• 대한치과보존학회:학술대회논문집
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• 대한치과보존학회 2003년도 제120회 추계학술대회 제 5차 한ㆍ일 치과보존학회 공동학술대회
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• pp.546.1-546
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• 2003

Laser doppler flowmeter (LDF) has been applied to the measurement of pulpal blood flow (PBF) in human teeth. As far as we searched, the detection area of the pulp in the blood flow measurement has not been clarified, yet. Therefore, the purpose of this study was to obtain information of the detection area in PBF measurement using LDF. The experiments were performed on the artificial blood circulation in extracted human upper central incisors. The apical portions of examined teeth (n=6) were severed and root canals were enlarged from the apical end to the 2mm incisal to the level of enamel-cement junction. An individual resin cap of each tooth was prepared and a hole was drilled 2mm incisal to enamel-cement junction of the labial side of the cap. The measurement probe of LDF (MBF3D, Moor Instrument, UK) was plugged into the hole of the cap. Heparinized human peripheral blood, which was in advance collected and diluted 3 times with physiological saline, was pumped through the apical foramen of the teeth via a silicone tube and a disposable needle (o.d. 0.7mm) and blood flow signals were monitored. The flux signal significantly increased with the enlargement of the root canal to incisal direction (p<0.01, Friedman analysis). The result indicates that the performance of LDF in PBF with human teeth is limited.

• 천문학회보
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• 제45권1호
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• pp.62.1-62.1
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• 2020

We present a scaling relation between black hole (BH) mass and bulge luminosity for 35 nearby (z<0.1) type 1 active galaxies, selected from the 70-month Swift-BAT X-ray source catalog. Thanks to the unbiased selection and proximity of the parent sample, our sample is suitable to study the physical connection between central black holes and host galaxies. We use the F814W images obtained with the Advanced Camera for Surveys on Hubble Space Telescope, to perform the imaging decomposition with GALFIT. With a careful treatment on the PSF model, we measure the I-band bulge brightness robustly. In combination with the BH mass estimated from a single-epoch spectroscopic data, we present the correlation between BH mass and bulge luminosity of the target AGNs. We demonstrate that our sample marginally lies off from the M(BH)-L(bulge) relation of inactive galaxies. We discuss possible physical origins of this discrepancy. Finally, we present how the relation depends on the photometric properties of AGNs and host galaxies, which may provide an useful insight on the co-evolution between BHs and host galaxies.

• 한국추진공학회:학술대회논문집
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• 한국추진공학회 2006년도 제27회 추계학술대회논문집
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• pp.377-381
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• 2006

본 논문에서는 노즐출구 단면에 설치된 메쉬 스크린을 이용하여 초음속 제트 소음 제어하기 위한 실험을 수행하였다. 메쉬 스크린은 미소 직경을 가진 스테인레스 철사들로 만들어졌으며 철망 형태이다. 노즐 압력비는 과팽창에서 부족팽창된 초음속 제트를 얻기 위해 다양하게 변화시켰다. 초기 제트 전단층을 교란하기 위해, 메쉬 스크린의 중앙 부분에 구멍을 만들었으며 그 구멍크기는 메쉬 스크린의 소음 저감효과를 조사하기 위해 변화시켰다. 유동장을 가시화하기 위해 쉴리렌 광학 장치를 사용하였고 OASPL과 소음 스펙트럼을 얻기 위해 음향을 측정하였다. 본 실험으로부터 얻어진 결과는 메쉬 스크린이 스크리치 톤을 상당히 억제하였으며, 메쉬 스크린의 구멍크기는 초음속 제트 소음을 저감하는 중요한 인자였다. 과팽창된 제트인 경우, 소음 저감효과는 적정팽창과 부족팽창된 제트에서의 저감효과보다 매우 크게 나타났다.

• 대한지리학회지
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• 제43권4호
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• pp.495-510
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• 2008

