Piritakua: the atmosphere as a high-energy physics laboratory

The atmosphere provides a large set of experimental conditions on which cosmic-ray induced high-energy hadron interactions can take place. These conditions include: sudden changes in the atmospheric pressure, temperature, and in the local electric and magnetic fields. In this talk we introduce the Piritakua (flash of lightning, in the language of the pre-Columbian Purépecha Empire in Mexico) project, a cosmic-ray detector located at the Instituto de Física of UNAM, in Mexico City at 2280 m. a.s.l. The experiment consists of a small array of scintillator detectors, which use the electronics developed by the CosmicWatch project. The scintillators operate simultaneously with an electric field meter, a magnetometer, a meteorological station, and a hemispheric camera. We propose to use Piritakua to study the modification of the secondary particle production and propagation under sudden variations in the standard atmospheric properties. We present the current status and the first results of the experiment.

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Publication Details

Published
2025-09-23
DOI
https://doi.org/10.22323/1.501.0315
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
0.00

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article

Piritakua: the atmosphere as a high-energy physics laboratory

E. Belmont, H. León Vargas, A. Sandoval, A. Galván-Gaméz et al.
Astrophysics and Cosmic Phenomena
article

Piritakua: the atmosphere as a high-energy physics laboratory

E. Belmont, H. León Vargas, A. Sandoval, A. Galván-Gaméz, A. Gonzalez Muñoz, Cindy Castellón Salguero
article en

Abstract

The atmosphere provides a large set of experimental conditions on which cosmic-ray induced high-energy hadron interactions can take place. These conditions include: sudden changes in the atmospheric pressure, temperature, and in the local electric and magnetic fields. In this talk we introduce the Piritakua (flash of lightning, in the language of the pre-Columbian Purépecha Empire in Mexico) project, a cosmic-ray detector located at the Instituto de Física of UNAM, in Mexico City at 2280 m. a.s.l. The experiment consists of a small array of scintillator detectors, which use the electronics developed by the CosmicWatch project. The scintillators operate simultaneously with an electric field meter, a magnetometer, a meteorological station, and a hemispheric camera. We propose to use Piritakua to study the modification of the secondary particle production and propagation under sudden variations in the standard atmospheric properties. We present the current status and the first results of the experiment.

Consejo Nacional de Ciencia y Tecnología, Universidad Nacional Autónoma de México
Openalex Percentile: Top 89%
Astrophysics and Cosmic Phenomena
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