JOURNAL OF APPLIED PHYSICS 105, 094701 共2009兲 Performance characterization of microtomography with complementary metal-oxide-semiconductor detectors for computer-aided defect inspection Ho Kyung Kim,1,a兲 Seungman Yun,1 Jong Chul Han,1 Hanbean Youn,1 Min Kook Cho,1 Chang Hwy Lim,1 Sung Kyn Heo,2 Cheol-Soon Shon,2 Seong-Sik Kim,3 Bong Hae Cho,3 and Thorsten Graeve Achterkirchen4 1 School of Mechanical Engineering, Pusan National University, Jangjeon-dong, Geumjeong-gu, Busan 609735, Republic of Korea 2 Sensor Business Division, E-WOO Technology Co., Ltd., Bora-dong, Giheung, Gyeonggi-do 449-904, Republic of Korea 3 School of Dentistry, Pusan National University, Ami-dong, Seo-gu, Busan 602-739, Republic of Korea 4 Rad-icon Imaging Corp., Belick Street, Santa Clara, CA 95054-2404, USA 共Received 10 November 2008; accepted 26 March 2009; published online 6 May 2009兲 We developed a computer-aided defect inspection system based on computed tomography 共CT兲. The system consists of a homemade small cone-beam CT 共CBCT兲 system and a graphical toolbox, which is used to extract a computer-aided design 共CAD兲 model from the CT data. In the small CBCT system, the x-ray imaging detector is based on a complementary metal-oxide-semiconductor photodiode array in conjunction with a scintillator. Imaging performance of the detector was evaluated in terms of modulation-transfer function, noise-power spectrum, and detective quantum efficiency. The tomographic imaging performance of the small CBCT system was evaluated in terms of signal-to-noise ratio and contrast-to-noise ratio. The graphical toolbox to support defect inspection incorporates various functional tools such as volume rendering, segmentation, triangular-mesh data generation, and data reduction. All the tools have been integrated in a graphical-user interface form. The developed system can provide rapid visual inspection as well as quantitative evaluation of defects by comparing the extracted CAD file with the original file, if available, of an object. The performance of the developed system is demonstrated with experimental CT volume data. © 2009 American Institute of Physics. 关DOI: 10.1063/1.3124360兴 I. INTRODUCTION X-ray computed tomography 共CT兲 is not only a well recognized imaging modality in medicine1 but also an essential one in industrial quality control and nondestructive evaluation.2,3 The recent cone-beam CT 共CBCT兲, enabling three-dimensional 共3D兲 scanning in almost real time, pushes further up the necessity in industry. Although the detailed technologies in CBCT, such as imaging detectors, scanning geometry, and image reconstruction algorithms, are still under development, the overall framework has been matured enough for diverse applications. Recent developments in microfocus x-ray sources and large-area pixel detectors resulted in the development of CBCT systems with resolving power of the order of tens of micrometers; these CBCT systems are called microtomography 共micro-CT兲 systems.4,5 Although micro-CT has the same technology as conventional CT, and thus, not a novel technology, the micro-CT has many new potential applications in biological as well as materials sciences.6–9 Moreover, with the 3D volume CT, the output voxel data can be used for rapid prototyping 共RP兲 modeling, nondestructive testing and evaluation, and reverse engineering, etc. In these aspects, the extraction of computer-aided design 共CAD兲 models of an object from CT data is essential. a兲 Electronic mail: hokyung@pnu.edu. 0021-8979/2009/105共9兲/094701/8/$25.00 We developed a cost-effective laboratory micro-CT system as well as software to support the defect inspection of small parts. The core of the micro-CT system is an x-ray detector. Since the performance of the detector is mostly responsible for image quality and eventually the quality of the tomographs, characterization of the detector is an important issue. The imaging characteristics of the detector were evaluated in terms of modulation-transfer function 共MTF兲, noisepower spectrum 共NPS兲, and detective quantum efficiency 共DQE兲. Tomographic imaging performances of the system, such as signal-to-noise ratio 共SNR兲 and contrast-to-noise ratio 共CNR兲, have also been evaluated by using quantitative phantoms. The micro-CT system and software, which is the integrated graphical toolbox for extracting CAD files in standard triangulation language 共STL兲 format from the voxel data, are described in detail. The overall performance of the developed toolbox is demonstrated with the experimental volume CT data. II. MATERIALS AND METHODS A. Micro-CT system We developed a cost-effective micro-CT system. As shown in Fig. 1, the system consists of