ÚTEFČVUT Ústav technické a experimentální fyziky ČVUT v PrazeInstitute of Experimental and Applied Physics, CTU in Prague

Wide energy range gamma-ray calibration facility

NázevTitle
Wide energy range gamma-ray calibration facilityWide energy range gamma-ray calibration facility
Druh výsledkuResult type
Příspěvek ve sborníkuProceedings paper
AutořiAuthors
M. Kroupa, Z. Janout, M. Králík, F. Krejčí, A. Owens, S. Pospíšil, F. Quarati, J. Šolc
Klíčová slovaKeywords
detector calibration, Gamma spectroscopy, prompt gamma-rays, thermal neutron capture, European Space Agency (ESA), cosmic space applications
KonferenceConference
2010 IEEE Nuclear Science Symposium, Medical Imaging Conference, and 17th Room Temperature Semiconductor Detectors Workshop (Knoxville, United States, 2010-10-30)
DOIDOI
10.1109/NSSMIC.2010.5873779
Časopis / citaceJournal / citation
In: IEEE Nuclear Science Symposuim & Medical Imaging Conference, IEEE, 2010, pp. 352-356 · ISSN 1095-7863
RokYear
2010
JazykLanguage
eng
ZáznamyRecords
ProjektProject
Laboratory Wide Dynamic Range Gamma Ray Calibration FacilityLaboratory Wide Dynamic Range Gamma Ray Calibration Facility; Institucionální podpora na rozvoj výzkumné org.Institucionální podpora na rozvoj výzkumné org.
CitovánoCited by
1 (OpenAlex)
2013: 1
Citace ke staženíDownload citation
TXT · BibTeX

AbstraktAbstract

A number of radiation-related applications in space such as γ-ray detection demands a flexible and wide-range γ-ray source which can serve as calibrating and testing facility for γ-ray detectors and γ-ray sensitive devices. A dedicated wide energy range γ-ray facility with adjustable and modular segments designed for γ-ray detector calibration and testing was built. Gamma rays are obtained from thermal neutron capture, which is the most suitable and cost efficient way how to provide discrete γ rays with energy above 3 MeV and of reasonable intensity. With appropriate and interchangeable targets the facility can generate γ rays with energy up to 10 MeV. Target materials of elements with high thermal neutron capture cross-section such as chrome, iron, chlorine, nickel and titanium provide suitable spectra. As neutron source 252Cf or 241Am-Be radionuclide sources with emission rate around 106 neutrons/s are used. The emitted fast neutrons are moderated by a modular interchangeable system of elements containing light materials such as graphite, water, heavy water or paraffin. Different geometries and moderator-target combinations have been tested and optimized; the best of them are presented. The facility is optimized with respect to space applications and needs by the European Space Agency (ESA). Performance of the facility is demonstrated by calibration spectra measured by HPGe and scintillator detectors (LaBr3, NaI(Tl)).

A number of radiation-related applications in space such as γ-ray detection demands a flexible and wide-range γ-ray source which can serve as calibrating and testing facility for γ-ray detectors and γ-ray sensitive devices. A dedicated wide energy range γ-ray facility with adjustable and modular segments designed for γ-ray detector calibration and testing was built. Gamma rays are obtained from thermal neutron capture, which is the most suitable and cost efficient way how to provide discrete γ rays with energy above 3 MeV and of reasonable intensity. With appropriate and interchangeable targets the facility can generate γ rays with energy up to 10 MeV. Target materials of elements with high thermal neutron capture cross-section such as chrome, iron, chlorine, nickel and titanium provide suitable spectra. As neutron source 252Cf or 241Am-Be radionuclide sources with emission rate around 106 neutrons/s are used. The emitted fast neutrons are moderated by a modular interchangeable system of elements containing light materials such as graphite, water, heavy water or paraffin. Different geometries and moderator-target combinations have been tested and optimized; the best of them are presented. The facility is optimized with respect to space applications and needs by the European Space Agency (ESA). Performance of the facility is demonstrated by calibration spectra measured by HPGe and scintillator detectors (LaBr3, NaI(Tl)).

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