Latin American Giant Observatory: Contributions to the 34th International Cosmic Ray Conference (ICRC 2015)

LAGO; O. ARESO

Conferencia; 34th International Cosmic Ray Conference (ICRC 2015); 2015

The Latin American Giant Observatory (LAGO) is an extended cosmic rayobservatory composed by a network of water-Cherenkov detectors spanningover different sites located at significantly different altitudes (fromsea level up to more than $5000$\,m a.s.l.) and latitudes across LatinAmerica, covering a huge range of geomagnetic rigidity cut-offs andatmospheric absorption/reaction levels. This detection network isdesigned to measure the temporal evolution of the radiation flux atground level with extreme detail. The LAGO project is mainly oriented toperform basic research in three branches: high energy phenomena, spaceweather and atmospheric radiation at ground level. LAGO is built andoperated by the LAGO Collaboration, a non-centralized collaborativeunion of more than 30 institutions from ten countries. These are thecontributions of the LAGO Collaboration to the 34th International CosmicRay Conference