Author/Authors :
Alfaro، نويسنده , , R. and De Donato، نويسنده , , C. and D’Olivo، نويسنده , , J.C. and Guzm?n، نويسنده , , Jeferson A. and Medina-Tanco، نويسنده , , G. and Moreno Barbosa، نويسنده , , E. and Paic، نويسنده , , G. and Pati?o Salazar، نويسنده , , E. and Salazar Ibarguen، نويسنده , , H. and Sanchez، نويسنده , , F.A. and Supanitsky، نويسنده , , A.D. and Valdés-Galicia، نويسنده , , J.F. and Vargas Trevi?o، نويسنده , , A.D. and Vergara Lim?n، نويسنده , , S. and Villase?or، نويسنده , , L.M.، نويسنده ,
Abstract :
Muon telescopes have multiple applications in the area of cosmic ray research. We are currently building such a detector with the objective of comparing the ground penetration of muon vs. electron-gamma signals originated in cosmic ray showers. The detector is composed by a set of three parallel dual-layer scintillator planes, buried at fixed depths ranging from 120 to 600 g / cm 2 . Each layer is 4 m 2 and is composed by 49 rectangular strips of 4 cm × 2 m , oriented at a 90 ∘ angle with respect to its companion layer, which gives an xy -coincidence pixel of 4 × 4 cm 2 . The scintillators are MINOS extruded polystyrene strips, with an embedded Bicron BC92 wavelength shifting (WLS) fibers, of 1.5 mm in diameter. Light is collected by Hamamatsu H7546B multi-anode PMTs of 64 pixels. The front-end (FE) electronics works in counting mode and signals are transmitted to the surface DAQ stage using low-voltage differential signaling (LVDS). Any strip signal above threshold opens a GPS-tagged 2 μ s data collection window. Data, including signal and background, are acquired by a system of FPGA (Spartan 2E) boards and a single-board computer (TS7800).
