• 대한치과교정학회지
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• 제36권2호
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• pp.136-144
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• 2006

본 연구는 표준 경두개 방사선사진에서 나타나는 하악두/관절와의 위치 관계 및 형태 특징과 MRI에서 관찰되는 관절원판의 변위 여부를 비교함으로써 측두하악관절 내장증 평가 시 경두개 방사선사진의 임상적 이용 가능성을 알아보고자 하였다. 연구는 성인 환자 76명(남자 26명, 여자 50명)의 113개 악관절을 대상으로 하였다 MRI 자료를 기초로 하여 각 악관절을 정상군, 정복성 관절원판 변위군, 비정복성 관절원판 변위군으로 분류하였으며 최대 감합시의 경두개 방사선사진에서 관절와와 하악두 간의 전방, 후방 및 상방 직선 거리를 계측하여 상대적 위치 평가를 하고 형태적 특징을 판별하기 위해 악관절 경부와 두부간의 각도를 계측하였다. 또한 각 군에 따라 경두개 방사선 계측항목 간에 유의성 있는 차이가 있는지 알아보기 위해 일원분산분석과 다중비교분석을 시행하였다. 표준 경두개 방사선사진에서 나타나는 관절와와 하악두의 위치 관계는 관절원판 변위 여부 및 진행 정도와 상관성을 보이지 않았다. 또한 하악측두관절 경부와 하악두가 이루는 각도는 비정복성 관절원판 변위군에서 유의성 있게 증가하였다. 이는 하악두각이 악관절 내장증의 진행에 따른 악관절의 구조적인 경조직 변화를 반영한다고 볼 수 있으나 이것에만 근거하여 관절원판 변위 여부를 판단하기에는 근거가 미약하다.

• Imaging Science in Dentistry
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• 제31권3호
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• pp.159-164
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• 2001

Purpose: To evaluate the osseous changes of TMJ in internal derangement and osteoarthritis patients using MRI. Materials and Methods: MR images of 111 TMJs in 64 patients were analyzed to evaluate the osseous changes, 111 TMJs were divided into 6 groups according to the radiologic Stages by Schellhas and Wilkes. On MR images, we evaluate the osseous changes of articular eminence and condylar head. Results: The most frequent Stage in internal derangement of TMJ was Stage I. And 28 joints (25.2%) revealed osteoarthritis with internal derangement. When osseous change of articular eminence and condylar head occur, flattening was the most common osseous change. Sclerosis was observed in all Stages and osteophytosis of condylar head was observed in Stage II (1.8%) and III (0.9%). Out of 28 joints with osteoarthritis, 6 joints (21.4%) showed joint effusion. Conclusion: MR image revealed abnormal configuration of disk, but the detection of minimal osseous change was subtle.

• 천문학회보
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• 제36권1호
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• pp.35.2-35.2
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• 2011

We have investigated a coronal jet near the limb on 2010 June 27 by Hinode/X-Ray Telescope (XRT), EUV Imaging Spectrograph (EIS), SDO/Atmospheric Imaging Assembly (AIA), and STEREO. From EUV (AIA and EIS) and soft X-ray (XRT) images we identify the erupting jet feature in cool and hot temperatures. Using the high temporal and multi wavelength AIA images, we found that the hot jet preceded its associated cool jet and their structures are well consistent with the numerical simulation of the emerging flux-reconnection model. From the spectroscopic analysis, we found that the jet structure changes from blue shift to red one with time, which may indicate the helical structure of the jet. The STEREO observation, which enables us to observe this jet on the disk, shows that there was a dim loop associated with the jet. On the other hand, we found that the structure of its associated active region seen in STEREO is similar to that in AIA observed 5 days before. Based on this fact, we compared the jet morphology on the limb with the magnectic fields extrapolated from a HMI vector magnetogram of this active region observed on the disk. Interestingly, the comparison shows that the open and closed magnetic field configuration correspond to the jet and the dim loop, respectively, as the Shibata's jet model predicted.

• Journal of Yeungnam Medical Science
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• 제12권1호
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• pp.141-148
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• 1995

본 교실에서는 측두하악관절주위의 동통, 관절 잡음동의 증상을 주소로 내원한 환자들에 있어서 역동적 자기공명영상의 촬영을 시행하여 관절원판의 전방변위와 형태적 이상 및 주위 구조물들과의 관계를 분석한 결과 근육성 동통기능장애와의 감별뿐만 아니라 환자의 중상에 따른 관절 내부 장애의 정도를 파악할 수 있었으며 악기능시의 구조적 이상, 장애의 원인 등을 판독하여 치료의 방침을 세우는데 있어 매우 유용한 정보를 얻을 수 있었기에 보고 하는 바이다.

• Journal of Mechanical Science and Technology
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• 제15권12호
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• pp.1691-1698
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• 2001

In recent years, significant progress has been made in modeling turbulence behavior in plasma and its effect on transport. It has also been made in diagnostics for turbulence measurement; however, there is still a large gap between theoretical model and experimental measurements. Visualization of turbulence can improve the connection to theory and validation of the theoretical model. One method to visualize the flow structures in plasma is a laser Schlieren imaging technique. We have recently applied this technique and investigated the characteristics of a highly underexpanded pulsed plasma jet originating from an electrothermal capillary source. Measurements include temporally resolved laser Schlieren imaging of a precursor blast wave. Analysis on the trajectory of the precursor blast wave shows that it does not follow the scaling expected for a strong shock resulting from the instantaneous deposition of energy at a point. However, the shock velocity does scale as the square root of the deposited energy, in accordance with the point deposition approximation.

