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Contributions of the LAGO Collaboration to the 36th ICRC

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arxiv 1909.10039 v1 pith:Y5F47WHB submitted 2019-09-22 hep-ex hep-ph

Contributions of the LAGO Collaboration to the 36th ICRC

classification hep-ex hep-ph
keywords lagoobservatorycollaborationcontributionscosmicicrclatinrays
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The LAGO (Latin American Giant Observatory) observatory is an experiment that spans over Latin America in a wide range of latitudes that gives different rigidity cut offs for the enter of cosmic rays in the atmosphere. The motivation of the Observatory is to study atmospheric radiation and space weather through the measurement of the secondary emission of low energy cosmic rays at ground level using Water Cherenkov Detectors (WCD). This work presents the contributions of the LAGO collaboration to the 2019 36th ICRC.

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