an x-ray source with small focal spot, an object jig, and an x-ray imaging detector.5 The source-to-object and source-to-detector distances 共SOD and SDD兲 are variables determining the imaging parameters, such as the geometrical magnification ratio, 105, 094701-1 © 2009 American Institute of Physics Downloaded 06 May 2009 to 164.125.73.26. Redistribution subject to AIP license or copyright; see http://jap.aip.org/jap/copyright.jsp 094701-2 J. Appl. Phys. 105, 094701 共2009兲 Kim et al. FIG. 1. Schematic describing the developed micro-CT system. The x-ray source continuously irradiates an object fixed onto a jig, which is rotated at a constant angular velocity, and the 2D imaging detector acquires a projection view at a given integration time. All the operations of components are computer controlled. The source status, such as potential and current, is separately monitored. Two variable distances, SOD and SDD, determine the system magnification factor, the actual cone-beam angle, and FOV of the object. actual cone-beam angles, and field-of-view 共FOV兲. A computer-controlled rotation system was adopted in the object jig for the cone-beam mode scan. The precision of the rotational motion was 0.036°. The x-ray source 共Series 5000 Apogee, Oxford Instruments, USA兲 is a sealed tube with a 125-m-thick beryllium exit window. A tungsten target produces x rays with energies ranging from 4 to 50 kVp at 50 W. Imaging conditions can be further enhanced by tailoring the x-ray beam profile with additional filtration. The nominal focal spot size is 35 m. The emitted x-ray beam angle is about 22°. The x-ray source continuously irradiates the sample to be imaged without any shutters while the detector acquires two-dimensional 共2D兲 projection data at a given frame time 共or integration time兲. The detector is based on a photodiode array in conjunction with a scintillator. A commercial phosphor screen 共MinR™, Carestream Health Care Inc., USA兲 was used as the scintillator. The screen is mainly made of a terbium-doped gadolinium oxysulfide 共Gd2O2S : Tb兲 showing an emission spectrum with the main peak at 545 nm. The photodiode arrays made by the complementary metal-oxidesemiconductor 共CMOS兲 process 共RadEye™, Rad-icon Imaging Corp., USA兲 were employed as the optical photon readout device.10 The CMOS photodiode array has a format of 512⫻ 1024 pixels with a pitch of 48 m. Only one narrow side of the CMOS photodiode array incorporates the readout electronics to allow tiling of the CMOS photodiode array into large mosaics. In this study, two CMOS photodiode arrays were tiled side by side and therefore the FOV was about 50⫻ 50 mm2. Two parallel voltage signals from the two CMOS photodiode arrays are then simultaneously digitized to 12-bit gray level through dual analog-to-digital converters 共ADCs兲 共PCI-6111, National Instruments, USA兲. The 12-bit image data are converted into 16-bit form for postprocessing and image reconstruction. The frame time of the CMOS detector to acquire a single projection could be variable and we normally operated the detector with the frame time of 275 ms. Algorithms and software to acquire digital x-ray images, to apply postimage processing, and to reconstruct volumetric images were developed by using Microsoft Visual C⫹⫹®. When we operated the system in the CT scan mode, the magnification factor was usually set to about 2 and image data were obtained through a 360° scan. For image reconstruction, we employed the Feldkamp’s cone-beam algorithm11 to the projection data filtered with a Ram-Lak filter 共or high-pass filter兲.12 The Feldkamp’s algorithm is a simple extended version of the conventional filtered backprojection method in longitudinal direction by considering cone angles. Therefore, it is an approximate approach and may cause distortion when the cone angle is wide. However, since Feldkamp’s algorithm is very fast and easily applicable, it is mostly widely used in commercial CBCT systems. For a typical scan in this study, the size of the acquired data was about 1 Gbyte 共=2 bytes/ pixel⫻ 10242 pixels/ projection ⫻ 500 projections兲. B. Imaging characteristics of the CMOS detector The performance of the CMOS detector has been evaluated in terms of MTF, NPS, and DQE, which are fundamental metrics describing the physical imaging characteristics of an imaging system. The MTF describes the contrast transfer efficiency as a function of an object detail, hence the resolving power of an imaging system. The NPS measures the change in the noise amplitude as a function of spatial frequency and bridges the noise power and spatial resolution in an image. The DQE is a measure of the square of the SNR 共SNR2兲 transfer