eVarticle