Next generation of scintillation detector based on cerium bromide crystal for space application in the gamma-ray spectrometer of the Mercurian gamma-ray and neutron spectrometer

A. S. Kozyrev; I. G. Mitrofanov; J. Benkhoff; A. Owens; F. Quarati; M. L. Litvak; A. V. Malakhov; M. I. Mokrousov; G. N. Timoshenko; V. N. Shvetsov

doi:10.1134/S0020441216030192

Next generation of scintillation detector based on cerium bromide crystal for space application in the gamma-ray spectrometer of the Mercurian gamma-ray and neutron spectrometer

Авторлар: Kozyrev A.S.¹, Mitrofanov I.G.¹, Benkhoff J.², Owens A.², Quarati F.³, Litvak M.L.¹, Malakhov A.V.¹, Mokrousov M.I.¹, Timoshenko G.N.⁴, Shvetsov V.N.⁴
Мекемелер:
1. Space Research Institute
2. SRE-PA
3. Delft University of Technology
4. Joint Institute for Nuclear Research
Шығарылым: Том 59, № 4 (2016)
Беттер: 569-577
Бөлім: Physical Instruments for Ecology, Medicine, and Biology
URL: https://bakhtiniada.ru/0020-4412/article/view/159201
DOI: https://doi.org/10.1134/S0020441216030192
ID: 159201

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A brief description is presented of the γ-ray spectrometer part of the Mercurian gamma-ray and neutron spectrometer (MGNS), the scientific instrument for planetary research on mapping of γ-ray and neutron emission from the Mercury surface onboard BepiColombo spacecraft of the European Space Agency (ESA) spacecraft. As the crystal for the γ-ray spectrometer, an innovative CeBr₃ scintillator was chosen on the basis of the ground tests and analysis of the results reported in this paper.