• 한국진공학회:학술대회논문집
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• 한국진공학회 2009년도 제38회 동계학술대회 초록집
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• pp.379-379
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• 2010

Recent technical advances in OLEDs (organic light emitting devices) requires more and more the improvement in low operation voltage, long lifetime, and high luminance efficiency. Inverted top emission OLEDs (ITOLED) appeared to overcome these problems. This evolved to operate better luminance efficiency from conventional OLEDs. First, it has large open area so to be brighter than conventional OLEDs. Also easy integration is possible with Si-based driving circuits for active matrix OLED. But, a proper buffer layer for carrier injection is needed in order to get a good performance. The buffer layer protects underlying organic materials against destructive particles during the electrode deposition and improves their charge transport efficiency by reducing the charge injection barrier. Hexaazatriphenylene-hexacarbonitrile (HAT-CN), a discoid organic molecule, has been used successfully in tandem OLEDs due to its high workfunction more than 6.1 eV. And it has the lowest unoccupied molecular orbital (LUMO) level near to Fermi level. So it plays like a strong electron acceptor. In this experiment, we measured energy level alignment and hole current density on inverted OLED structures for hole injection. The normal film structure of Al/NPB/ITO showed bad characteristics while the HAT-CN insertion between Al and NPB greatly improved hole current density. The behavior can be explained by charge generation at the HAT-CN/NPB interface and gap state formation at Al/HAT-CN interface, respectively. This result indicates that a proper organic buffer layer can be successfully utilized to enhance hole injection efficiency even with low work function Al anode.

• Spatial Information Research
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• 제8권2호
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• pp.301-315
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• 2000

지반조사 자료는 구조물을 시공하거나 설계하기 위해 필요한 기본자료이며 지층의 구성, 토질의 종류 등 기반을 구별하는 정보를 포함한다. 매년 대량으로 발생하는 지반조사 자료들은 현장의 특성을 정확하게 반영하기 때문에 지반조사 자료를 이용하여 지반을 분석한다면, 기존의 지질도나 토양도보다 뛰어난 결과를 얻을 수 있다. 따라서 비균질하고 비정형화된 지반의 특성을 고려하여 서로구별하는 특징을 추출하고, 현장의 특성을 정확하게 반영하는 지반분석 시스템이 필요하다. 본 논문은 지반조사 정보 시스템이 관리하고 있는 시추공의 지층구성 정보와 위치 근접성을 바탕으로 시추공을 클러스터링하여 지반의 구성을 분석하는 지반분석시스템의 설계 및 구현에 대해 전반적으로 기술하였다. 개발된 지반분석시스템은 지반조사 데이터베이스의 시추공 정보를 이용하여 지반이 가지고 있는 특성 정보를 추출하고, 이를 이용하여 유사한 특성 및 위치 근접성을 갖는 시추공의 집합으로 클로스터링하여 사용자에게 정확한 지반구성 정보를 제공하는 시스템이다. 또한, 수치지도의 사용으로 지리적 위치와 지역·지형에 대한 지반구조의 특성조사를 가능하게 하며, 지반조사를 필요로 하는 지역에 대한 지반의 유추가 가능하여 경제적 효과를 볼 수 있다. 따라서, 지반조사 데이터로부터 다양한 종류의 정보를 얻을 수 있으며 지질도나 토양도보다 정확한 지반특성을 제공할 수 있다.

• 천문학회지
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• 제50권5호
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• pp.151-155
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• 2017

We investigate the radio properties of the dwarf galaxy SDSS J133245.62+263449.3 which shows optical signatures of black hole activity. Dwarf galaxies are known to host intermediate mass black holes (IMBHs) with masses $M_{BH}{\sim}10^{4-6}M_{\odot}$, some of them being radio loud. Recently, Reines et al. (2013) found dwarf galaxy candidates which show signatures of being black hole hosts based on optical spectral lines. SDSS J133245.62+263449.3 is one of them; it shows a flux density of ~ 20 mJy at 1.4 GHz, which corresponds to $L_{1.4GHz}{\sim}10^{23}W\;Hz^{-1}$. This is much brighter than other black hole host dwarf galaxies. However, star formation activity can contribute to radio continuum emission as well. To understand the nature of the radio emission from SDSS J133245.62+263449.3, we imaged this radio loud dwarf galaxy at low frequencies (325 MHz and 610 MHz) using the Giant Metrewave Radio Telescope (GMRT). We present here the high resolution images from our GMRT observations. While we detect no obvious extended emission from radio jets from the central AGN, we do find the emission to be moderately extended and unlikely to be dominated by disk star formation. VLBI observations using the Korean VLBI Network (KVN) are now being planned to understand the emission morphology and radiation mechanism.

