Radon contribution to single particle counts of the ARGO-YBJ detector
Creators
- 1. Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, Complesso Universitario di Monte Sant'Angelo, via Cinthia, 80126 Napoli (Italy)
- 2. Dipartimento di Fisica dell'Università di Napoli "Federico II", Complesso Universitario di Monte Sant'Angelo, via Cinthia, 80126 Napoli (Italy)
- 3. Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, via per Arnesano, 73100 Lecce (Italy)
- 4. Dipartimento di Matematica e Fisica "Ennio De Giorgi", Università del Salento, via per Arnesano, 73100 Lecce (Italy)
- 5. Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Science, P.O. Box 918, 100049 Beijing (China)
- 6. Istituto Nazionale di Fisica Nucleare, Sezione di Pavia, via Bassi 6, 27100 Pavia (Italy)
- 7. Dipartimento di Fisica dell' Università degli Studi di Pavia, via Bassi 6, 27100 Pavia (Italy)
- 8. Istituto Nazionale di Fisica Nucleare, Sezione di Roma3, via della Vasca Navale 84, 00146 Roma (Italy)
- 9. Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tor Vergata, via della Ricerca Scientifica 1, 00133 Roma (Italy)
- 10. Dipartimento di Fisica dell'Università di Roma "Tor Vergata", via della Ricerca Scientifica 1, 00133 Roma (Italy)
Description
The ARGO-YBJ experiment is an air shower detector for gamma ray astronomy and cosmic ray studies with an energy threshold of ∼500 GeV. Working in "single particle mode", i.e. counting the single particles hitting the detector at fixed time intervals, ARGO-YBJ can monitor cosmic ray and gamma ray transients at energies of a few GeV. The single particle counting rate is modulated by the atmospheric pressure and temperature, and is affected by the local radioactivity from soil and air. Among the radioactive elements, radon gas is of particular importance since its concentration in air can vary significantly, according to environmental conditions. In this paper we evaluate the contribution of the radon daughter gamma ray emitters to the single particle counting rate measured by ARGO-YBJ. According to our analysis, the radon gas contribution is roughly 1–2%, producing a counting rate modulation of the same order of magnitude of the atmospheric effects. - Highlights: • The ARGO-YBJ experiment is an air shower detector for gamma ray astronomy of very large area. • The ARGO-YBJ detector can work into two modes: single particle mode and shower mode. • The work shows how natural radioactivity can influence the single particle counting. • The paper shows how to evidence (and correct) the radon influence on the detector counting
Availability note (English)
Available from http://dx.doi.org/10.1016/j.radmeas.2014.07.006Additional details
Identifiers
- DOI
- 10.1016/j.radmeas.2014.07.006;
- PII
- S1350-4487(14)00209-1;
Publishing Information
- Journal Title
- Radiation Measurements
- Journal Volume
- 68
- Journal Page Range
- p. 42-48
- ISSN
- 1350-4487
- CODEN
- RMEAEP
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 46127876
- Subject category
- S61: RADIATION PROTECTION AND DOSIMETRY;
- Descriptors DEI
- AIR; ATMOSPHERIC PRESSURE; COUNTING RATES; EXTENSIVE AIR SHOWERS; GAMMA ASTRONOMY; GAMMA RADIATION; NATURAL RADIOACTIVITY; RADON; SINGLE-PARTICLE MODES; SOILS
- Descriptors DEC
- ASTRONOMY; COSMIC RADIATION; COSMIC SHOWERS; ELECTROMAGNETIC RADIATION; ELEMENTS; FLUIDS; GASES; IONIZING RADIATIONS; NONMETALS; OSCILLATION MODES; RADIATIONS; RADIOACTIVITY; RARE GASES; SECONDARY COSMIC RADIATION; SHOWERS
Optional Information
- Copyright
- Copyright (c) 2014 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.