and measures the fraction of the incident x-ray fluence contributing to image quality. Therefore, the DQE represents the performance of an imaging system. A detailed description of measurement procedures can be found in a previous study.13 Briefly, the presampling MTF was measured using the slanted-slit method to avoid aliasing14 and the NPS was determined by 2D Fourier analysis of white images.15,16 Gain and offset corrections were performed on all images used to obtain the MTF and NPS. We actually measured a normalized NPS 共NNPS兲 to avoid the additional measurement of the detector gain. A 45 kVp x-ray spectrum tailored by a 0.5-mm-thick aluminum filter was used for all measurements. The DQE was then assessed from the measured MTF, NPS, and the estimated photon fluence q̄ as DQE共f兲 = MTF2共f兲 q̄ ⫻ NNPS共f兲 , 共1兲 where f denotes the spatial frequency. The fluence was calculated using the experimentally measured exposure and half-value layer, and the computational program for x-ray spectral analysis.17 The exposure rate at the entrance surface of the detector was measured by replacing the detector with a calibrated ion chamber 共Victoreen 6000–528, Inovision, USA兲 while keeping the same distance. Downloaded 06 May 2009 to 164.125.73.26. Redistribution subject to AIP license or copyright; see http://jap.aip.org/jap/copyright.jsp 094701-3 J. Appl. Phys. 105, 094701 共2009兲 Kim et al. D. Graphical toolbox to extract CAD files from CT data FIG. 2. 共Color online兲 Homemade phantoms to evaluate the tomographic imaging performance of the micro-CT system. 共a兲 The cylindrical acrylic vessel, which contains water, is scanned for the estimation of the voxel noise and SNR. 共b兲 Low-contrast inserts, which are immersed in water inside the cylindrical acrylic vessel and scanned for the estimation of CNR. Each insert has three different diameters: 1.5, 3.0, and 5.0 mm. C. Tomographic imaging performances of the microCT system Tomographic imaging performance of the developed micro-CT system was evaluated with homemade quantitative phantoms as shown in Fig. 2. A water-filled cylindrical acrylic vessel having a diameter of 30 mm was used in evaluating the voxel signal and noise characteristics. The CNR was evaluated with the contrast phantom, which consists of six low-contrast inserts. The contrast phantom is completed when the inserts are immersed in the water vessel. As shown in Fig. 2共b兲, each insert was made of commercial electronic density phantoms 共Model 76-430, Nuclear Associates, NY, USA兲 and it had three different diameters; 1.5, 3.0, and 5 mm. The insert materials are plastic water nylon 共1.15 g / cm3兲, polyethylene 共1.03 g / cm3兲, 3 acryl 共1.18 g / cm3兲, polystyrene 共0.95 g / cm 兲, 共1.11 g / cm3兲, and polycarbonate 共1.18 g / cm3兲, and their densities are similar to that of water. From the crosssectional images obtained with the contrast phantom, the CNR was calculated by18 CNRi = 兩S̄i − S̄w兩 冑2i + w2 , 共2兲 where S̄ and are the mean signal and standard deviation of the voxel values, respectively. The subscripts i and w denote the inserts and the background water region in the contrast phantom, respectively. The CNR was analyzed in terms of various imaging conditions, such as dose, diameter of inserts, and slice thickness. Radiation doses, addressed in this study, are based on the exposure measurement in air at the axis-of-rotation 共AOR兲.19 To take into account the dose, the measured exposure was converted to the kerma in air using the exposure-to-kerma conversion factor of 8.736 mGy/R for the x-ray spectrum of 45 kVp, which was interpolated with tabulated data between 40 and 50 kVp.20 In this study, we used two approaches for defect inspection. One is a simple visual inspection of three-dimensionally reconstructed image data. The other is the defect inspection based on CAD data. In these regards, we developed a graphical toolbox capable of visualizing 3D data as well as extracting CAD files from the CT data. Main functional tools incorporated in the developed toolbox are the volumetric rendering of the reconstructed 3D data, the segmentation of region-of-interests 共ROIs兲, the generation of triangular-mesh data of the segmented ROIs, and the smoothening and reduction of mesh data. Volume rendering is a discrete representation and visualization of objects as sampled data, of not only the surface but also the entire inner of an object, in three dimensions. We independently considered two different methods, such as ray casting and maximum intensity projection 共MIP兲.21 Ray casting is a direct volume rendering that sums the intensity values of voxels based on the light absorbed as it propagates from back to front through