At the Testa Grigia high altitude research Station (3480 m. a.s.l, Italy, 45◦57′ N, 7◦42’ E) several dosimetric campaigns for the measurement of the dose due to secondary neutrons produced in the atmosphere and in the surrounding environment by primary cosmic rays have been carried out from 2014 until 2021. Because of the high altitude of the site, the neutron flux at Testa Grigia is 10–15 times higher than at the sea level. Various instruments has been used to evaluate the dependence of the ambient dose equivalent rate from different factors as atmospheric parameters, environmental conditions and solar activity. Moreover, since October 2014 a modular neutron monitor designed, realized and tested by the SVIRCO Observatory Group INAF-IAPS in Rome, is permanently operating in the laboratory, providing a continuous monitoring of primary cosmic ray variability and making the laboratory an ideal place for dosimetric studies, instrument calibration and “in field” tests. In this paper the results of several neutron measurements carried out in the last years in periods of different solar ac- tivity and environmental conditions are reported, with a discussion on the origin of the observed variations of the ambient dose equivalent rate.

Long term measurements of neutron dose rates at Testa Grigia high altitude research station (3480 m. a.s.l.)

Cirilli, S.
2022-01-01

Abstract

At the Testa Grigia high altitude research Station (3480 m. a.s.l, Italy, 45◦57′ N, 7◦42’ E) several dosimetric campaigns for the measurement of the dose due to secondary neutrons produced in the atmosphere and in the surrounding environment by primary cosmic rays have been carried out from 2014 until 2021. Because of the high altitude of the site, the neutron flux at Testa Grigia is 10–15 times higher than at the sea level. Various instruments has been used to evaluate the dependence of the ambient dose equivalent rate from different factors as atmospheric parameters, environmental conditions and solar activity. Moreover, since October 2014 a modular neutron monitor designed, realized and tested by the SVIRCO Observatory Group INAF-IAPS in Rome, is permanently operating in the laboratory, providing a continuous monitoring of primary cosmic ray variability and making the laboratory an ideal place for dosimetric studies, instrument calibration and “in field” tests. In this paper the results of several neutron measurements carried out in the last years in periods of different solar ac- tivity and environmental conditions are reported, with a discussion on the origin of the observed variations of the ambient dose equivalent rate.
File in questo prodotto:
File Dimensione Formato  
1-s2.0-S0969806X22000147-main.pdf

Accesso chiuso

Tipologia: Documento in Versione Editoriale
Licenza: Copyright Editore
Dimensione 5.39 MB
Formato Adobe PDF
5.39 MB Adobe PDF   Visualizza/Apri   Richiedi una copia
1-s2.0-S0969806X22000147-main-Post_print.pdf

Open Access dal 15/01/2024

Tipologia: Bozza finale post-referaggio (post-print)
Licenza: Creative commons
Dimensione 5.8 MB
Formato Adobe PDF
5.8 MB Adobe PDF Visualizza/Apri
Pubblicazioni consigliate

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11368/3007916
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 4
  • ???jsp.display-item.citation.isi??? 4
social impact