• 천문학회보
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• 제42권2호
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• pp.39.2-39.2
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• 2017

Over the last decade, deep studies of nearby galaxies have led to the discovery of vast stellar envelopes that are often rich in substructure. These components are naturally predicted in models of hierarchical galaxy assembly, and their observed properties place important constraints on the amount, nature, and history of satellite accretion. One of the most effective ways of mapping the peripheral regions of galaxies is through resolved star studies. Using wide-field cameras equipped to 8 m class telescopes, it has recently become possible to extend these studies to systems beyond the Local Group. Located at a distance of 3.6 Mpc, M81 is a prime target for wide-field mapping of its resolved stellar content. In this talk, we present the detailed results from our deep wide-field imaging survey of the M81 group with the Hyper Suprime-Cam (HSC), on the Subaru Telescope. We report on the analysis of the structures, stellar populations, and metallicities of old dwarf galaxies such as NGC3077, IKN, KDG061, as well as young stellar systems such as Arp's Loop and Holmberg IX. Several candidates for yet-undiscovered faint dwarf galaxies and young stellar clumps in the M81 group will also be introduced. The peculiar galaxy NGC3077 has been classified as the irregular galaxy. Okamoto et al. (2015, ApJ 809, L1) discovered an extended halo structure with S-shape elongated tails, obvious feature of tidal interaction. With a help of numerical simulation by Penarrubia et al. (2009, ApJ 698, 222), we will demonstrate that this tidal feature was formed during the latest close encounters between M81, M82, and NGC 3077, which induced star formation in tidally stripped gas far from the main bodies of galaxies. It is not clear whether the latest tidal interaction was the first close encounters of three galaxies. If NGC3077 is still surrounded by the dark matter halo, it implies that NGC3077 has undergone the first tidal stripping by larger companions. Kinematic studies of inter galactic globular clusters and planetary nebulae would tell us the past history of tidal interaction in this group of galaxies.

• Applied Microscopy
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• 제45권4호
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• pp.225-229
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• 2015

Transition metal dichalcogenides (TMDs) are a class of two-dimensional (2D) materials that have attracted growing interest because of their promising applications. The properties of TMDs strongly depend on the crystalline structure and the number and stacking sequence of layers in their crystals and thin films. Though electrical, mechanical, and magnetic studies of 2D materials are being conducted, there is an evident lack of direct atom-by-atom visualization, limiting insight on these highly exciting material systems. Herein, we present our recent studies on the characterization of 2D layered materials by means of aberration corrected scanning transmission electron microscopy (STEM), in particular via high angle annular dark field (HAADF) imaging. We have identified the atomic arrangements and defects in 2H stacked TMDs, 1T stacked TMDs, distorted 1T stacked TMDs, and vertically integrated heterojunctions of 2D TMDs crystals.

• 대한방사선치료학회지
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• 제27권2호
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• pp.167-174
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• 2015