the 3D voxel data set. On the other hand, in the MIP method, the shade of gray of a voxel having maximum intensity is chosen in the 3D voxel data encountered along the projection line. We consider the STL format as a CAD file, which is mesh data containing geometrical information that details the object.22 It consists of vectors designating three vertices of a triangle and its surface normal vector. The procedure to extract a STL file from the voxel data mainly consists of two steps: segmentation of voxel data in binary form and triangulation of the segmented volume data. Segmentation, the most important procedure, is very sensitive to each voxel value and largely responsible for the reliability of the mesh data. We basically incorporate the thresholding method based on histogram analysis. The threshold is determined by a simple calculation that maximizes the variance of the intensities between the user-defined ROI and the other regime in the histogram.23 This approach can be easily realized with effective computation. In order to generate triangle meshes, we employed the well-known marching cube algorithm.24 A virtual cube is defined by eight-pixel 共or eight-vertex兲 values between two vertically consecutive slices of the segmented volume data. Therefore, this algorithm determines how the slice surfaces intersect the cube by comparing the vertex values, which are prescribed as unities, with the segmented data. Since possible triangles 共256 cases兲 are already prepared as a look-up table, the triangulation is automatic. The cube marches to the next location and the process is repeated. However, since the number of triangles that could be generated per cube is limited to four,24 the degree of surfaces that should be expressed is restricted. Reducing the gap between slices or a higherorder interpolation method might be a way to overcome this restriction, but it entails computational cost. It is completed when the triangulated meshes are exported according to the STL file format. Since the file size of the mesh data extracted by the marching cube algorithm is normally large, it is often necessary to remove unnecessary meshes and merge the meshes in Downloaded 06 May 2009 to 164.125.73.26. Redistribution subject to AIP license or copyright; see http://jap.aip.org/jap/copyright.jsp 094701-4 Kim et al. J. Appl. Phys. 105, 094701 共2009兲 coplanar planes.25 This data reduction process should preserve the original topology and approximate the original geometry reasonably. We employed various mesh-data reduction algorithms, such as mesh decimation, quadric decimation, and quadric clustering.25 Most of the algorithms describing each tool were coded by using Microsoft Visual C⫹⫹®. For user convenience, the toolbox was developed in an integrated graphical user interface 共GUI兲 form. E. Experimental simulation In order to implement the developed toolbox, we designed a chessman, bishop, in STL file format using a commercial CAD software, Pro/Engineering™ and manufactured an RP sample using optical stereolithography 共SLA 350, 3D Systems, USA兲 with SL-51902 resin. The manufactured RP bishop sample was then scanned by the developed micro-CT system and a 3D image was reconstructed in voxel size of 0.096⫻ 0.096⫻ 0.096 mm3. By using the developed toolbox, we extracted the STL file from the scanned CT voxel data and used the developed toolbox to compare the extracted STL file with the original one. The bishop sample was designed to have a height of 67.44 mm and the manufactured RP sample was measured to 67.58 mm. Both the imaging FOV of the CMOS detector and the introduction of magnification in imaging geometry restricted the sample height to be imaged to about 34.69 mm. III. RESULTS FIG. 3. Fourier analyses for the imaging characteristics of the CMOS detector. 共a兲 The measured system MTF and theoretical MTFs representing physical parameters affecting the overall MTF, the focal spot of x-ray source, the pixel aperture of detector, and the width of slit camera. 共b兲 The measured NNPS and the least-squares fits to analyze the NNPS. 