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Coronary segmentation based motion corrected cardiac CT reconstruction 基于冠状动脉分割的运动校正心脏CT重建
Pub Date : 2010-12-01 DOI: 10.1109/NSSMIC.2010.5874132
A. Isola, C. Metz, M. Schaap, S. Klein, W. Niessen, M. Grass
A method to obtain motion artifact-free reconstructed images of the coronary arteries is proposed and evaluated. The method relies on the integration of coronary motion estimation in an iterative computed tomography reconstruction technique. Coronary motion fields are derived from a set of coronary centerlines extracted at multiple cardiac phases within the R-R interval. Start and end points are provided by the user in one time-frame only. Corresponding centerline positions are used to determine the motion fields from phase to phase. Finally, dense motion fields are achieved by thin-plate-spline interpolation and are used to perform a motion-corrected iterative reconstruction of a selected region of interest, which results in an effective improvement of the reconstructed image quality.
提出并评价了一种获取无运动伪影的冠状动脉重建图像的方法。该方法依赖于迭代计算机断层扫描重建技术中冠状动脉运动估计的集成。冠状动脉运动场来源于在R-R间期内多个心脏相提取的一组冠状动脉中心线。起始点和结束点仅由用户在一个时间范围内提供。相应的中心线位置用于确定各相位的运动场。最后,通过薄板样条插值获得密集运动场,并对选定的感兴趣区域进行运动校正迭代重建,有效地提高了重建图像的质量。
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引用次数: 7
Clock distribution and synchronization over 1000BASE-T Ethernet 通过1000BASE-T以太网进行时钟分配和同步
Pub Date : 2010-12-01 DOI: 10.1109/NSSMIC.2010.5874287
J. Imrek, G. Hegyesi, G. Kalinka, J. Molnár, F. Nagy
We report on a Synchronous Ethernet based clock distribution and timestamp synchronization implementation over 1000BASE-T (Gigabit over twisted pair) Ethernet. A central 125 MHz global clock is distributed to all detector modules using only commercial off-the-shelf components. The timestamps generated on different modules has a maximum fixed offset of 24–60 ns (depending on the switch tested), and a jitter of less than 500 ps (with no clock cleaner IC being used).
我们报告了在1000BASE-T(千兆双绞线)以太网上基于同步以太网的时钟分布和时间戳同步实现。中央125 MHz全局时钟仅使用商用现成组件分配到所有检测器模块。在不同模块上生成的时间戳具有24-60 ns的最大固定偏移(取决于测试的开关),以及小于500 ps的抖动(没有使用时钟清洁器IC)。
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引用次数: 2
A thermal-neutron detector with a phoswich system of LiCaAlF6 and BGO crystal scintillators onboard PoGOLite 在PoGOLite上采用LiCaAlF6和BGO晶体闪烁体的光导系统的热中子探测器
Pub Date : 2010-12-01 DOI: 10.1109/NSSMIC.2010.5873712
H. Takahashi, M. Yonetani, M. Matsuoka, T. Mizuno, Y. Fukazawa, T. Yanagida, Y. Fujimoto, Y. Yokota, A. Yoshikawa, N. Kawaguchi, S. Ishizu, K. Fukuda, T. Suyama, K. Watanabe, H. Tajima, Y. Kanai, N. Kawai, J. Kataoka, J. Katsuta, T. Takahashi, S. Gunji, M. Axelsson, M. Jackson, M. Kiss, W. Klamra, M. Kole, S. Larsson, P. Mallol, M. Pearce, F. Ryde, S. Rydstrom, G. Olofsson, H. Floren, T. Kamae, G. Madejski, G. Varner
To measure the flux of atmospheric neutrons and study the neutron contribution to the background of the main detector of the PoGOLite (Polarized Gamma-ray Observer) balloon-borne experiment, a thermal-neutron detector with a phoswich system of LiCaAlF6 (Eu) and BGO crystal scintillators is developed. The performance to separate thermal-neutron events from those of gamma-rays and charged particles is validated with 252Cf on ground. The detector is attached to the PoGOLite instrument and is launched in 2011 from the Esrange facility in the North of Sweden. Although the emission wavelength of the LiCaAlF6 (Ce) is ∼ 300 nm and overlaps with the absorption wavelength of the BGO, the phoswich capability of the LiCaAlF6 (Ce) with the BGO is also confirmed with installing a waveform shifter.
