{"paper":{"title":"Multichannel Data Acquisition System for Scintillation Detectors of the Emma Experiment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"A.F. Yanin, B.K. Lubsandorzhiev, G.V. Volchenko, H. Fynbo, I.M. Dzaparova, J. Joutsenvaara, J. Sarkamo, L.B. Bezrukov, L. Olanter\\\"a, L.V. Inzhechik, M. Slupecki, O.V. Mineev, P. Kuusiniemi, T. Enqvist, T. R\\\"aih\\\"a, V.B. Petkov, V.I. Volchenko, W. Trzaska, Y.G. Kudenko, Zh. Sh. Guliev","submitted_at":"2011-01-24T10:34:31Z","abstract_excerpt":"The multichannel data acquisition system is intended to be used in the EMMA experiment studying cosmic rays. The array will be in the Pihasalmi mine (central Finland) at a depth of about 85 m. The scintillator counters (SC-1) of the array are cast plastic scintillators with a wavelength of each SC-1 detector is 12.2{\\times}12.2{\\times}3.0 cm^3. 16 SC-1 detectors are placed in the metal case of 50.0{\\times}50.0{\\times}13.0 cm^3 dimension. Each case, called SC-16 detector, contains electronics of preliminary processing of signals and operating mode stabilization. The whole of the array will cont"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.4489","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"}