• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 1996년도 추계학술대회논문집; 한국과학기술회관, 8 Nov. 1996
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• pp.422-430
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• 1996

The automated scanning laser Doppler vibrometer (LDV) has been designed, and built to measure in-plane displacements associated with waves propagating on vibrating structures. Use of optical fibers allows the compact design of a laser probe head which can be scanned over the vibrating structures. An algorithm for automated self-alignment of the laser probe is developed. The system is completely automated for scanning over the structures, focusing two laser beams at each data point until the detected vibration signal is stable, and for recording and transferring the data to a system computer. The automated system allows one to get extensive data of the vibration field over the structures. The system is tested by scanning a piezoelectric cylindrical shell and a plate excited by a continuous signal and by a pulse signal, respectively. Results show that the automated scanning LDV system can be a useful tool to measure the in-plane vibration field and to detect the elastic waves propagating on the vibrating structures.

• 한국항공우주학회지
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• 제43권3호
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• pp.265-271
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• 2015

본 연구에서는 소형 위성카메라의 영상성능 저하를 궤도상에서 능동적으로 보정하기 위해 광학보정장치를 적용한 위성카메라의 광학설계를 수행하였다. 2개의 광학 보정장치는 각각 부반사경 및 초점면부에 부착되며 총 5자유도의 운동이 가능하다. 본 논문에서 설계한 광학부는 슈미트-카세그레인(Schmidt-Cassegrain)타입으로 주반사경의 직경은 200mm이고, GSD 3.8m, MTF 성능은 약 50% 정도이다. 설계된 광학계는 수차곡선과 Spot diagram과 MTF를 통해 성능평가를 수행하였다. 수차곡선을 통해 광학성능에 가장 큰 영향을 미치는 수차가 구면수차인 것을 확인 할 수 있고, MTF 해석을 통해서 나이퀴스트 주파수에서 MTF 30%이상의 요구 성능을 충분히 만족하는 것을 확인하였다.

• KSII Transactions on Internet and Information Systems (TIIS)
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• 제12권10호
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• pp.4903-4929
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• 2018

In this study, a fully automatic pose and expression invariant 3D face alignment algorithm is proposed to handle frontal and profile face images which is based on a two pass course to fine alignment strategy. The first pass of the algorithm coarsely aligns the face images to an intrinsic coordinate system (ICS) through a single 3D rotation and the second pass aligns them at fine level using a minimum nose tip-scanner distance (MNSD) approach. For facial recognition, multi-view faces are synthesized to exploit real 3D information and test the efficacy of the proposed system. Due to optimal separating hyper plane (OSH), Support Vector Machine (SVM) is employed in multi-view face verification (FV) task. In addition, a multi stage unified classifier based face identification (FI) algorithm is employed which combines results from seven base classifiers, two parallel face recognition algorithms and an exponential rank combiner, all in a hierarchical manner. The performance figures of the proposed methodology are corroborated by extensive experiments performed on four benchmark datasets: GavabDB, Bosphorus, UMB-DB and FRGC v2.0. Results show mark improvement in alignment accuracy and recognition rates. Moreover, a computational complexity analysis has been carried out for the proposed algorithm which reveals its superiority in terms of computational efficiency as well.

• 한국컴퓨터정보학회논문지
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• 제16권9호
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• pp.27-33
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• 2011

본 논문에서는 필기체 문자의 Convex-Concave한 곡선 특징을 문자로 변환하고 추출된 문자를 Smith-Waterman 정렬 알고리즘을 이용하여 온라인 필기체 숫자 인식 방법을 제안한다. 필기체 숫자 인식을 위한 입력 데이터는 시간에 순서적인 좌표로 순서화하고 전처리의 입력데이터로 적용된다. 필기자의 개성이 표현된 필기체 문자는 크기, 회전, 곡선 비율이 다양한 형태로 나타난다. 따라서 본 논문에서는 곡선의 Convex-Concave 특징을 이용하여 크기, 회전에 강인한 특징을 추출한다. 추출된 특징은 문자로 변환하고 Smith-Waterman 정렬 알고리즘의 입력데이터로 적용한다. 본 논문에서는 실시간 필기체 숫자를 대상으로 실험한 결과, 오류역전파 신경 회로망을 적용한 것과 비교하여 제안된 방법이 좋은 성능을 보였다.

• Clinics in Orthopedic Surgery
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• 제10권4호
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• pp.500-507
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• 2018

Background: The sagittal alignment of the spine and pelvis is not only closely related to the overall posture of the body but also to the evaluation and treatment of spine disease. In the last few years, the EOS imaging system, a new low-dose radiation X-ray device, became available for sagittal alignment assessment. However, there has been little research on the reliability of EOS. The purpose of this study was to evaluate the intrarater and interrater reliability of EOS for the sagittal alignment assessment of the spine and pelvis. Methods: Records of 46 patients were selected from the EOS recording system between November 2016 and April 2017. The exclusion criteria were congenital spinal anomaly and deformity, and previous history of spine and pelvis operation. Sagittal parameters of the spine and pelvis were measured by three examiners three times each using both manual and EOS methods. Means comparison t-test, Pearson bivariate correlation analysis, and reliability analysis by intraclass correlation coefficients (ICCs) for intrarater and interrater reliability were performed using R package "irr." Results: We found excellent intrarater and interrater reliability of EOS measurements. For intrarater reliability, the ICC ranged from 0.898 to 0.982. For interrater reliability, the ICC ranged from 0.794 to 0.837. We used a paired t-test to compare the values measured by manual and EOS methods: there was no statistically significant difference between the two methods. Correlation analysis also showed a statistically significant positive correlation. Conclusions: EOS showed excellent reliability for assessment of the sagittal alignment of the spine and pelvis.