共c兲 The measured DQE. A. Radiographic imaging performance Fourier analysis of the radiographic imaging performance of the detector equipped in the micro-CT system is summarized in Fig. 3. The measured MTF is plotted in Fig. 3共a兲. At 10% of MTF, the spatial resolution is about 10.5 mm−1. We could easily resolve 10 lp/mm of the highresolution line-pair phantom from a separate measurement as shown in Fig. 4. Figure 3共b兲 describes the NNPS as a function of the spatial frequency. There is a noticeable increase in noise power around zero frequency due to large-scale gain variation across the detector, which would normally be eliminated by the gain correction procedure. In order to remove or reduce the large-scale nonuniformity, a 2D second-order polynomial fit to an image is used and is subtracted from the corresponding image. In this study, however, we subtracted the mean value of the image instead. The measured NPS shows essentially white-noise property with respect to the spatial frequency. The higher MTF performance might reflect this white-noise property in part because the noise is also transferred through the MTF as a signal.26 A previous study pointed out that in a detector employing a thin phosphor, the extra noise due to the direct absorption of x-ray photons in the photodiode is white.5 Together with the measured MTF and NNPS, the DQE was calculated and the result is shown in Fig. 3共c兲. B. Tomographic imaging performance Cross-sectional images of the contrast phantom with respect to various parameters, such as the diameter of the lowcontrast inserts, the dose and the slice thickness, are shown in Fig. 5. We applied narrow threshold windows to clearly differentiate the inserts. The default voxel size is 0.139 ⫻ 0.139⫻ 0.278 mm3. The voxel heights or the slice thicknesses of the images shown in Figs. 5共f兲 and 5共g兲 are 0.556 and 1.112 mm, respectively. FIG. 4. Radiograph of the line-pair test phantom, which supports the result of measured MTF. Downloaded 06 May 2009 to 164.125.73.26. Redistribution subject to AIP license or copyright; see http://jap.aip.org/jap/copyright.jsp 094701-5 Kim et al. J. Appl. Phys. 105, 094701 共2009兲 FIG. 7. The SNR, calculated from the images obtained for the water phantom, as a function of dose. The solid lines show a trend curve proportional to the square root of the dose. FIG. 5. Cross-sectional images of the contrast phantom with respect to various imaging parameters, such as the dose, the diameters of inserts, and the slice thickness. Reference images of 共a兲–共c兲 depict the effect of the insert diameter, 共d兲 and 共e兲 the effect of the dose, and 共f兲 and 共g兲 the effect of the slice thickness. Note that and t denote the insert diameter and the slice thickness, respectively. For three different diameters of inserts 关see Figs. 5共a兲–5共c兲兴, no severe change in contrast was observed, even down to the diameter of 1.5 mm, for each insert material. The acquired images also showed similar CNR values and tendencies as a function of dose for the three different diameters of inserts. For the inserts having a diameter of 1.5 mm, the calculated CNR as a function of the dose at the AOR is plotted in Fig. 6. The CNR was found to be proportional to the square root of the dose.27 Figure 5共a兲, 5共d兲, and 5共e兲 demonstrate the effect of dose on visual impact. In general, the image quality of a radiograph is mainly dependent on the number of detected photons and it is definitely increased as the number of incident x rays is increased. The tomograph becomes poorer as the dose FIG. 6. The CNR, calculated from the images obtained for low-contrast inserts having a diameter of 1.5 mm, as a function of dose. The dotted lines are trend curves that are proportional to the square root of the dose. decreases. For a given dose, the increase in the slice thickness has the same effect as an increased number of detected photons, as shown in Figs. 5共a兲, 5共f兲, and 5共g兲. In all the measurements, the worst CNR was observed with the insert made of acrylic. The minimum resolvable CNR with the naked eye was approximately 1 and the voxel noise of the water phantom corresponding to this CNR value was about 250 CT numbers. The SNR, calculated from the measured cross-sectional image of the water phantom, as a function of dose is shown in Fig. 7. Like the CNR, the SNR is also dependent on the square root of dose. At the dose of 83 mGy, the SNR is about 6, and the corresponding voxel noise is 295 CT numbers. C. Graphical toolbox and the extraction of CAD files from CT data Figure 8 describes the main frame of the developed graphical toolbox. The toolbar at the top of the main frame contains various symbolic buttons, which are used to run the corresponding functions, such as loading of the volume data or STL data, handling of visualization and cropping, the ex- FIG. 8. 共Color online兲 Screenshot of the main window describing the developed graphical toolbox. Downloaded 06 May 2009 to 164.125.73.26. Redistribution subject to AIP license or copyright; see http://jap.aip.org/jap/copyright.jsp 094701-6 Kim et al. J. Appl. Phys. 105, 094701 共2009兲 the approximate Feldkamp’s algorithm for cone angle could produce an error,11 the generated error for small cone angle or small sample volume would be negligible. For the reliable performance evaluation of the developed system, the error should be quantitatively analyzed in terms of each contributing factor. IV. DISCUSSIONS AND CONCLUSION FIG. 9. 