Resumen
We present the results of three years of continuous operations and the principal characteristics of our new 3 He 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 3 He neutron monitor, with the intention of replacing the older proportional tubes of the BF 3 . 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 BF 3 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.
| Idioma original | Inglés |
|---|---|
| Páginas (desde-hasta) | 1670-1683 |
| Número de páginas | 14 |
| Publicación | Advances in Space Research |
| Volumen | 49 |
| N.º | 12 |
| DOI | |
| Estado | Publicada - 15 jun 2012 |
Huella
Profundice en los temas de investigación de 'New 3 He neutron monitor for Chilean Cosmic-Ray Observatories from the Altiplanic zone to the Antarctic zone'. En conjunto forman una huella única.Citar esto
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