W. Alvarez
- Astrophysics and Cosmic Phenomena
- Dark Matter and Cosmic Phenomena
- Neutrino Physics Research
- Radio Astronomy Observations and Technology
- Smart Grid Security and Resilience
- Optimal Power Flow Distribution
- Particle Detector Development and Performance
- Microgrid Control and Optimization
- Color Science and Applications
- Gamma-ray bursts and supernovae
- Particle physics theoretical and experimental studies
University of San Carlos of Guatemala
2016-2017
John Wiley & Sons (United States)
2012
The Latin American Giant Observatory (LAGO) is an extended cosmic ray observatory composed by a network of water-Cherenkov detectors spanning over different sites located at significantly altitudes (from sea level up to more than $5000$\,m a.s.l.) and latitudes across America, covering huge range geomagnetic rigidity cut-offs atmospheric absorption/reaction levels. This detection designed measure the temporal evolution radiation flux ground with extreme detail. LAGO project mainly oriented...
The Latin American Giant Observatory (LAGO) is an extended cosmic ray observatory composed by a network of water-Cherenkov detectors spanning over different sites located at significantly altitudes (from sea level up to more than 5000\,m a.s.l.) and latitudes across America, covering huge range geomagnetic rigidity cut-offs atmospheric absorption/reaction levels. This detection designed measure the temporal evolution radiation flux ground with extreme detail. LAGO project mainly oriented...
The LAGO (Latin American Giant Observatory) observatory is an experiment that spans over Latin America in a wide range of latitudes gives different rigidity cut offs for the enter cosmic rays atmosphere. motivation Observatory to study atmospheric radiation and space weather through measurement secondary emission low energy at ground level using Water Cherenkov Detectors (WCD). This work presents contributions collaboration 2019 36th ICRC.