共Color online兲 Experimental simulation with a chessman, bishop, using the developed toolkit. 共a兲 Original CAD data, which were as an input file for the RP machine, and the manufactured RP bishop sample. 共b兲 3Drendered images of voxel data obtained from the CT scan. Two different visualizations, ray casting, and MIP, are shown. 共c兲 Extracted CAD files from the voxel data by using the developed toolkit. The left is the extracted, as is, and the right is after decimation and smoothening processes. 共d兲 A map describing the difference between the original and the extracted CAD files. traction of STL files from the volume data including segmentation and triangulation, etc. The loaded 3D CT or STL image is displayed on four subwindows. The large window renders a 3D view of an object. In this window, cropping and free rotation of the 3D view for any axis can help the inner and surface investigations. The small three subwindows describe the cross-sectional views of the object parallel to x, y, and z, and those are synchronized with one anther so that we can simultaneously identify the inner investigation for the three axes. Figure 9 shows the results of the experimental simulation. Figure 9共a兲 shows the original CAD file 共left兲 used as the input file for the RP machine and the photograph of the manufactured RP bishop sample 共right兲. 3D-rendered images of the CT-scanned voxel data are shown in Fig. 9共b兲. Two different visualizations, i.e., ray casting 共left兲 and MIP 共right兲 are shown. Figure 9共c兲 shows the extracted CAD files from the developed toolbox and two images are distinguished from each other by the degree of data reduction and smoothing. As designated by magnifiers, the right image was obtained after about 30% reduction in the number of meshes. Figure 9共d兲 shows a difference map of geometries and dimensions between the original and extracted CAD files. The scale bar designates the degree of difference in dimension in the unit of millimeter. As shown in Fig. 9共d兲, the difference is as large as 1 mm, but this is not purely resulted from the manufacturing error. The most significant factor affecting the errors is presumed to misalignment in imaging geometry, which was not characterized in this study. Another cause that may provide an error is probably the threshold-based segmentation procedure because the threshold determined from histogram already has some extent of uncertainty.23 Although The overall MTF of the detector system is affected by various physical parameters such as the x-ray focal spot size, the slit width, the magnification ratio, and the inherent detector resolving power.19 The inherent resolving power of the detector employed in this study is mainly determined by the optical photon scattering in the phosphor screen and the pixel aperture size of the CMOS photodiode array. Since the SDD was set to 200 mm when measuring MTF with a slit camera having a 10-m-width slit aperture and made of the 1.5-mmthick tantalum28 and the slit camera was in contact with the entrance surface of the detector, we neglected the magnification of focal spot and slit width. The theoretical MTF due to an aperture function can be expressed by the “sine cardinal” or simply “sinc” function. Accounting for the onedimensional 共1D兲 geometries of the focal spot, the slit aperture, and the detector pixel, the theoretical MTFs are plotted in Fig. 3共a兲. The pixel MTF was estimated with consideration of the geometric pixel fill factor of 0.87. From the results, the overall MTF was seemed to be mostly determined by the resolving power of the phosphor screen; in other words, the dominant blurring factor was the optical photon scattering within the phosphor screen. On the other hand, tomography is obtained with a certain magnification factor, i.e., the ratio of SDD to SOD. Therefore, there is a compromise between the magnification of details in an object and the blur due to the magnified focal spot size. In addition, image reconstruction is another blurring factor in tomography.29 In the previous study on the development of a microtomography system incorporating a focal spot size of 10 m and a pixel pitch of 50 m,19 the system total MTF was mostly determined by the detector resolving power at the magnification factor of 2. We assumed that the system MTF of our micro-CT system would be similar. However, the MTF in tomography should be measured for optimal and reliable use. As long as the additive electronic noise is not exceptionally large, the NPS of an imaging