Buried plastic scintillator muon telescope (BATATA)

R. ALFARO; C. DE DONATO; J. C. DOLIVO; A. GUZMÁN; G. MEDINA-TANCO; E. MORENO BARBOSA; G. PAIC; E. PATIÑO SALAZAR; H. SALAZAR IBARGUEN; F. A. SÁNCHEZ; A. D. SUPANITSKY; J. F. VALDÉS-GALICIA; A. D. VARGAS TREVIÑO; S. VERGARA LIMÓN; L. M. VILLASEÑOR

Encuentro; 11th Pisa Meeting on Advanced Detectors; 2009

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 x 2 m, oriented at a 903 angle with respect to its companion layer, which gives an xy-coincidence pixel of 4 x 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 ms data collection window. Data, including signal and background, are acquired by a system of FPGA (Spartan 2E) boards and a single-board computer (TS7800).