Abstract
Detector characteristics are investigated for solar neutron detection at cosmic stations. It is shown that usage of the identification method by the shape of scintillation flash is CsI(Tl) provides for reliable discrimination of neutron and {gamma}-quanta in the studied energy range. Estimations are obtained for the identification efficiency of secondary protons and electrons in 13,5-80 MeV. The spectrum of isotopic composition of the products of neutron interaction with Cs and nuclei is estimated. Dependences are calculated of the neutron detection efficiency on the identification circuit threshold for space conditions. 14 refs.; 8 figs.; 1 tab.
Citation Formats
Antipov, A V, Belogorlov, E A, Bogomolov, A V, Britvich, G I, Kuptsov, S I, Lupenko, G V, Myagkova, I N, Ryumin, S P, and Chumakov, A A.
Detection of 40-2000 MeV neutrons at the intensive gamma-ray background by means of a CsJ(Tl)-detector during the synchrotron U-70 experiment; Registratsiya nejtronov s ehnergiyami 40-2000 MehV na intensivnom fone {gamma}-kvantov s pomoshch`yu CsJ(Tl) v ehksperimente na sinkhrofazotrone U-70.
Russian Federation: N. p.,
1992.
Web.
Antipov, A V, Belogorlov, E A, Bogomolov, A V, Britvich, G I, Kuptsov, S I, Lupenko, G V, Myagkova, I N, Ryumin, S P, & Chumakov, A A.
Detection of 40-2000 MeV neutrons at the intensive gamma-ray background by means of a CsJ(Tl)-detector during the synchrotron U-70 experiment; Registratsiya nejtronov s ehnergiyami 40-2000 MehV na intensivnom fone {gamma}-kvantov s pomoshch`yu CsJ(Tl) v ehksperimente na sinkhrofazotrone U-70.
Russian Federation.
Antipov, A V, Belogorlov, E A, Bogomolov, A V, Britvich, G I, Kuptsov, S I, Lupenko, G V, Myagkova, I N, Ryumin, S P, and Chumakov, A A.
1992.
"Detection of 40-2000 MeV neutrons at the intensive gamma-ray background by means of a CsJ(Tl)-detector during the synchrotron U-70 experiment; Registratsiya nejtronov s ehnergiyami 40-2000 MehV na intensivnom fone {gamma}-kvantov s pomoshch`yu CsJ(Tl) v ehksperimente na sinkhrofazotrone U-70."
Russian Federation.
@misc{etde_10113090,
title = {Detection of 40-2000 MeV neutrons at the intensive gamma-ray background by means of a CsJ(Tl)-detector during the synchrotron U-70 experiment; Registratsiya nejtronov s ehnergiyami 40-2000 MehV na intensivnom fone {gamma}-kvantov s pomoshch`yu CsJ(Tl) v ehksperimente na sinkhrofazotrone U-70}
author = {Antipov, A V, Belogorlov, E A, Bogomolov, A V, Britvich, G I, Kuptsov, S I, Lupenko, G V, Myagkova, I N, Ryumin, S P, and Chumakov, A A}
abstractNote = {Detector characteristics are investigated for solar neutron detection at cosmic stations. It is shown that usage of the identification method by the shape of scintillation flash is CsI(Tl) provides for reliable discrimination of neutron and {gamma}-quanta in the studied energy range. Estimations are obtained for the identification efficiency of secondary protons and electrons in 13,5-80 MeV. The spectrum of isotopic composition of the products of neutron interaction with Cs and nuclei is estimated. Dependences are calculated of the neutron detection efficiency on the identification circuit threshold for space conditions. 14 refs.; 8 figs.; 1 tab.}
place = {Russian Federation}
year = {1992}
month = {Dec}
}
title = {Detection of 40-2000 MeV neutrons at the intensive gamma-ray background by means of a CsJ(Tl)-detector during the synchrotron U-70 experiment; Registratsiya nejtronov s ehnergiyami 40-2000 MehV na intensivnom fone {gamma}-kvantov s pomoshch`yu CsJ(Tl) v ehksperimente na sinkhrofazotrone U-70}
author = {Antipov, A V, Belogorlov, E A, Bogomolov, A V, Britvich, G I, Kuptsov, S I, Lupenko, G V, Myagkova, I N, Ryumin, S P, and Chumakov, A A}
abstractNote = {Detector characteristics are investigated for solar neutron detection at cosmic stations. It is shown that usage of the identification method by the shape of scintillation flash is CsI(Tl) provides for reliable discrimination of neutron and {gamma}-quanta in the studied energy range. Estimations are obtained for the identification efficiency of secondary protons and electrons in 13,5-80 MeV. The spectrum of isotopic composition of the products of neutron interaction with Cs and nuclei is estimated. Dependences are calculated of the neutron detection efficiency on the identification circuit threshold for space conditions. 14 refs.; 8 figs.; 1 tab.}
place = {Russian Federation}
year = {1992}
month = {Dec}
}