为了测量大气中子通量,研究极化伽玛射线观测者(PoGOLite)气球载实验主探测器的中子对背景的贡献,研制了一种由LiCaAlF6 (Eu)和BGO晶体闪烁体组成的热中子探测器。在地面上用252Cf验证了热中子事件与伽马射线和带电粒子分离的性能。该探测器与PoGOLite仪器相连,于2011年从瑞典北部的Esrange设施发射。虽然LiCaAlF6 (Ce)的发射波长为~ 300 nm,并且与BGO的吸收波长重叠,但通过安装波形移位器也证实了LiCaAlF6 (Ce)与BGO的光交换能力。
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引用次数: 11
Applying the neutron scatter camera to treaty verification and warhead monitoring 中子散射相机在条约核查和弹头监测中的应用
Pub Date : 2010-12-01 DOI: 10.1109/NSSMIC.2010.5873848
J. Brennan, R. Cooper, M. Gerling, P. Marleau, N. Mascarenhas, S. Mrowka
The neutron scatter camera was originally developed for a range of SNM detection applications. We are now exploring the feasibility of applications in treaty verification and warhead monitoring using experimentation, maximum likelihood estimation method (MLEM), detector optimization, and MCNP-PoliMi simulations.
中子散射相机最初是为一系列SNM检测应用而开发的。我们现在正在利用实验、最大似然估计方法(MLEM)、探测器优化和MCNP-PoliMi模拟探索条约核查和弹头监测应用的可行性。
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引用次数: 8
Comparative gamma spectroscopy with SrI2(Eu), GYGAG(Ce) and Bi-loaded plastic scintillators SrI2(Eu), GYGAG(Ce)和bi负载塑料闪烁体的比较伽马能谱
Pub Date : 2010-11-19 DOI: 10.1109/NSSMIC.2010.5873975
N. Cherepy, S. Payne, B. Sturm, J. Kuntz, Z. Seeley, B. L. Rupert, R. Sanner, O. Drury, T. A. Hurst, S. Fisher, M. Groza, L. Matei, A. Burger, K. Shah, L. Boatner, R. Hawrami
We are developing new scintillator materials that offer potential for high resolution gamma ray spectroscopy at low cost. Single crystal SrI2(Eu) offers ∼3% resolution at 662 keV, in sizes of ∼1 in3. We have developed ceramics processing technology allowing us to achieve cubic inch scale transparent ceramic scintillators offering gamma spectroscopy performance superior to NaI(Tl). Our bismuth-loaded plastic scintillator demonstrates energy resolution of ∼8% at 662 keV, for samples of ∼0.5 cm3.
我们正在开发新的闪烁体材料,以低成本提供高分辨率伽马射线光谱的潜力。单晶SrI2(Eu)在662 keV下提供~ 3%的分辨率,尺寸为~ 1 in3。我们已经开发了陶瓷加工技术,使我们能够实现立方英寸规模的透明陶瓷闪烁体,提供优于NaI(Tl)的伽马光谱性能。我们的铋负载塑料闪烁体在662 keV下的能量分辨率为~ 8%,样品为~ 0.5 cm3。
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引用次数: 48
Evaluation of large volume SrI2(Eu) scintillator detectors 大体积SrI2(Eu)闪烁体探测器的评价
Pub Date : 2010-11-18 DOI: 10.1109/NSSMIC.2010.5874047
B. Sturm, N. Cherepy, O. Drury, P. Thelin, S. Fisher, A. Magyar, S. Payne, A. Burger, L. Boatner, J. O. Ramey, K. Shah, R. Hawrami
There is an ever increasing demand for gamma-ray detectors which can achieve good energy resolution, high detection efficiency, and room-temperature operation. We are working to address each of these requirements through the development of large volume SrI2(Eu) scintillator detectors. In this work, we have evaluated a variety of SrI2 crystals with volumes >10 cm3. The goal of this research was to examine the causes of energy resolution degradation for larger detectors and to determine what can be done to mitigate these effects. Testing both packaged and unpackaged detectors, we have consistently achieved better resolution with the packaged detectors. Using a collimated gamma-ray source, it was determined that better energy resolution for the packaged detectors is correlated with better light collection uniformity. A number of packaged detectors were fabricated and tested and the best spectroscopic performance was achieved for a 3% Eu doped crystal with an energy resolution of 2.93% FWHM at 662keV. Simulations of SrI2(Eu) crystals were also performed to better understand the light transport physics in scintillators and are reported. This study has important implications for the development of SrI2(Eu) detectors for national security purposes.