• 천문학회지
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• 제38권2호
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• pp.219-222
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• 2005

We present the high-resolution (2"-4") images of the molecular envelopes surrounding the evolved stars, V Hya, VY CMa, and ${\pi}^1$ Gru observed with the Submillimeter Array. The CO J=2-1 and 3-2 images of the carbon star V Hya show that the circumstellar structure of this star consists of three kinematic components; there is a flattened disk-like envelope that is expanding with a velocity of ${\~}16 km\;s^{-1}$, the second component is the medium-velocity wind having a deprojected velocity of 40-120 km $s^{-l}$ moving along the disk plane, and the third one is the bipolar molecular jet having an extreme velocity of 70-185 km $s^{-l}$. The axis of this high velocity jet is perpendicular to the plane of the disk-like envelope. We found that the circumstellar structure of the S-star ${\pi}^1$ Gru traced by the CO J =2-1 resembles that of V Hya quite closely; the star is surrounded by the expanding disk-like envelope and is driving the medium-velocity wind along the disk plane. We also obtained the excellent images of VY CMa with the CO and $^{13}CO$ J=2-1 and $SO\;6_5-5_4$ lines. The maps of three molecular lines show that the envelope has a significant velocity gradient in the east-west direction, suggesting that the envelope surrounding VY CMa is also flattened and expanding along its radial direction. The high-resolution images obtained with the SMA show that some AGB stars are associated with the asymmetric mass loss including the equatorial wind and bipolar jet.

• 정보보호학회논문지
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• 제26권4호
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• pp.911-919
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• 2016

과거에 비해 현재의 디스크 저장 공간은 비약적으로 증가하고 있으며, 네트워크상에서도 이전과 비교할 수 없는 수많은 데이터들이 처리되고 있다. 이러한 데이터의 대용량화는 앞으로도 계속 될 추세이지만, 그에 비해 포렌식 관점에서 데이터를 이미징 하는 시간을 개선시키기 위한 연구는 부족한 상황이다. 본 논문은 데이터 이미징 시간을 개선시키기 위한 방안으로 전체 이미징 소요시간 중 해시함수에 대한 소요시간을 암호학적 관점에서 살펴보고, 이를 토대로 EWF 파일 이미징 과정에 대한 효율성 개선 방안을 제안한다.

• 천문학회지
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• 제38권2호
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• pp.73-75
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• 2005

The latest scientific highlights obtained with the Subaru telescope are given together with its current status and on-going instrumentation. We have been successfully operating the telescope and 8 observatory instruments (including an adaptive optics system) since January 1999, when the first light was accomplished. Open-use of Subaru began in December 2000. Subaru has a unique capability of its prime focus among other 8-10 meter class telescopes and has an excellent imaging performance as a result of its sophisticated active optics combined with the high stability of the sky at Mauna Kea. Scientific highlights are given on the discoveries of the most distant galaxies, spiral structure on a protoplanetary disk around AB Aur, and planetesimal belts in the debris disk around $\beta$ Pic. Brief summaries are given for three new instruments: the Multi-Object Infrared Camera and Spectrograph (MOIRCS), 188 element adaptive optics system, and Fiber Multi-Object Spectrograph (FMOS)

• 천문학논총
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• 제30권2호
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• pp.513-515
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• 2015

We investigate $H\small{I}$ data for a pair of blue compact dwarf galaxies (BCDs), ESO 435-IG20 and ESO 435-IG16, obtained with the Australia Telescope Compact Array. The outer $H\small{I}$ disk is highly disturbed and asymmetric in both galaxies showing a gas tail and/or a broad/extended gas disk on only one side. Based on their low-density surroundings and small projected distance (<80 kpc) at a similar redshift, we conclude that tidal interaction between these two BCDs is responsible for the morphological and kinematical peculiarities in $H\small{I}$. We also investigate their star formation rates using $H{\alpha}$ and UV imaging data to probe their interaction history.

• Journal of Astronomy and Space Sciences
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• 제21권4호
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• pp.329-342
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• 2004

In this paper, we present preliminary feasibility studies on three types of solar observation payloads for future Korean Science and Technology Satellite (STSAT) programs. The three candidates are (1) an UV imaging telescope, (2) an UV spectrograph, and (3) an X-ray spectrometer. In the case of UV imaging telescope, the most important constraint seems to be the control stability of a satellite in order to obtain a reasonably good spatial resolution. Considering that the current pointing stability estimated from the data of the Far ultraviolet Imaging Spectrograph (FIMS) onboard the Korean STSAT-1, is around 1 arc minutes/sec, we think that it is hard to obtain a spatial resolution sufficient for scientific research by such an UV Imaging Telescope. For solar imaging missions, we realize that an image stabilization system, which is composed of a small guide telescope with limb sensor and a servo controller of secondary mirror, is quite essential for a very good pointing stability of about 0.1 arcsec. An UV spectrograph covering the solar full disk seems to be a good choice in that there is no risk due to poor pointing stability as well as that it can provide us with valuable UV spectral irradiance data valuable for studying their effects on the Earth's atmosphere and satellites. The heritage of the FIMS can be a great advantage of developing the UV spectrograph. Its main disadvantage is that two major missions are in operation or scheduled. Our preliminary investigations show that an X-ray spectrometer for the full disk Sun seems to be the best choice among the three candidates. The reasons are : (1) high temporal and spectral X-ray data are very essential for studying the acceleration process of energetic particles associated with solar flares, (2) we have a good heritage of X-ray detectors including a rocket-borne X-ray detector, (3) in the case of developing countries such as India and Czech, solar X-ray spectrometers were selected as their early stage satellite missions due to their poor pointing stabilities, and (4) there is no planned major mission after currently operating Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) mission. Finally, we present a preliminary design of a solar X-ray spectrometer covering soft X-ray (2 keV) to gamma ray (10 MeV).