Abstract
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.
| Original language | English |
|---|---|
| Pages (from-to) | 1670-1683 |
| Number of pages | 14 |
| Journal | Advances in Space Research |
| Volume | 49 |
| Issue number | 12 |
| DOIs | |
| State | Published - 15 Jun 2012 |
Keywords
- Ground level event
- High mountain observatories
- Monte Carlo method
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