• 한국재료학회지
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• 제11권6호
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• pp.441-447
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• 2001

PACVD 방법으로 다이캐스팅용 금형에 적용할 수 있는 TiN 코팅막을 형성시키는 연구를 하였다. 직류 펄스전원을 사용하여 지름이 4 mm인 작은 동공내부에 최고 20 mm 깊이까지 균일한 TiN 코팅층을 형성할 수 있었다. 코팅공정시 발광분광분석기를 사용해 Ti와 $N_{2}$ 및 $Ar^{+}$의 분광선을 측정함으로써 TiN 코팅막의 형성기구에 대하여 고찰하였다. 듀티비율이 50% 이상인 경우는 Ti, $N_{2}^{+}$ 및 $Ar^{+ }$ 의 분광선이 나타났으나, 듀터비율이 28.6%이하인 경우 분광선이 전혀 나타나지 않았으며 TiN 코팅층의 형성도 불안정하였다. 펄스전원으로 Bipolar로 사용한 경우 Unipolar를 사용한 경우보다 지름이 4 mm인 구멍에서 2배 깊게 코팅되었다.

• 한국산학기술학회논문지
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• 제11권3호
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• pp.815-820
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• 2010

본 연구에서는 자동차용 가솔린엔진에 장착되는 인젝터의 연료공급 특성을 실험적으로 분석하였다. 4홀과 12홀 인젝터의 장착각 변화와 포트 마스킹의 형상변화에 따른 벽유량을 측정하고 분석하였다. 분무가시화 실험을 통하여 분무성장과정과 분사각, 연료미립화 및 분무도달거리를 분석하였다. 벽류측정 실험 결과, 벽유량은 흡기유동과 인젝터 장착각에 큰 영향을 받으며, 인젝터 장착각이 감소할수록 벽유량은 감소하였다. 마스킹의 경우 유동 면적이 감소하여 국소 유속이 증가할때 벽유량 감소에 효과를 보였다. 분무 가시화를 통하여 12홀 인젝터가 압력 변화에 대한 미립화의 강건성 측면에서 우수한 분무특성을 보였다.

• 한국정밀공학회지
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• 제18권10호
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• pp.200-207
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• 2001

Burrs farmed in drilling are classified into three types, no burr, burrs with cap, teared burr. To control burr size in drilling, the second type burrs with cap are to be formed because it is small and uniform. It is necessary to understand the mechanism of cap formation to derive the burr formation into second type burr with cap. In several materials. second type burrs are formed in drilling by changing cutting conditions. It is observed that cap is formed as a result of the plastic deformation along the outside of exit hope. According to the tension behavior of the material in concentrated region between hole and drill outside edge, the geometry of burr with cap is determined. Simplified 2D FEM analysis shows good prediction for burr formation.

• 한국소성가공학회:학술대회논문집
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• 한국소성가공학회 2009년도 추계학술대회 논문집
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• pp.227-230
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• 2009

In order to predict failure behavior of advanced high-strength steel sheets (AHSS) in hole expansion tests, damage model was developed considering surface condition sensitivity (with specimens prepared by milling and punching: 340R, TRIP590, TWIP940). To account for the micro-damage initiation and evolution as well as macro-crack formation, the stress triaxiality dependent fracture criterion and rate-dependent hardening and ultimate softening behavior were characterized by performing numerical simulations and experiments for the simple tension and V-notch tests. The developed damage model and the characterized mechanical property were incorporated into the FE program ABAQUS/Explicit to perform hole expansion simulations, which showed good agreement with experiments.

• 한국정밀공학회지
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• 제30권3호
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• pp.278-283
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• 2013

While Built-in Spindle is working in machining center, the tool is changed by ATC(Automatic Tool Changer) automatically. However, impurities could be stacked in front of spindle because of chips formation while machining, and positional error between spindle and tool could be generated. Compressed air holes are necessary for removal of the impurities. But, the diameter and number of compressed air hole are different for each built-in spindle in market. In this paper, flow analysis is carried out to find out the efficient figuration of the compressed air hole by using velocity and pressure distributions.

• 한국지구물리탐사학회:학술대회논문집
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• 한국지구물리탐사학회 2003년도 Proceedings of the international symposium on the fusion technology
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• pp.432-436
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• 2003

Geophysical well logging techniques which are useful for delineating permeability of geological formation have been reviewed. A new technique for obtaining permeability using conductivity log technique has been discussed. This conductivity logging technique has been tested by monitoring the conductivity change within the model hole using borehole environment water and incoming-outgoing water of different salinity with constant flow rate by maintaining balance between inflow and outflow. Conductivity variation features depended mainly on flow rate, density contrasts due to salinity and temperature contrasts between fluid within the hole and incoming-outgoing fluid. The results of the experiment show uniform change of fluid conductivity within bore hole with time, and a fairly good correlation between the flow rate and the conductivity change rate. This conductivity logging technique is expected to be an efficient tool for determining permeability.

• 천문학회지
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• 제23권1호
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• pp.63-70
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• 1990

The original axisymmetric, stationary electrodynamic model of the central engine in an active galactic nucleus proposed by Macdonald and Thorne consists of a supermassive black hole with magnetic field lines that pass through the region just outside the event horizon of the black hole. Each magnetic field line rotates with a constant angular velocity which will exceed the speed of light at large radii. Even though the field lines are purely mathematical entities this condition sets a stringent physical constraint on the motion of the magnetic field lines and the particles on them. In this paper we will show that we can remove this auxiliary constraint in our model by allowing nonstationary processes. As a result the magnetic field lines can be twisted and wound up in a region lying outside of the quasi-stationary magnetosphere of the black hole. We conclude that astrophysical jets are formed in that region due to the twisted and wound magnetic field lines powered by the Blandford-Znajek process and the other driving forces.