system is mainly governed by the stochastic variation of information-carrying quanta introduced in various image-forming states. Typical examples are the interaction of x-rays in a scintillator, the absorption of its energy, the conversion of x-ray to optical photons, the spread of an optical photon burst, and the escape of optical photons, and, in a photodiode, the collection of optical photons, the conversion of optical photons to electronic charges, and the spread of electronic charges. This stochastic variation increases the noise at the output, and whose effect can be seen by examining the NPS. According to Rossmann,26 because the spatial-frequency dependence of the signal transfer is described by MTF共f兲, the NPS would behave as MTF2共f兲. However, as shown in Fig. 3共b兲, the Downloaded 06 May 2009 to 164.125.73.26. Redistribution subject to AIP license or copyright; see http://jap.aip.org/jap/copyright.jsp 094701-7 J. Appl. Phys. 105, 094701 共2009兲 Kim et al. NPS of our detector system shows behavior close to that of a white noise spectrum except at the very low frequency band, probably due to the imperfect removal of the fixed-pattern noise during the gain-offset correction procedure. For comparison, a best fit function, proportional to MTF2共f兲, is plotted in Fig. 3共b兲. A large discrepancy is observed in the high spatial-frequency region. From Lubberts,30 the NPS generally falls off more slowly at high frequency than the MTF2 because of the stochastic variation caused by the depthdependent interaction of x rays within a phosphor screen and the fluctuation of processes at the corresponding depth. Badano et al.31 demonstrated the Lubberts’ effect on a phosphor screen by estimating the Lubberts fraction, L共f兲 = MTF2共f兲 / NNPS共f兲 based on Monte Carlo simulation. However, their result on the phosphor screen having a similar thickness as that employed in our detector is quite different. Our measurement and analysis showed a much stronger effect than Lubberts’ effect, indicating another factor affecting the NPS degradation. A previous study5 pointed out that in a detector employing a thin phosphor, the extra noise due to the direct absorption of x-ray photons in the photodiode has a white spectrum. The direct x rays are those that are unattenuated from the phosphor screen and that directly interact with the photodiode. This additional white noise can further raise the spectral density in the high spatial frequency band. The proof that the NNPS due to the direct x rays is white is shown in Ref. 32. Considering this additional white noise, we analyzed the measured NPS with a least-squares fit of the form aMTF2共f兲 + b, where a and b are the constants obtained from the numerical fit and plotted the resultant fit in Fig. 3共b兲. This analysis was directly applied to the DQE result as shown in Fig. 3共c兲. The analysis reasonably agreed with the measured DQE data. The degradation of NPS due to the direct x-ray absorption noise decreased the DQE performance, especially in the high frequency region. Not only do direct x rays affect the image quality or the detector performance, such as NPS and DQE, but they also can give rise to a change in the characteristics of the active devices in the photodiode array, such as the leakage current of a photodiode and the threshold voltage of a switching transistor. The radiation-induced increase in the dark signal and noise can result in the gradual reduction in the dynamic range and enhance the fixed-pattern noise in digital radiography.33 Therefore, a phosphor screen must be designed or selected optimally. In digital radiography, the offset and gain correction is typically performed. With carefully updated and applied correction during the operation of CBCT, the detrimental effects of increased dark current on NPS and DQE can be overcomed.33 The applicability of the developed system is somewhat limited by the FOV of the detector. If magnified images and tomograms are needed for a detailed analysis of an object to be scanned, FOV becomes a more serious problem. The detector can extend the tiling approach of the CMOS photodiode array used in this study to a larger dimension, for example, the FOV of about 100⫻ 100 mm2 with 2 ⫻ 4 arrangements of the photodiode array. Moreover, commercial large-area flat-panel detectors are available. With an undersized detector, the extension of the reconstructed volume with mechanical motion or a smart image reconstruction algorithm is another approach that can be used to overcome the restricted FOV of a detector. Spiral motion, which is typical in medicine, on a long object is an example. For a wide object, by shifting a detector laterally so