Juan José Blanco, Mr. - Dr.
Universidad de Alcalá (UAH), Madrid, Spain
       
       
Session 5 - Poster

Tragaldabas: a muon ground-based detector for the stuty of the solar activity

H. Alvarez-Pol (8), A. Blanco (3), J.J. Blanco (1), J. Collazo (9), P. Fonte (3), J.A. Garzon (9), A. Gomez (7), G. Kornakov (6), T. Kurtukian (2), L. Lopes (3), M. Morales (9,11), A. Morozova (4), M.A. Pais (4), M. Palka (5), V. Perez Munuzuri (10), P. Rey (7), P. Ribeiro (4), M. Seco (8), J. Taboada (10); 1 - Univ. Alcalá. Alcalá de Henares, Spain, 2 - CEN-Bordeaux, Bordeaux-Gradignan, France, 3 - LIP-Coimbra. Coimbra, Portugal, 4 - Univ. Coimbra, Coimbra, Portugal, 5 - Jagellionan Univ. Cracow, Poland, 6 - TU-Darmstad, Darmstadt, Germany, 7 - CESGA, S. de Compostela, Spain, 8 - Depto. de Fisica de Particulas & IGFAE - Univ. Santiago de Compostela, S. de Compostela, Spain, 9 - LabCAF Univ. Santiago de Compostela, S. de Compostela, Spain, 10 - Meteogalicia, Xunta de Galicia, S. de Compostela, Spain
       

A new RPC-based cosmic ray detector, TRAGALDABAS (acronym of "TRAsGo for the AnaLysis of the nuclear matter Decay, the Atmosphere, the earth's B-field And the Solar activity”) has been installed at the Univ. of Santiago de Compostela, Spain (N:42°52'34", W:8°33'37"). The detector, in its present layout, consists of two 1.8 m2 planes of two 1mm-gap glass RPCs. Each plane is readout with 120 pads with grounded guard electrodes between them to minimize the crosstalk noise. The main performances of the detectors are: an arrival time resolution of about ~300 ps, a tracking angular resolution below 3°, a detection efficiency close to 1, and a solid angle acceptance of ~5 srad. Another two planes of RPC detectors will be added in the next future in order to improve both the resolutions and the acceptance. TRAGALDABAS will be able to monitor the cosmic ray low energy component strongly modulated by solar activity. Its cadence and its angular resolution will allow to study in detail, small variations in cosmic ray anisotropy. These variations can be a key parameter to understand the effect of solar disturbances on the propagation of cosmic ray in the inner heliosphere and, maybe, provide a new tool for space weather analysis.