对能量分辨率高、探测效率高、能在室温下工作的伽玛射线探测器的需求日益增长。我们正在努力通过开发大体积SrI2(Eu)闪烁体探测器来满足这些要求。在这项工作中,我们评估了各种体积为bbb10 cm3的SrI2晶体。这项研究的目的是检查大型探测器能量分辨率下降的原因,并确定可以做些什么来减轻这些影响。测试了封装和未封装的检测器,我们一致地使用封装检测器获得了更好的分辨率。使用准直伽玛射线源,确定了封装探测器的更好的能量分辨率与更好的光收集均匀性相关。制作并测试了多个封装的探测器,在662keV下,3% Eu掺杂晶体的能量分辨率为2.93% FWHM,获得了最佳的光谱性能。为了更好地理解闪烁体中的光输运物理,还对SrI2(Eu)晶体进行了模拟。该研究对用于国家安全目的的SrI2(Eu)探测器的开发具有重要意义。
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引用次数: 21
Probing the eV-Mass range for solar axions with CAST 用CAST探测太阳轴子的eV-Mass范围
Pub Date : 2010-11-11 DOI: 10.1109/NSSMIC.2010.5873777
J. Vogel, H. Brauninger, G. Cantatore, J. Carmona, S. Cetin, J. Collar, T. Dafni, M. Davenport, C. Eleftheriadis, N. Elias, C. Ezer, G. Fanourakis, E. Ferrer-Ribas, H. Fischer, J. Franz, P. Friedrich, J. Galán, A. Gardikiotis, E. Gazis, T. Geralis, I. Giomataris, S. Gninenko, H. Gómez, E. Gruber, T. Guthorl, R. Hartmann, F. Haug, M. Hasinoff, D. Hoffmann, F. Iguaz, I. Irastorza, J. Jacoby, K. Jakovčić, D. Kang, T. Karageorgopoulou, M. Karuza, K. Konigsmann, R. Kotthaus, M. Krčmar, K. Kousouris, M. Kuster, B. Lakić, P. Lang, C. Lasseur, J. Laurent, A. Liolios, A. Ljubičić, V. Lozza, G. Lutz, G. Luzón, D. Miller, A. Mirizzi, J. Morales, T. Niinikoski, A. Nordt, T. Papaevangelou, M. Pivovaroff, G. Raiteri, G. Raffelt, T. Rashba, H. Riege, A. Rodriguez, M. Roșu, J. Ruz, I. Savvidis, Y. Semertzidis, P. Serpico, P. Silva, S. Solanki, R. Soufli, L. Stewart, A. Tomás, M. Tsagri, K. Van Bibber, T. Vafeiadis, J. Villar, J. Vogel, L. Walckiers, Y. Wong, S. C. Yıldız, K. Zioutas
The CERN Axion Solar Telescope (CAST) is searching for solar axions which could be produced in the core of the Sun via the so-called Primakoff effect. Not only would these hypothetical particles solve the strong CP problem, but they are also one of the favored candidates for dark matter. In order to look for axions originating from the Sun, CAST uses a decommissioned LHC prototype magnet. In its 10 m long magnetic field region of 9 Tesla, axions could be reconverted into X-ray photons. Different X-ray detectors are installed on both ends of the magnet, which is mounted on a structure built to follow the Sun during sunrise and sunset for a total of about 3 hours per day. The analysis of the data acquired during the first phase of the experiment with vacuum in the magnetic field region yielded the most restrictive experimental upper limit on the axion-to-photon coupling constant for axion masses up to about 0.02 eV. In order to extend the sensitivity of the experiment to a wider mass range, the CAST experiment continues its search for axions with helium in the magnet bores. In this way it is possible to restore coherence of conversion for larger masses. Changing the pressure of the helium gas enables the experiment to scan different axion masses in the range of up to about 1.2 eV. Especially at high pressures, a precise knowledge of the gas density distribution is crucial to obtain accurate results. In the first part of this second phase of CAST, 4He was used and the axion mass region was extended up to 0.39 eV, a part of phase space favored by axion models. In CAST's ongoing 3He phase the studied mass range is now being extended further. In this contribution the final results of CAST's 4He phase will be presented and the current status of the 3He run will be given. This includes latest results as well as prospects of future axion experiments.