목 적 : 복잡하고 정교하게 계획된 용적변조회전 방사선치료(Volumetric Arc Therapy, VMAT)의 Portal Dosimetry를 이용한 치료 전 선량평가가 다양한 인자에 따라 재현성을 유지하는지 분석하고자 하였다. 대상 및 방법 : 실험에는 TrueBeam STx$^{TM}$(Ver.1.5, Varian, USA), Portal dosimetry application(Ver.10, Varian)과 Portal Vision aS1000 Imager(Varian, USA)을 사용하였다. 두경부암 환자 2명, 전립샘암 환자 3명, 폐암 환자 1명, 자궁경부암 환자 1명, 총 7명의 환자에 대하여 Portal Dosimetry용 VMAT 전산화치료계획(Eclipse, Ver.10.0, Varian, USA)을 수립하였다. 오전 치료 전과 후 오후 치료 종료 후 각 4시간 간격을 두고 3회씩 5일에 걸쳐 선량평가를 시행하였다. Gamma pass rate(GPR 3%, 3mm 95%신뢰구간)와 Beam 출력의 상관관계를 확인하기 위하여 선량평가 시행 전 Beam 출력 을 물등가모형과 이온전리함(IBA dosimetry, Germany)을 이용하여 측정하였다. Electronic Portal Imaging Device(EPID) 상태에 따른 GPR 의 변화를 확인하기 위하여 EPID의 영상 교정 (Dark field correction, Flood field correction) 전과 후로 나누어 선량평가를 시행하였다. 또한 다엽콜리메이터(Multi Leaf Collimator) 상태에 따른 GPR의 변화를 확인하기 위해 다엽콜리메이터 Initialize 전과 후로 나누어 선량평가를 시행하였다. 결 과 : Portal Dosimetry를 시행하여 얻은 모든 환자들의 각 시간대 별 GPR의 평균값은 97.11%, 96.09%, 95.37% 였고 최대 차이를 보인 환자의 경우 각 시간대 별 GPR의 평균값은 95.73%, 94.20% 93.23% 였다. 선량평가 시점의 Beam 출력을 측정한 결과 각 시간대별 평균값은 100.45%, 100.46%, 100.59% 였다. EPID의 영상 교정(Dark field correction, Flood field correction)을 시행하기 전과 후의 대상 환자들의 GPR의 평균값은 95.94 %, 96.01% 였다. 또한 다엽콜리메이터 의 Initialize 를 시행하기 전과 후의 대상 환자들의 GPR 의 평균값은 95.83%, 96.40%였다. 결 론 : 치료기 사용시간이 경과됨에 따라 대상 환자들의 GPR 평균값이 0.8% 감소함을 확인할 수 있었다. Beam 출력은 각 측정시점에 0.1% 오차범위 안에서 일정한 상태를 유지하였다. EPID의 영상 교정 전, 후 의 선량평가 결과 GPR은 평균 0.1% 차이를 나타내었다. 다엽콜리메이터의 Initialize 전, 후의 선량평과 결과 Initialize 시행 후 GPR이 평균 0.6% 상승하였고 다엽콜리메이터 상태에 따라 GPR이 변화할 수 있다는 것을 확인할 수 있었다. 복잡하고 정교하게 계획된 VMAT의 치료 전 선량평가 도구로서 재현성을 유지하며 Portal Dosimetry를 이용하기 위해서는 주기적인 장비의 점검뿐만 아니라, 선량평가에 영향을 미칠 수 있는 다양한 인자들에 대한 관리가 이뤄져야 할 것으로 판단된다.

• 천문학회보
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• 제36권1호
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• pp.37.2-37.2
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• 2011

Our previous study on tiny pores (R < 2") observed by HINODE/Solar Optical Telescope (SOT) revealed that the plasma in the pores at the photosphere is always moving down and the pores are surrounded by the strong downward motions (highly red-shifted) of neighboring granulations. From this study, we speculated that the flow motions above the pore should be related with the motions at the photosphere, since the pore is strong magnetic field region. Meanwhile, SNU and KASI installed Fast Imaging Solar Spectrograph (FISS) in the Cude room of the 1.6 m New Solar Telescope (NST) at Big Bear Solar Observatory. FISS is a unique system that can do imaging of H-alpha and Ca II 8542 band simultaneously, which is quite suitable for studying of dynamics of chromosphere. To get some clue on the relationship between the photospheric and low-chromospheric motions at the pore region, we took a coordinate observation with NST/FISS and Hinode/SOT for new emerging active region (AR11117) on October 26, 2010. In the observed region, we could find two tiny pores and two small magnetic islands (SMIs), which have similar magnetic flux with the pores but does not look dark. Magnetic flux density and Doppler velocities at the photosphere are estimated by applying the center-of-gravity (COG) method to the HINODE/spectropolarimeter (SP) data. The line-of-sight motions above the photosphere are determined by adopting the bisector method to the wing spectra of Ha and CaII 8542 lines. As results, we found the followings. (1) There are upflow motion on the pores and downflow motion on the SMIs. (2) Towards the CaII 8542 line center, upflow motion decrease and turn to downward motion in pores, while the speed of down flow motion increases in the SMIs. (3) There is oscillating motion above pores and the SMIs, and this motion keep its pattern along the height. (4) As height increase, there is a general tendency of the speed shift to downward on pores and the SMIs. This is more clearly seen on the other regions of stronger magnetic field. In this talk, we will present preliminary understanding of the coupling of pore dynamics between the photosphere and the low-chromosphere.

