Piritakua: the atmosphere as a high-energy physics laboratory
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 FÃsica 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.
Hermes León Vargas、Antonio Galván、Andrés Sandoval、Ernesto Belmont、Cindy Castellón Salguero、Adiv González Muñoz
大气科学(气象学)天文学
Hermes León Vargas,Antonio Galván,Andrés Sandoval,Ernesto Belmont,Cindy Castellón Salguero,Adiv González Muñoz.Piritakua: the atmosphere as a high-energy physics laboratory[EB/OL].(2025-07-28)[2025-08-11].https://arxiv.org/abs/2507.21373.点此复制
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