New He neutron monitor for Chilean Cosmic-Ray Observatories from the Altiplanic zone to the Antarctic zone |
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Authors: | EG Cordaro E Olivares D Galvez D Salazar-Aravena D Laroze |
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Institution: | 1. Observatorios de Radiación Cósmica, Universidad de Chile, Casilla 487-3, Santiago, Chile;2. Escuela de Ingeniería Electrónica, Facultad de Ingeniería, Universidad Mayor, Av. Manuel Montt 367, Santiago, Chile;3. Departamento de Física, Universidad de Santiago de Chile, Av. Ecuador 3493, Santiago, Chile;4. Max Planck Institute for Polymer Research, D 55021 Mainz, Germany;5. Instituto de Alta Investigación, Universidad de Tarapacá, Casilla 7D, Arica, Chile |
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Abstract: | We present the results of three years of continuous operations and the principal characteristics of our new 3He neutron monitors installed in the Chilean Network of Cosmic-Ray Observatories. During the years 2004 and 2005, we began the construction of this International Geophysical Year (IGY)-type 3He neutron monitor, with the intention of replacing the older proportional tubes of the BF3. These new monitors are installed in stations at locations ranging from the near-equatorial zone to the Antarctic zone. As a reference system, we used our own BF3 neutron monitors and previously complemented the collected data with a Monte Carlo simulation for the proton-yield function response of the Putre neutron monitor. Herein, we present for the first time the data obtained from our new high-mountain observatory located in the Altiplanic zone. |
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Keywords: | 3He neutron monitor High mountain observatories Ground level event Monte Carlo method |
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