• 천문학회보
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• 제37권2호
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• pp.111.2-111.2
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• 2012

We observed an Ellerman bomb(EB) and its associated surge using the Fast Imaging Solar Spectrograph(FISS) and the broadband TiO filter of the 1.6 meter New Solar Telescope at Big Bear Solar Observatory. As is well-known, the EB appears as a feature that is very bright at the far wings of the H alpha line. The lambdameter method applied to these wings indicates that the EB is blue-shifted up to 6km/s in velocity. In the photospheric level below the EB, we see rapidly growing "granule-like" feature. The transverse velocity of the dark lane at the edge of the "granule" increased with time as reached a peak of 6km/s, at the time of the EB's occurrence. The surge was seen in absorption and varied rapidly both in the H alpha and the Ca II 8542 line. It originated from the Ellerman bomb, and was impulsively accelerated to 20km/s toward us(blueshift). Then the velocity of the surge gradually changed from blueshift of 20km/s to redshift of 40km/s. By adopting the cloud model, we estimated the temperature of the surge material at about 27000K and the non-thermal velocity at about 10km/s. Our results shed light on the conventional idea that an EB results from the magnetic reconnection of an emerging flux tube and pre-existing field line.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2013년도 제44회 동계 정기학술대회 초록집
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• pp.334-334
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• 2013

In the past decade, the infrared detectors based on intersubband transition in quantum dots (QDs) have attracted much attention due to lower dark currents and increased lifetimes, which are in turn due a three-dimensional confinement and a reduction of scattering, respectively. In parallel, focal plane array development for infrared imaging has proceeded from the first to third generations (linear arrays, 2D arrays for staring systems, and large format with enhanced capabilities, respectively). For a step further towards the next generation of FPAs, it is envisioned that a two-dimensional metal hole array (2D-MHA) structures will improve the FPA structure by enhancing the coupling to photodetectors via local field engineering, and will enable wavelength filtering. In regard to the improved performance at certain wavelengths, it is worth pointing out the structural difference between previous 2D-MHA integrated front-illuminated single pixel devices and back-illuminated devices. Apart from the pixel linear dimension, it is a distinct difference that there is a metal cladding (composed of a number of metals for ohmic contact and the read-out integrated circuit hybridization) in the FPA between the heavily doped gallium arsenide used as the contact layer and the ROIC; on the contrary, the front-illuminated single pixel device consists of two heavily doped contact layers separated by the QD-absorber on a semi-infinite GaAs substrate. This paper is focused on analyzing the impact of a two dimensional metal hole array structure integrated to the back-illuminated quantum dots-in-a-well (DWELL) infrared photodetectors. The metal hole array consisting of subwavelength-circular holes penetrating gold layer (2DAu-CHA) provides the enhanced responsivity of DWELL infrared photodetector at certain wavelengths. The performance of 2D-Au-CHA is investigated by calculating the absorption of active layer in the DWELL structure using a finite integration technique. Simulation results show the enhanced electric fields (thereby increasing the absorption in the active layer) resulting from a surface plasmon, a guided mode, and Fabry-Perot resonances. Simulation method accomplished in this paper provides a generalized approach to optimize the design of any type of couplers integrated to infrared photodetectors.

• 한국방사선학회논문지
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• 제8권7호
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• pp.383-387
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• 2014

본 연구에서는 선형가속기의 소조사면에 보다 정확한 선량계측이 가능하고, 빔 분포 영상화가 가능 계측시스템 개발을 위해 반도체화합물을 이용한 검출 센서를 제작하여 성능평가를 하였다. 센서 제작은 대면적 필름 형성을 위해 입자침전법을 이용하였다. 고에너지 X선에 대한 검출 특성은 암전류, 출력전류, 상승시간, 하강시간, 응답지연 측정을 통해 조사되었다. 측정 결과, $TiO_2$가 혼합된 $HgI_2$ 센서가 $PbI_2$, PbO, $HgI_2$ 보다 우수한 특성을 보였다. 선형가속기를 이용하여 선형성, 재현성 및 정확성 평가를 수행하였으며, 결과적으로 실제 임상에 적용되고 있는 선량 검출기와 감응 특성을 비교 시 재현성, 선형성 및 정확성 등에서 매우 우수한 특성을 나타내는 것을 확인할 수 있었다.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2014년도 제46회 동계 정기학술대회 초록집
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• pp.324-325
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• 2014

