The Flows of Neutrons of Spase Radiation and from Terrestrial Crust

Details The Flows of Neutrons of Spase Radiation and from Terrestrial Crust The Flows of Neutrons of Spase Radiation and from Terrestrial Crust

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc...10.4204v&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The experimental researches at North of Tien Shan were carried out at height 3340 m above a sea level (Zhusalykesen' pass, high-level scientific station of the Physical Institute RAS) in August and December, 1999. The fluxes of neutrons and alfa-particles have been measured. The data of the neutron monitor and the counters of charged particles, that have been locating there too, were attracted also. The data set has allowed to estimate a share of thermal and slow neutrons, caused by processes in terrestrial crust, into a total neutron background. Dynamics of the neutron fluxes, connected with the tide forces in terrestrial crust during the complete solar eclipse in August 11, 1999 and the new moon in December 7, 1999, also have been observed. The contribution of neutrons from terrestrial crust was then not less 10% from a total neutron background. The flux of alfa-particles which form the additional flux of neutrons had the top limit 0.12±0.08 min-1 sm-2 . The experiment has confirmed, that one of the reasons for appearance of the additional neutrons can be the gravitational influence on the Earth of the Moon and the Sun.

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