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  • The Extreme Energy Events HECR array: status and perspectives
    Gnesi, I; Abbrescia, M; Avanzini, C; Baldini, L; R Baldini Ferroli; Batignani, G; Bencivenni, G; Bossini, E; Chiavassa, A; Cicalo, C; Cifarelli, L; Coccetti, F; Coccia, E; Corvaglia, A; De Gruttola, D; De Pasquale, S; A Di Giovanni; D'Incecco, M; Dreucci, M; Fabbri, F L; Fattibene, E; Ferraro, A; Frolov, V; Galeotti, P; Garbini, M; Gemme, G; Grazzi, S; Gustavino, C; Hatzifotiadu, D; Liciulli, F; La Rocca, P; Maggiora, A; Rodriguez, O Maragoto; Maron, G; Martelli, B; Mazziotta, M N; Miozzi, S; Nania, R; Noferini, F; Nozzoli, F; Panareo, M; Panetta, M P; Paoletti, R; Park, W; Perasso, L; Pilo, F; Piragino, G; Riggi, F; Righini, G C; Rizzi, M; Sartorelli, G; Scapparone, E; Schioppa, M; Scribano, A; Selvi, M; Serci, S; Siddi, E; Squarcia, S; Stori, L; Taiuti, M; Terreni, G; Visnyei, O B; Vistoli, M C; Votano, L; Williams, M C S; Zani, S; Zichichi, A; Zuyeuski, R

    arXiv.org, 03/2017
    Paper, Journal Article

    The Extreme Energy Events Project is a synchronous sparse array of 52 tracking detectors for studying High Energy Cosmic Rays (HECR) and Cosmic Rays-related phenomena. The observatory is also meant to address Long Distance Correlation (LDC) phenomena: the network is deployed over a broad area covering 10 degrees in latitude and 11 in longitude. An overview of a set of preliminary results is given, extending from the study of local muon flux dependance on solar activity to the investigation of the upward-going component of muon flux traversing the EEE stations; from the search for anisotropies at the sub-TeV scale to the hints for observations of km-scale Extensive Air Shower (EAS).

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