that data from at least half the width of the object are acquired for each view, the image reconstruction based on the estimation of the missing rays through the unprojected part of the object from the redundant rays can be used to enlarge the reconstructed volume in laterally.34 A series of algorithms to realize computer-aided defect inspection has been integrated in a GUI form. The developed graphical toolkit was used to extract CAD files from the scanned CT volume data of an RP sample. In the serial procedures, the most important procedure is the segmentation. An object containing various inner structures with similar material properties, such as density and atomic number, requires the implementation of more elaborate segmentation algorithms. However, the segmentation algorithm used in this study is reasonable for typical industrial applications because most industrial parts are composed of a few materials. Although the developed system is somewhat restricted in FOV, it can be used for diverse industrial applications, such as the inspection of solder joins in electronic components and reverse engineering of small parts, and for biological applications, such as small-animal imaging, tissue engineering, etc. ACKNOWLEDGMENTS This research was performed for the Nuclear R&D Programs 共Grant No. M20609000107-06B0900-10710兲 and the Korea Science and Engineering Foundation 共KOSEF兲 共Grant No. R01-2006-000-10233-0兲 funded by the Korean Government 共MEST兲. W. A. Kalender, Phys. Med. Biol. 51, R29 共2006兲. D. V. Rao, R. Cesareo, A. Brunetti, and G. E. Gigante, NDT & E Int. 33, 523 共2000兲. 3 J. Hofmann and A. Flisch, NDT & E Int. 39, 668 共2006兲. 4 B. P. Flannery, H. W. Deckman, W. G. Roberge, and K. L. D’Amico, Science 237, 1439 共1987兲. 5 M. K. Cho, H. K. Kim, T. Graeve, and J.-M. Kim, Key Eng. Mater. 321–323, 1052 共2006兲. 6 P. Rüegsegger, B. Koller, and R. Müller, Calcif. Tissue Int. 58, 24 共1996兲. 7 C. Neubauer, IEEE Trans. Compon., Packag. Manuf. Technol., Part B 20, 111 共1997兲. 8 A. Sasov and D. Van Dyck, J. Microsc. 191, 151 共1998兲. 9 S. C. Lee, H. K. Kim, I. K. Chun, M. H. Cho, M. H. Cho, and S. Y. Lee, Key Eng. Mater. 270–273, 245 共2004兲. 10 T. Graeve and G. Weckler, Proc. SPIE 4320, 68 共2001兲. 11 L. A. Feldkamp, L. C. Davis, and J. W. Kress, J. Opt. Soc. Am. A 1, 612 共1984兲. 12 G. N. Ramachandran and A. V. Lakshminarayanan, Proc. Natl. Acad. Sci. U.S.A. 68, 2236 共1971兲. 13 M. K. Cho, H. K. Kim, T. Greave, S. M. Yun, C. H. Lim, H. Cho, and J.-M. Kim, IEEE Trans. Nucl. Sci. 55, 1338 共2008兲. 14 H. Fujita, D. Y. Tsai, T. Itoh, K. Doi, J. Morishita, K. Ueda, and A. Ohtsuka, IEEE Trans. Med. Imaging 11, 34 共1992兲. 15 M. J. Flynn and E. Samei, Med. Phys. 26, 1612 共1999兲. 16 E. Samei and M. J. Flynn, Med. Phys. 30, 608 共2003兲. 17 C.-S. Shon, H. K. Kim, M. K. Cho, M. H. Cheong, C. H. Lim, and J.-M. Kim, Key Eng. Mater. 321–323, 1060 共2006兲. 18 H. K. Kim, S. C. Lee, M. H. Cho, S. Y. Lee, and G. Cho, IEEE Trans. Nucl. Sci. 52, 193 共2005兲. 19 S. C. Lee, H. K. Kim, I. K. Chun, M. H. Cho, S. Y. Lee, and M. H. Cho, 1 2 Downloaded 06 May 2009 to 164.125.73.26. Redistribution subject to AIP license or copyright; see http://jap.aip.org/jap/copyright.jsp 094701-8 Phys. Med. Biol. 48, 4173 共2003兲. J. M. Boone, in Handbook of Medical Imaging, edited by J. Beutel, H. L. Kundel, and R. L. Van Metter 共SPIE, Bellingham, WA, 2000兲, Vol. 1, Chap. 1, p. 61. 21 U. Tiede, K. H. Hoehne, M. Bomans, A. Pommert, M. Riemer, and G. Wiebecke, IEEE Comput. Graphics Appl. 10, 41 共1990兲. 22 D. Ma, F. Lin, and C. K. Chua, Int. J. Adv. Manuf. Technol. 18, 118 共2001兲. 23 N. Otsu, IEEE Trans. Syst. Man Cybern. 9, 62 共1979兲. 24 W. E. Lorensen and H. E. Cline, ACM SIGGRAPH, Comput. Graph. 共ACM兲 21, 163 共1987兲. 25 W. J. Schroeder, J. A. Zarge, and W. E. Lorensen, ACM SIGGRAPH, Comput. Graph. 共ACM兲 26, 65 共1992兲. 26 K. Rossmann, J. Opt. Soc. Am. 52, 774 共1962兲. 20 J. Appl. Phys. 105, 094701 共2009兲 Kim et al. 27 H. H. Barrett, S. K. Gordon, and R. S. Hershel, Comput. Biol. Med. 6, 307 共1976兲. 28 C. D. Bradford, W. W. Peppler, and M. Waidelich, Med. Phys. 26, 2286 共1999兲. 29 D. W. Holdsworth, M. Drangova, and A. Fenster, Med. Phys. 20, 449 共1993兲. 30 G. Lubberts, J. Opt. Soc. Am. 58, 1475 共1968兲. 31 A. Badano, R. M. Gagne, B. D. Gallas, R. J. Jennings, J. S. Boswell, and K. J. Myers, Med. Phys. 31, 3122 共2004兲. 32 H. K. Kim, Appl. Phys. Lett. 89, 233504 共2006兲. 33 H. K. Kim, M. K. Cho, and T. Graeve, J. Biomed. Eng. Res. 28, 756 共2007兲. 34 P. S. Cho, A. D. Rudd, and R. H. Johnson, Comput. Med. Imaging Graph. 20, 49 共1996兲. Downloaded 06 May 2009 to 164.125.73.26. Redistribution subject to AIP license or copyright; see http://jap.aip.org/jap/copyright.jsp