High-energy radiographic imaging performance of LYSO
Abstract
Here, a comprehensive comparison of the dominant sources of radiation-induced blur for radiographic imaging system performance is made. End-point energies of 6, 10, 15, and 20 MeV bremsstrahlung photon radiation produced at the Los Alamos National Laboratory Microtron facility were used to examine the performance of large-panel cerium-doped lutetium yttrium silicon oxide (LYSO:Ce) scintillators 3, 5 and 10 mm thick. The system resolution was measured and compared between the various end-point energies and scintillator thicknesses. Contrary to expectations, it is found that there was only a minor dependence of system resolution on scintillator thickness or beam end-point energy. This indicates that increased scintillator thickness does not have a dramatic effect on system performance. The data are then compared to Geant4 simulations to assess contributions to the system performance through the examination of modulation transfer functions. It was determined that the low-frequency response of the system is dominated by the radiation-induced signal, while the higher-frequency response of the system is dominated by the optical imaging of the scintillation emission.
- Authors:
-
[2];
[2];
[2];
- Nevada National Security Site (NNSS), New Mexico Operations, Los Alamos, NM (United States)
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Sandia National Lab. (SNL-NM), Albuquerque, NM (United States)
- Keystone International, Inc., Albuquerque, NM (United States)
- Publication Date:
- Research Org.:
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States); Sandia National Lab. (SNL-NM), Albuquerque, NM (United States)
- Sponsoring Org.:
- USDOE National Nuclear Security Administration (NNSA), Office of Defense Programs (DP) (NA-10); National Security Technologies, LLC, Las Vegas, NV (United States); Nevada National Security Site (NNSS), New Mexico Operations, Los Alamos, NM (United States). Mission Support and Test Services (MSTS)
- OSTI Identifier:
- 1441332
- Alternate Identifier(s):
- OSTI ID: 1457364
- Report Number(s):
- [LA-UR-18-20251; SAND-2018-1045J]
[Journal ID: ISSN 0168-9002; TRN: US1900906]
- Grant/Contract Number:
- [AC52-06NA25396; AC52-06NA25946; NA0003624; NA-0003525; AC04-94AL85000]
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment
- Additional Journal Information:
- [ Journal Volume: 914]; Journal ID: ISSN 0168-9002
- Publisher:
- Elsevier
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY; Radiography; Imaging; Blur
Citation Formats
Smalley, Duane, Duke, Dana, Webb, Timothy, Baker, Stuart, Castaneda, Jesus, Corredor, Andrew, Danielson, Jeremy, Gehring, Mandie, Haines, Todd, Lutz, Steve, Montoya, Kristina, and Stearns, John. High-energy radiographic imaging performance of LYSO. United States: N. p., 2018.
Web. doi:10.1016/j.nima.2018.05.044.
Smalley, Duane, Duke, Dana, Webb, Timothy, Baker, Stuart, Castaneda, Jesus, Corredor, Andrew, Danielson, Jeremy, Gehring, Mandie, Haines, Todd, Lutz, Steve, Montoya, Kristina, & Stearns, John. High-energy radiographic imaging performance of LYSO. United States. doi:10.1016/j.nima.2018.05.044.
Smalley, Duane, Duke, Dana, Webb, Timothy, Baker, Stuart, Castaneda, Jesus, Corredor, Andrew, Danielson, Jeremy, Gehring, Mandie, Haines, Todd, Lutz, Steve, Montoya, Kristina, and Stearns, John. Wed .
"High-energy radiographic imaging performance of LYSO". United States. doi:10.1016/j.nima.2018.05.044. https://www.osti.gov/servlets/purl/1441332.
@article{osti_1441332,
title = {High-energy radiographic imaging performance of LYSO},
author = {Smalley, Duane and Duke, Dana and Webb, Timothy and Baker, Stuart and Castaneda, Jesus and Corredor, Andrew and Danielson, Jeremy and Gehring, Mandie and Haines, Todd and Lutz, Steve and Montoya, Kristina and Stearns, John},
abstractNote = {Here, a comprehensive comparison of the dominant sources of radiation-induced blur for radiographic imaging system performance is made. End-point energies of 6, 10, 15, and 20 MeV bremsstrahlung photon radiation produced at the Los Alamos National Laboratory Microtron facility were used to examine the performance of large-panel cerium-doped lutetium yttrium silicon oxide (LYSO:Ce) scintillators 3, 5 and 10 mm thick. The system resolution was measured and compared between the various end-point energies and scintillator thicknesses. Contrary to expectations, it is found that there was only a minor dependence of system resolution on scintillator thickness or beam end-point energy. This indicates that increased scintillator thickness does not have a dramatic effect on system performance. The data are then compared to Geant4 simulations to assess contributions to the system performance through the examination of modulation transfer functions. It was determined that the low-frequency response of the system is dominated by the radiation-induced signal, while the higher-frequency response of the system is dominated by the optical imaging of the scintillation emission.},
doi = {10.1016/j.nima.2018.05.044},
journal = {Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment},
number = ,
volume = [914],
place = {United States},
year = {2018},
month = {5}
}
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