{"paper":{"title":"First results of the cosmic ray NUCLEON experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"A. Kurganov, A. Panov, A. Tkachenko, A. Turundaevskiy, A. Voronin, D. Karmanov, D. Podorozhny, D. Polkov, E. Atkin, I. Kovalev, I. Kudryashov, L. Sveshnikova, L. Tkachev, M. Merkin, N. Gorbunov, O. Vasiliev, S. Filippov, S. Porokhovoy, V. Bulatov, V. Dorokhov, V. Grebenyuk, V. Shumikhin","submitted_at":"2017-02-08T10:08:13Z","abstract_excerpt":"The NUCLEON experiment was designed to study the chemical composition and energy spectra of galactic cosmic ray nuclei from protons to zinc at energies of $\\sim10^{11}$--$10^{15}$\\,eV per particle. The research was carried out with the NUCLEON scientific equipment installed on the Russian satellite \"Resurs-P\" No.\\,2 as an additional payload. This article presents the results for the measured nuclei spectra related to the first approximately 250 days of the scientific data collection during 2015 and 2016. The all-particle spectrum and the spectra of p, He, C, O, Ne, Mg, Si and Fe are presented."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1702.02352","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}