欧洲核子研究中心的轴子太阳望远镜(CAST)正在寻找通过所谓的Primakoff效应在太阳核心产生的太阳轴子。这些假设的粒子不仅可以解决强CP问题,而且它们也是暗物质的首选候选者之一。为了寻找来自太阳的轴子,CAST使用了一个退役的大型强子对撞机原型磁铁。在其10米长的9特斯拉磁场区,轴子可以重新转化为x射线光子。不同的x射线探测器安装在磁体的两端,磁体安装在一个结构上,在日出和日落时每天跟随太阳大约3小时。对实验第一阶段在磁场区真空条件下获得的数据进行分析,得到了轴子-光子耦合常数最严格的实验上限,即轴子质量约为0.02 eV。为了将实验的灵敏度扩展到更大的质量范围,CAST实验继续在磁体孔中寻找含氦的轴子。这样就有可能恢复较大质量的转换相干性。通过改变氦气的压力,实验可以在1.2 eV范围内扫描不同的轴子质量。特别是在高压下,精确了解气体密度分布对于获得准确的结果至关重要。在CAST第二阶段的第一部分中,使用了4He,轴子质量区域扩展到0.39 eV,这是轴子模型所青睐的相空间的一部分。在CAST正在进行的3He阶段,研究的质量范围正在进一步扩大。在这篇文章中,将介绍CAST的4He阶段的最终结果,并给出3He运行的当前状态。这包括最新的结果以及未来轴子实验的前景。
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引用次数: 0
Applications of nuclear resonance fluorescence 核共振荧光的应用
Pub Date : 2010-11-05 DOI: 10.1109/NSSMIC.2010.5873819
G. Warren, R. Detwiler, P. Peplowski
Nuclear Resonance Fluorescence (NRF) has the potential of addressing a wide variety of applications, which require isotopic and/or elemental information about a sample. We have investigated a variety of non-proliferation applications that may be addressed by NRF. From these applications, we have selected two, measuring uranium enrichment in UF6 cylinders and material verification in dismantlement, to investigate in more detail. Analytical models have been developed to evaluate these applications, and test measurements have been conducted to validate those models. We found that it is unlikely with current technology to address the requirements for UF6 cylinder enrichment measurements. In contrast, NRF is a very promising approach for material verification for dismantlement.
核共振荧光(NRF)具有解决各种各样的应用,这需要同位素和/或元素信息的样品的潜力。我们已经研究了各种各样的防扩散应用,可以通过NRF来解决。从这些应用中,我们选择了两个,测量UF6钢瓶中的铀浓缩和拆除中的材料核查,以进行更详细的研究。已经开发了分析模型来评估这些应用,并进行了测试测量来验证这些模型。我们发现,目前的技术不太可能满足UF6钢瓶富集测量的要求。相反,非核反应堆是一种非常有前途的拆除材料核查方法。
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引用次数: 2
Results with a 32-element dual mode imager 结果32元双模成像仪
Pub Date : 2010-11-01 DOI: 10.1109/NSSMIC.2010.5874053
J. Brennan, R. Cooper, M. Gerling, P. Marleau, N. Mascarenhas, S. Mrowka
We present advances with a 32 element scalable, segmented dual mode imager. Scaling up the number of cells results in a 1.4 increase in efficiency over a system we deployed last year. Variable plane separation has been incorporated which further improves the efficiency of the detector. By using 20 cm diameter cells we demonstrate that we could increase sensitivity by a factor of 6. We further demonstrate gamma ray imaging in from Compton scattering. This feature allows for powerful dual mode imaging. Selected results are presented that demonstrate these new capabilities.
我们提出了一个32元可扩展,分段双模式成像仪的进展。与我们去年部署的系统相比,增加电池数量可以使效率提高1.4倍。采用可变平面分离,进一步提高了探测器的效率。通过使用直径20厘米的电池,我们证明我们可以将灵敏度提高6倍。我们从康普顿散射进一步论证了伽马射线成像。此功能允许强大的双模式成像。本文给出了演示这些新功能的选定结果。
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引用次数: 6
Neutron imaging using the anisotropic response of crystalline organic scintillators 利用晶体有机闪烁体各向异性响应的中子成像
Pub Date : 2010-11-01 DOI: 10.1109/NSSMIC.2010.5874055
E. Brubaker, J. Steele
An anisotropy in a scintillator's response to neutron elastic scattering interactions can in principle be used to gather directional information about a neutron source using interactions in a single detector. In crystalline organic scintillators, such as anthracene, both the amplitude and the time structure of the scintillation light pulse vary with the direction of the proton recoil with respect to the crystalline axes. Therefore, we have investigated the exploitation of this effect to enable compact, high-efficiency fast neutron detectors that have directional sensitivity via a precise measurement of the pulse shape. We report measurements of the pulse height and shape dependence on proton recoil angle in anthracene, stilbene, p-terphenyl, diphenyl anthracene (DPA), and tetraphenyl butadiene (TPB). Image reconstruction for simulated neutron sources is demonstrated using maximum likelihood methods for optimal directional sensitivity.
闪烁体对中子弹性散射相互作用响应的各向异性原则上可用于利用单个探测器中的相互作用收集有关中子源的方向信息。在晶体有机闪烁体中,如蒽,闪烁光脉冲的振幅和时间结构都随质子反冲相对于晶体轴的方向而变化。因此,我们研究了利用这种效应来实现紧凑、高效的快中子探测器,通过精确测量脉冲形状来具有方向灵敏度。我们报告了脉冲高度和形状依赖于质子反冲角在蒽,苯乙烯,对三苯基,二苯基蒽(DPA)和四苯基丁二烯(TPB)的测量。利用最大似然方法对模拟中子源的图像重建进行了论证,以获得最佳的方向灵敏度。
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引用次数: 13
期刊
IEEE Nuclear Science Symposuim & Medical Imaging Conference
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