GARZÓN, J.A.; COLLAZO, J.; CUENCA-GARCÍA, J.; GARCÍA CASTRO, D.; OTERO, J.; YERMO, M.; BLANCO, J.J.; KURTUKIAN, T.; MOROZOVA, A.; PAIS, M.A.; BLANCO, A.; FONTE, P.; LOPES, L.; KORNAKOV, G.; ÁLVAREZ-POL, H.; CABANELAS, P.; PAZOS, A.; SECO, M.; RIÁDIGOS, I.; PÉREZ MUÑUZURI, V.; GÓMEZ-TATO, A.; MOURIÑO, J.C.; REY, P.; TABOADA, J.

Métadonnées

Afficher la notice complète

Licence d’utilisation du document

Langue

Communication dans un congrès

Ce document a été publié dans

2016-09-04, Turin.

Résumé en anglais

Cosmic rays originating from extraterrestrial sources are permanently arriving at Earth atmosphere, where they produce up to billions of secondary particles. The analysis of the secondary particles reaching to the surface of the Earth may provide a very valuable information about the Sun activity, changes in the geomagnetic field and the atmosphere, among others. In this article, we present the first preliminary results of the analysis of the cosmic rays measured with a high resolution tracking detector, TRAGALDABAS, located at the Univ. of Santiago de Compostela, in Spain.< Réduire

Mots clés en anglais

tracking detector: resolution

cosmic radiation

atmosphere

magnetic field

surface

solar

particle

secondary

Origine

Importé de hal

Unités de recherche

Centre d'Études Nucléaires de Bordeaux Gradignan (CENBG)