월귤은 극지 고산식물로 북극권과 고산대에 주로 자라며, 한반도에서는 북한의 고산대와 아고산대, 남한의 설악산 대청봉과 중청봉 사이 암석지, 귀때기청봉 등 아고산대 그리고 홍천의 산록에 자란다. 월귤이 격리 분포하는 강원도 홍천군 해발고도 350m 부근 애추 말단은 풍혈이다. 플라이스토세 빙하기에 널리 분포했던 월귤은 홀로세에 기후가 온난해지면서 한반도 북부와 중부의 고산대 및 아고산대와 함께 여름이 서늘한 홍천 풍혈 주위를 후빙기 피난처로 삼아 빙하기 유존종으로 격리 분포하게 되었다. 월귤의 남한계선이며 하한계선인 홍천에 자라는 군락은 가장 가까운 거리에 있는 설악산 아고산대와 1,200m의 해발고도 차이가 있으므로 빙하기의 기온은 현재보다 $6.6^{\circ}C$ 내외로 낮았던 것으로 추정된다 극지와 고산에 격리 분포하는 월귤은 여름 고온에 민감한 식물이다. 홍천의 산록에 자라는 월귤은 지구온난화에 따라 생리적으로 영향을 받거나 높은 온도를 좋아하는 식물과의 경쟁에 밀려 사라질 수도 있다. 한반도의 생물다양성 보전 차원에서 홍천의 월귤 군락지에 대한 보호 관리가 필요하다.

• Journal of Biosystems Engineering
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• 제27권4호
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• pp.341-348
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• 2002

Quality evaluation of red ginsengs is determined by outer shape and inner qualities. Especially, the inner qualities are main grading criteria. Currently, red ginsengs are classified into 3-grades; heaven, earth and good. The best heaven grade must not include inner holes and sponge tissues. This study was conducted to develop a red ginseng sorting system using x-ray image processing technique. Because of lens characteristic, gray values of the central region in the x-ray image are higher and gradually decreased towards the edge regions. This difference of gray values gives trouble in segmentation and detection of inner holes in red ginseng image, so preprocessing technique is necessary. The preprocessing was done by subtracting source image from an empty background image. But, simple subtraction was not quite appropriate because of too small contrast between inner holes and sound part. Scaled subtraction images were obtained by multiplying all gray values by some numbers. However this method could not help to set threshold value because the gray values of root part are generally lower than body part when red ginseng is exposed to the x-ray. To determine threshold value for detecting inner holes, an algorithm was developed by increasing overall gray values of less clear images.

• 대한기계학회논문집B
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• 제38권12호
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• pp.991-997
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• 2014

이 연구는 Gun식 가스버너의 스월유동장을 연소실과 화염이 없는 상태에서 직선형 5공압력프로브의 측정을 통해 고찰하였다. 직선형 5공압력프로브에 의한 속도 및 정압성분들은 넌널링 교정방법에 의해 연산하였으며, X형 열선프로브와 전산유체역학의 해석에 의한 결과들과 비교하였다. 결과적으로 Gun식 가스버너의 중심부에서 스월유동장에 대해 5공압력프로브에 의한 속도 및 정압의 측정값들은 비교적 X형 열선프로브에 의한 경우보다는 좋은 성능을 보였으나 전산유체역학의 해석에 의한 경우보다는 다소 미흡한 결과를 보였다.

• 한국산업융합학회 논문집
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• 제24권5호
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• pp.589-596
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• 2021

In this study, the optimum gating system was designed, and the two zinc alloy worm gears were manufactured in single process by applying a symmetrical gating system with 2 runners. The SRG ratio is set to 1 : 0.9 : 0.6, and the cross-sectional shapes such as sprue, runner and gate are designed. In order to determine whether the design of the gating system is appropriate, casting analysis was carried out. It takes 4.380 s to charge the casting 100%, 0.55 to 0.6 m/s at the gates and solidification begins after the casting is fully charged. The amount of air entrapment is 2% in the left gear and 6% in the right gear. Hot spots occurred in the center hole of the gear, and pores were found to occur around the upper part of the hole. Therefore, the design of the casting method is suitable for worm gears. CT analysis showed that all parts of worm gear were distributed with fine pores and some coarse pores were distributed around the central hole of worm gear. The yield strength and tensile strength were 220 MPa, 285 MPa, and the elongation rate was 8%. Vickers hardness is 82 HV.

• 한국컴퓨터정보학회논문지
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• 제14권4호
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• pp.111-117
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• 2009

