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Title: DIFFERENTIAL SPECTRUM OF NEUTRONS AT CHACALTAYA-BOLIVIA

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3141372· OSTI ID:21308654
 [1];  [2]; ;  [3]
  1. Carrera de Fisica, Universidad Mayor de San Andres, La Paz-Bolivia (Bolivia, Plurinational State of)
  2. Instituto Nazionale di Fisica Nucleare Sez. Torino Via P. Giuria n. 10125, Torino (Italy)
  3. Instituto de Investigaciones Fisicas, UMSA, La Paz-Bolivia (Bolivia, Plurinational State of)

We describe the Neutron Spectrometer Experiment installed at Chacaltaya Cosmic Rays Observatory (68 deg. O, 16.2 deg. S), located in Bolivia, at 5230 m.a.s.l. This experimental system is constituted by passive detectors which register the flux of neutrons, in an energy range of 10 KeV-20 MeV. Using the unfolding code BUNTO a peak around 1 MeV of the characteristic spectrum of neutrons was obtained. Experimental values, observed during April of 2008, are compared with similar ones carried out in 1997 at the same place, in order to look for eventual changes due to local atmosphere. A similar experiment was also carried up at the Laboratory of Testa Grigia-Italy (45.56 deg. N, 7.42 deg. E,. 3480 m.a.l.s). Data of both stations allow us to compare the spectra in order to explain the difference of neutron flux of these two stations.

OSTI ID:
21308654
Journal Information:
AIP Conference Proceedings, Vol. 1123, Issue 1; Conference: 3. school on cosmic rays and astrophysics, Arequipa (Peru), 25 Aug - 5 Sep 2008; Other Information: DOI: 10.1063/1.3141372; (c) 2009 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
Country of Publication:
United States
Language:
English