The Astroparticle Detectors Array—An Educational Project in Cosmic Ray Physics

Author:

Arcani Marco1ORCID,Conte Elio2,Monte Omar Del3ORCID,Frassati Alessandra4,Grana Andrea5ORCID,Guaita Cesare6,Liguori Domenico7,Nemolato Altea Renata Maria8,Pigato Daniele9,Rubino Elia10

Affiliation:

1. Astroparticle Detectors Array Lab–GAT Astronomical Center, 21040 Tradate, Italy

2. Laboratory of Nuclear Physics, School of Advanced International Studies on Applied Theoretical and Non Linear Methodologies of Physics, 70121 Bari, Italy

3. VVF, Corpo Nazionale dei Vigili del Fuoco, 14100 Asti, Italy

4. OABi Osservatorio Astronomico & Astrofisico Biellese, Biella–Università degli Studi di Padova, 35122 Padova, Italy

5. Lycée “Ermesinde”, L-7590 Mersch, Luxembourg

6. GAT Tradate–Planetarium “Ulrico Hoepli”, 20121 Milano, Italy

7. IIS Liceo Scientifico “Patrizi”, 87062 Cariati, Italy

8. Dipartimento di Scienze e Tecnologie Ambientali, Biologiche eFarmaceutiche, Università Degli Studi Della Campania “Luigi Vanvitelli”, 81100 Caserta, Italy

9. OABi Osservatorio Astronomico & Astrofisico Biellese, 13900 Biella, Italy

10. Associazione Arma Aeronautica, 81100 Caserta, Italy

Abstract

ADA, short for Astroparticle Detectors Array, is an educational project aiming to detect cosmic radiation and possibly high-energy particles known as ultra-high-energy cosmic rays (UHECRs) or even to spot a supernova event. Its working process is the same as that used in professional cosmic ray observatories: it consists of simple detectors spread over the entire Italian territory and beyond. The detectors are hosted among high schools, associations, and private astronomical observatories. ADA has been operating since 2013 and was brought about with the intention of promoting astroparticle physics to any given level of outreach. Furthermore, ADA is becoming an interesting tool not only for teachers but also for independent and keen scientists. Over the years, we have discovered the importance of having a long series of data for studying the relation between and among cosmic rays, weather, and space weather and to investigate the main cause of oscillations in cosmic ray data. In this paper, we show what we find to be the most compelling results, such as the beautiful symmetry of the behavior between muons and the atmospheric temperature and, likewise, the evident anti-correlation between the intensity of the muons at ground level compared with solar activity.

Publisher

MDPI AG

Subject

Physics and Astronomy (miscellaneous),General Mathematics,Chemistry (miscellaneous),Computer Science (miscellaneous)

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