무선 인터넷의 속도 향상과 휴대용 단말기의 컴퓨팅 파워 향상으로 이동 중에도 다양한 멀티미디어 서비스를 이용할 수 있게 되었다. 그러나, 휴대용 단말기를 통한 인터넷 사용을 위해서는 액세스 포인트(Access Point) 장비가 요구되고, 해당 장비에서는 동적으로 가상 네트워크 주소를 할당하는 방식을 사용하기 때문에, 휴대용 단말기간의 직접 통신이 요구되는 서비스 즉, 1:1 음성 또는 화상 통화 및 메신저 서비스 등은 거의 제공되지 않고 있는 실정이다. 또한 이러한 서비스를 제공하는 측에서도, 중앙에 중계 서버를 두어 단말에서 전송되는 패킷을 수집, 반대편 단말로 중계하도록 구현함으로써, 실시간 멀티미디어 데이터 등 대량의 데이터 전송이 요구되는 서비스에서는 중계 서버의 전송량과 이를 감당하기 위한 비용이 증가하게 되어, 실시간 대용량 데이터 전송 서비스는 제한적으로 제공되고 있는 실정이다. 이 연구에서는 TCP/UDP Hole Punching이라는 기술을 이용하여 휴대용 단말기나 가상 개인 네트워크 주소를 사용하는 장비들 간의 실시간 멀티미디어 데이터 직접 전송이 가능한 P2P서비스를 구현하였다.

• 천문학회보
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• 제45권1호
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• pp.59.2-59.2
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• 2020

Disks around protostars are the birthplace of planets. The first step toward planet formation is grain growth from ㎛-sized grains to mm/cm-sized grains in a disk, particularly in dense regions. In order to study whether grains grow and segregate at the protostellar stage, we investigate the ALMA Band 3 (3.1 mm) and 7 (0.87 mm) dust continuum observations of the protostellar disk WL 17 in ρ Ophiuchus L1688 cloud. As reported in a previous study, the Band 3 image shows substructures: a narrow ring and a large central hole. On the other hand, the Band 7 image shows different substructures: a non-axisymmetric ring and an off-center hole. The two-band observations provide a mean spectral index of 2.3, which suggests the presence of mm/cm-sized large grains. Its non-axisymmetric distribution may imply dust segregation between small and large grains. We perform radiative transfer modeling to examine the size and spatial distributions of dust grains in the WL 17 disk. The best-fit model suggests that large grains (>1 cm) exist in the disk, settling down toward the midplane, whereas small grains (~10 ㎛) well mixed with gas are distributed off-center and non-axisymmetrically in a thick layer. The low spectral index and the modeling results suggest that grains rapidly grow at the protostellar stage and that grains differently distribute depending on sizes, resulting in substructures varying with observed wavelengths. To understand the differential grain distributions and substructures, we discuss the effects of the protoplanet(s) expected inside the large hole and the possibility of gravitational instability.

• Korean Journal of Radiology
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• 제25권2호
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• pp.166-178
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• 2024

Objective: This study aimed to determine the predictive performance of non-contrast CT (NCCT) signs for hemorrhagic growth after intracerebral hemorrhage (ICH) when stratified by onset-to-imaging time (OIT). Materials and Methods: 1488 supratentorial ICH within 6 h of onset were consecutively recruited from six centers between January 2018 and August 2022. NCCT signs were classified according to density (hypodensities, swirl sign, black hole sign, blend sign, fluid level, and heterogeneous density) and shape (island sign, satellite sign, and irregular shape) features. Multivariable logistic regression was used to evaluate the association between NCCT signs and three types of hemorrhagic growth: hematoma expansion (HE), intraventricular hemorrhage growth (IVHG), and revised HE (RHE). The performance of the NCCT signs was evaluated using the positive predictive value (PPV) stratified by OIT. Results: Multivariable analysis showed that hypodensities were an independent predictor of HE (adjusted odds ratio [95% confidence interval] of 7.99 [4.87-13.40]), IVHG (3.64 [2.15-6.24]), and RHE (7.90 [4.93-12.90]). Similarly, OIT (for a 1-h increase) was an independent inverse predictor of HE (0.59 [0.52-0.66]), IVHG (0.72 [0.64-0.81]), and RHE (0.61 [0.54-0.67]). Blend and island signs were independently associated with HE and RHE (10.60 [7.36-15.30] and 10.10 [7.10-14.60], respectively, for the blend sign and 2.75 [1.64-4.67] and 2.62 [1.60-4.30], respectively, for the island sign). Hypodensities demonstrated low PPVs of 0.41 (110/269) or lower for IVHG when stratified by OIT. When OIT was ≤ 2 h, the PPVs of hypodensities, blend sign, and island sign for RHE were 0.80 (215/269), 0.90 (142/157), and 0.83 (103/124), respectively. Conclusion: Hypodensities, blend sign, and island sign were the best NCCT predictors of RHE when OIT was ≤ 2 h. NCCT signs may assist in earlier recognition of the risk of hemorrhagic growth and guide early intervention to prevent neurological deterioration resulting from hemorrhagic growth.