Ali E S M, Rogers D W O
Carleton Laboratory for Radiotherapy Physics, Ottawa Carleton Institute for Physics, Carleton University, 1125 Colonel By Drive, Ottawa, Ontario K1S 5B6, Canada.
Med Phys. 2008 Sep;35(9):4149-60. doi: 10.1118/1.2966348.
In a typical x-ray tube, off-focal radiation is mainly generated by the backscattered electrons that reenter the anode outside the focal spot. In this study, BEAMnrc (an EGSnrc user-code) is modified to simulate off-focal radiation. The modified BEAMnrc code is used to study the characteristics of electrons that backscatter from the anode, and to quantify their effect on the output of typical x-ray systems. Results show that the first generation backscatter coefficient is approximately 50% for tungsten anodes at diagnostic energies, and approximately 38% for molybdenum anodes at mammography energies. Second and higher generations of backscatter have a relatively minor contribution. At the patient plane, our simulation results are in excellent agreement with experimental measurements in the literature for the spectral shape of both the primary and the off-focal components, and also for the integral off-focal-to-primary ratio. The spectrum of the off-focal component at the patient plane is softer than the primary, which causes a slight softening in the overall spectrum. For typical x-ray systems, the off-focal component increases patient exposure (for a given number of incident primary electrons) by up to 11% and reduces the half-value layer and the effective energy of the average spectrum by up to 7% and 3%, respectively. The larger effects are for grounded cathode tubes, smaller interelectrode distance, higher tube voltage, lighter filtration, and less collimation. Simulation time increases by approximately 30% when the off-focal radiation is included, but the overall simulation time remains of the order of a few minutes. This study concludes that the off-focal radiation can have a non-negligible effect on the output parameters of x-ray systems and that it should be included in x-ray tube simulations for more realistic modeling of these systems.
在典型的X射线管中,焦外辐射主要由重新进入焦斑外阳极的背散射电子产生。在本研究中,对BEAMnrc(一种EGSnrc用户代码)进行了修改以模拟焦外辐射。修改后的BEAMnrc代码用于研究从阳极背散射的电子特性,并量化它们对典型X射线系统输出的影响。结果表明,在诊断能量下,钨阳极的第一代背散射系数约为50%,在乳腺摄影能量下,钼阳极的第一代背散射系数约为38%。第二代及更高代的背散射贡献相对较小。在患者平面,我们的模拟结果与文献中的实验测量结果在初级和焦外成分的光谱形状以及焦外与初级积分比方面都非常吻合。患者平面上焦外成分的光谱比初级光谱更软,这会导致整体光谱略有软化。对于典型的X射线系统,焦外成分会使患者照射量(对于给定数量的入射初级电子)增加高达11%,并使平均光谱的半值层和有效能量分别降低高达7%和3%。对于接地阴极管、较小的电极间距、较高的管电压、较轻的过滤和较少的准直,影响更大。当包含焦外辐射时,模拟时间增加约30%,但总体模拟时间仍为几分钟量级。本研究得出结论,焦外辐射对X射线系统的输出参数可能有不可忽略的影响,并且在X射线管模拟中应包含焦外辐射,以便对这些系统进行更逼真的建模。