{"paper":{"title":"Modulations of the Cosmic Muon Signal in Ten Years of Borexino Data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.ins-det"],"primary_cat":"hep-ex","authors_text":"A. Caminata, A. Chepurnov, A. Derbin, A. Di Ludovico, A. Formozov, A. Goretti, A. Jany, Aldo Ianni, Andrea Ianni, A. Pocar, A. Porcelli, A. Razeto, A. Re, A. Romani, A. Sotnikov, A. Vishneva, B. Caccianiga, B. Neumair, B. Opitz, C. Galbiati, C. Ghiano, C. Hagner, D. Basilico, D. Bick, D. Bravo, D. D'Angelo, D. Franco, D. Guffanti, D. Jeschke, D. Korablev, D. Semenov, E. Hungerford, E. Litvinovich, E. Meroni, E. Unzhakov, F. Calaprice, F. Cavanna, F. Gabriele, F. Lombardi, F. Ortica, F. von Feilitzsch, G. Bellini, G. Bonfini, G. Korga, G. Lukyanchenko, G. Manuzio, G. Raikov, G. Ranucci, G. Testera, G. Zuzel, I. Bolognino, I. Drachnev, I. Machulin, J. Benziger, J. Maricic, J. Martyn, J. Thurn, K. Altenm\\\"uller, K. Choi, K. Fomenko, K. Zuber, L. Collica, L. Di Noto, L.F.F. Stokes, L. Ludhova, L. Lukyanchenko, L. Miramonti, L. Oberauer, L. Papp, L. Pietrofaccia, M. Agostini, M. Carlini, M. Giammarchi, M. Gromov, M. Gschwender, M. Laubenstein, M. Meyer, M. Misiaszek, M. Nieslony, M. Pallavicini, M. Redchuk, M. Skorokhvatov, M. Toropova, M. Wojcik, M. Wurm, N. Pilipenko, N. Rossi, \\\"O. Penek, O. Smirnov, O. Zaimidoroga, P. Cavalcante, P. Lombardi, R.B. Vogelaar, R. Tartaglia, S. Appel, S. Caprioli, S. Davini, S. Kumaran, S. Marcocci, S. Meighen-Berger, S. Rottenanger, S. Sch\\\"onert, S. Weinz, S. Zavatarelli, The Borexino Collaboration, T. Houdy, T. Lachenmaier, V.A. Kudryavtsev, V. Atroshchenko, V. Kobychev, V. Muratova, V. Orekhov, X.F. Ding, Y. Suvorov, Z. Bagdasarian, Z. Yokley","submitted_at":"2018-08-13T13:41:47Z","abstract_excerpt":"We have measured the flux of cosmic muons in the Laboratori Nazionali del Gran Sasso at 3800\\,m\\,w.e. to be $(3.432 \\pm 0.003)\\cdot 10^{-4}\\,\\mathrm{{m^{-2}s^{-1}}}$ based on ten years of Borexino data acquired between May 2007 and May 2017. A seasonal modulation with a period of $(366.3 \\pm 0.6)\\,\\mathrm{d}$ and a relative amplitude of $(1.36 \\pm0.04)\\%$ is observed. The phase is measured to be $(181.7 \\pm 0.4)\\,\\mathrm{d}$, corresponding to a maximum at the 1$^\\mathrm{st}$ of July. Using data inferred from global atmospheric models, we show the muon flux to be positively correlated with the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1808.04207","kind":"arxiv","version":3},"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"}