• PNF and Movement
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• 제12권4호
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• pp.243-248
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• 2014

Purpose: The transverse abdominis and themultifidus muscle are located in the core. They surround one's trunk and help in body stabilization. Specifically, they control spine articulation to maintain posture and balance. Therefore, weakened deep muscle in the trunk may cause spinal malalignment. This study aims to compare the correlation between the thickness of the transverse abdominis and the multifidus muscle and the spine alignment among college students in their 20s. Methods: This study measured the thickness of the transverse abdominis and the multifidus muscle of 42 healthy college students in their 20s using ultrasonic waves. The thickness of the muscle was measured for the length of the cross-section except for fascia. The thickness of the left and right muscles was measured, and the mean value was calculated. As the thickness of the transverse abdominis can increase because of pressure during exhalation, it was measured at the last moment of exhalation. Spinal alignment was measured by the kyphosis angle, lordosis angle, pelvic tilt, trunk inclination, lateral deviation, trunk imbalance, and surface rotation using Formetric III, which is a three-dimensional imaging equipment. They were measured for three times, and the mean values were calculated. The general characteristics of the subjects were analyzed using descriptive statistics. The correlations between each factor were analyzed using Pearson's correlation analysis. Results: The transverse abdominis showed asignificant correlation with trunk inclination (p<.05). The multifidus muscle showed a significant positive correlation with pelvic tilt and a negative correlation with surface rotation (p<.05). Conclusion: The thickness of transverse abdominis and the multifidus muscle appears to influence spinal alignment. Specifically, the multifidus muscle, which plays an important role on the sagittal plane, influences surface rotation, thus making it an important muscle for scoliosis patients. Therefore, a strengthening training program for the transverse abdominis and the multifidus muscle is necessary according to specific purposes among adults with spinal malalignment.

• 한국위성정보통신학회논문지
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• 제7권3호
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• pp.54-57
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• 2012

최근 비접촉식 액정배향방법에 대한 요구가 산업계 전반으로 확산되면서, 기존의 UV 광배향을 비롯하여, 여러 가지 비접촉식 액정 배향방법이 활발히 연구되고 있다. 본 연구에서는 이러한 비접촉식 액정배향방법 중에서 SiOF 무기막에 이온빔을 정량적으로 조사하는 방법을 사용하여 액정을 배향하고, 이 기술을 사용하여, 상용화 수준의 IPS(In-Plane Switching) 방식의 액정 셀을 제작함으로써 전기광학 특성을 평가하였다. 특히 이러한 무기막 배향의 경우 배향안정성에 많은 문제를 가지고 있는 것이 보통이나, 본 연구에서 제안한 방법으로 제조된 평가셀은 $200^{\circ}C$의 높은 온도로 열처리를 하여도 배향성을 잃지 않고 균일한 배향을 지속하는 것을 관찰할 수 있었다.

• 천문학회보
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• 제42권1호
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• pp.56.4-57
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• 2017

The Schwarzschild-Chang off-axis telescope is a "linear astigmatism-free" confocal system. The telescope comprises two pieces of aluminum-alloy freeform mirrors that are fabricated with diamond turning machine (DTM) process. We designed optomechanical structures where optical components in the telescope system can be adjustable on a linear stage. Optomechanical deformation caused by the weight of system itself and its temperature variation is analyzed by the finite element analysis (FEA). The results show that the deformation is estimated in the tolerance range. For the optic-axis alignment of telescope system, three-point alignment (TPA) method is chosen. The TPA method uses three parallel lasers and a plane mirror. Point source images were taken from collimated light and field observation. The performance of optical system was tested by point spread function and aberration measurement of the point sources.

• 대한치과교정학회지
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• 제18권1호
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• pp.65-78
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• 1988

The development of good arch form, the orientation of the dentition with relation to the craniofacial skeleton and the establishment of correct relationship of axial inclination of upper and lower teeth are required in normal occlusion, but different teeth present different degrees of axial inclination. The purpose of this study was to investigate the axial inclination of upper and lower teeth by analyzing $45^{\circ}$ oblique and $90^{\circ}$ cephalometric roentgenograms of 35 Korean males and 34 females with normal occlusion. The obtained results were as follows: 1. Mean and standard deviation of mesiodistal axial inclination of upper and lower teeth related to palatal plane and occlusal plane were obtained. 2. Mesiodistal axial inclination of upper first premolar was nearly perpendicular to palatal plane, and the axis of lower first premolar was nearly perpendicular to occlusal plane. 3. There was no difference in the mesiodistal axial inclination of anteriorly positioned teeth between the three groups: third molar eruption into good alignment (Group 1), third molar impaction or partial eruption (Group 2), third molar agenesis (Group 3). 4. There were low correlationships only between the axial inclination of central incisor and the mesiodistal axial inclination of canine and first premolar, but no correlationships between central incisor and posterior teeth behind first premolar.

• 천문학회보
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• 제40권2호
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• pp.29.2-29.2
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• 2015

Interactions such as mergers and flybys play a fundamental role in shaping galaxy morphology. We used the Horizon Run 4 cosmological N-body simulations to study the aligments of spins and shapes of interacting haloes as a function of the halo mass and large-scale density. Interactions preferentially occur in the plane of rotation, and in the direction of the major axis of prolate haloes, and the trajectories are preferentially radial and prograde. We found a very strong alignment of the shapes already at redshift as high as 4. The spins are initially unaligned or even anti-aligned, and become more and more aligned as the redshift decreases. The alignment signals are stronger and evolve more at lower densities, and mass plays a secondary role.