{"paper":{"title":"The results of ATIC-2 experiment for elemental spectra of cosmic rays","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A.D. Panov, A.R. Fazely, E.N. Kouznetsov, E.S. Seo, G.L. Bashindzhagyan, H.S. Ahn, J. Chang, J.H. Adams, J. Isbert, John W. Watts, J.P. Wefel, J. Wu, K.C. Kim, K.E. Batkov, M. Christl, M.I. Panasyuk, N.V. Sokolskaya, O. Ganel, R.M. Gunashingha, T.G. Guzik, V.I. Zatsepin, W.K.H. Schmidt","submitted_at":"2006-12-14T12:09:57Z","abstract_excerpt":"The results of ATIC-2 baloon experiment (2002-2003) for energy spectra of protons, He, C, O, Ne, Mg, Si, Fe, some groups of nuclei, and all-particle spectrum in primary cosmic rays are presented in energy region 50GeV--200TeV. The conclusion is that the spectra of protons and helium nuclei are essentially different (the spectrum of protons is steeper) and the spectra of protons and heavy nuclei have no-power form."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0612377","kind":"arxiv","version":1},"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"}