Quantum wells infrared photodetectors (QWIPs) have been used to detect infrared radiations through the principle based on the localized stated in quantum wells (QWs) [1]. The mature III-V compound semiconductor technology used to fabricate these devices results in much lower costs, larger array sizes, higher pixel operability, and better uniformity than those achievable with competing technologies such as HgCdTe. Especially, GaAs/AlGaAs QWIPs have been extensively used for large focal plane arrays (FPAs) of infrared imaging system. However, the research efforts for increasing sensitivity and operating temperature of the QWIPs still have pursued. The modification of heterostructures [2] and the various fabrications for preventing polarization selection rule [3] were suggested. In order to enhance optical performances of the QWIPs, double barrier quantum well (DBQW) structures will be introduced as the absorption layers for the suggested QWIPs. The DBWQ structure is an adequate solution for photodetectors working in the mid-wavelength infrared (MWIR) region and broadens the responsivity spectrum [4]. In this study, InGaAs/GaAs/AlGaAs double barrier quantum well infrared photodetectors (DB-QWIPs) are successfully fabricated and characterized. The heterostructures of the InGaAs/GaAs/AlGaAs DB-QWIPs are grown by molecular beam epitaxy (MBE) system. Photoluminescence (PL) spectroscopy is used to examine the heterostructures of the InGaAs/GaAs/AlGaAs DB-QWIP. The mesa-type DB-QWIPs (Area : $2mm{\times}2mm$) are fabricated by conventional optical lithography and wet etching process and Ni/Ge/Au ohmic contacts were evaporated onto the top and bottom layers. The dark current are measured at different temperatures and the temperature and applied bias dependence of the intersubband photocurrents are studied by using Fourier transform infrared spectrometer (FTIR) system equipped with cryostat. The photovoltaic behavior of the DB-QWIPs can be observed up to 120 K due to the generated built-in electric field caused from the asymmetric heterostructures of the DB-QWIPs. The fabricated DB-QWIPs exhibit spectral photoresponses at wavelengths range from 3 to $7{\mu}m$. Grating structure formed on the window surface of the DB-QWIP will induce the enhancement of optical responses.

• 비파괴검사학회지
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• 제26권4호
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• pp.211-219
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• 2006

초음파 서모그라피는 초음파 진동 에너지 여기에 의한 물체의 표면 및 표면 아래에 존재하는 결함부위의 선택적 발열 특성을 적외선 열영상 카메라로 관측하는 것이다. 결함(균열, 박리, 공극 등) 이 존재하는 구조물에 초음파 진동 에너지를 입사시킬 경우 결함 부근에서의 국부적인 발열로 인해 건전 부위와의 급격한 온도차를 드러내는 핫 스폿이 관측된다. 초음파 진동 에너지 여기에 의한 핫 스폿 관측 및 분석을 통해 결함을 진단하는 것이 초음파 서모그라피를 이용한 비파괴 결함 진단 방법이다. 이를 이용한 결함 검출을 위해서는 초음파의 진동에너지를 검사 구조물에 효율적으로 전달하는 것이 중요하다 본 논문에서는 초음파 서모그라피를 이용한 실시간 결함검출에 대해 기술한다. 초음파 진동에너지의 입사 방향에 따른 결함 검출 특성을 평가하기 위해 진동에너지의 전달 방향을 시편과 수직 또는 수평방향으로 각각 입사시켰다. 각각의 입사 방향에 따른 초음파 트랜스듀서 양단에 인가되는 전압을 디지털 오실로스코우프로 계측 비교하였다. 결함 검출에 사용한 시편은 14 mm 두께의 SUS 균열(crack) 시편, PCB 기판(1.8 mm), 인코넬 600 판(1.0 mm) 및 CFRP 판(3.0 mm)의 4종류이다. 4종류의 시편에 대해 280ms 펄스폭의 초음파에너지를 수직 수평으로 각각 입사시켰다. 4종류 모두 수직방향으로 초음파 진동에너지를 입사시켰을 때 수평방향에 비해 전달 손실이 적었다. 복합재료인 PCB, CFRP 판은 수직방향으로 초음파 진동에너지를 입사시켰을 때 수평방향에 비해 결함 위치에서 열이 크게 발생하였으며 선택적 발열 현상도 3배 이상 지속되었다. 금속재료인 인코넬 600판과 SUS 시편은 수평방향이 수직방향보다 핫 스폿이 빨리 관측되었다.