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Influence of Lithiation on Nanomechanical Properties of Silicon Nanowires Probed with Atomic Force Microscopy

  • Lee, Hyun-Soo;Shin, Weon-Ho;Kwon, Sang-Ku;Choi, Jang-Wook;Park, Jeong-Young
    • 한국진공학회:학술대회논문집
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    • 한국진공학회 2011년도 제41회 하계 정기 학술대회 초록집
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    • pp.110-110
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    • 2011
  • The nanomechanical properties of fully lithiated and unlithiated silicon nanowire deposited on silicon substrate have been studied with atomic force microscopy. Silicon nanowires were synthesized using the vapor-liquid-solid process on stainless steel substrates using Au catalyst. Fully lithiated silicon nanowires were obtained by using the electrochemical method, followed by drop-casting on the silicon substrate. The roughness, derived from a line profile of the surface measured in contact mode atomic force microscopy, has a smaller value for lithiated silicon nanowire and a higher value for unlithiated silicon nanowire. Force spectroscopy was utilitzed to study the influence of lithiation on the tip-surface adhesion force. Lithiated silicon nanowire revealed a smaller value than that of the Si nanowire substrate by a factor of two, while the adhesion force of the silicon nanowire is similar to that of the silicon substrate. The Young's modulus obtained from the force-distance curve, also shows that the unlithiated silicon nanowire has a relatively higher value than lithiated silicon nanowire due to the elastically soft amorphous structures. The frictional forces acting on the tip sliding on the surface of lithiated and unlithiated silicon nanowire were obtained within the range of 0.5-4.0 Hz and 0.01-200 nN for velocity and load dependency, respectively. We explain the trend of adhesion and modulus in light of the materials properties of silicon and lithiated silicon. The results suggest a useful method for chemical identification of the lithiated region during the charging and discharging process.

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모바일 레이저 스캐닝 데이터로부터 철도 시설물 인식에 관한 연구 (Railway Object Recognition Using Mobile Laser Scanning Data)

  • ;좌윤석;손건호;원종운;이석
    • 한국산업정보학회논문지
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    • 제19권2호
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    • pp.85-91
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    • 2014
  • 본 연구는 MLS 데이터로부터 자동으로 철도 시설물들을 인식하여 시설물 간의 기하학적인 공간정보를 추출하는데 기여 하고자 한다. 본 연구에서 제안된 방법은 9개 주요 철도 시설물(노반, 레일, 철로, 수목, 플렛폼, 방음벽, 철주, 절연체, 고압선)들의 분류를 목적으로 하고 있다. 이를 위해 제안된 방법은 크게 두 단계로 나뉘어 진행된다. 첫 번째 단계에서는 포인트, 라인, 체적과 수직 프로파일 레벨에서 데이터의 맥락 특징(contextual feature)들이 추출된다. 두 번째 단계에서는 CRF(Conditional Random Field)가 맥락 분류자(contextual classifier)로 사용되어 각 데이터 포인트에 객체 정보가 할당되고 철도 시설물들이 분류된다. 사용된 CRF 모델은 다른 맥락 분류자 와는 달리 로컬지역에서 데이터들의 분류정보가 일관성을 유지하게 하는 장점이 있다. 제안된 방법의 성능은 commission과 omission 오류분석을 통해 입증되었다.

리켓츠 분석을 이용한 한국인 아동의 두부방사선 계측학적 연구 (A CEPHALOMETRIC STUDY OF KOREAN CHILDREN BY RICKETTS' ANALYSIS)

  • 양규호;김선미
    • 대한소아치과학회지
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    • 제25권2호
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    • pp.430-440
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    • 1998
  • This study was performed to establish the cephalometric standards and to compare measurement of Korean children in the Field I, II, III, IV, V, VI to Japanese and Caucasians by the Ricketts' analysis. Lateral cephalograms of 24 males and 27 females with normal occlusion and acceptable profile 9 years of age were obtained and statistically analyzed. 1. Norms of Korean males, females and both sexes at 9 years old were established. 2. Significant differences between male and female exist in incisor overjet, maxillary incisor protrusion, mandibular incisor inclination, cranial deflection, corpus length. Maxillary incisor of male was more protrude and overjet was larger than female 3. Korean was similar to Japanese but different from Caucasian. Compare with facial axis and facial depth, chin was retruded dolichofacial pattern and due to large mandibular plane angle and small corpus length, mandibular plane was inclined and mandible body was short. Compare with porion location, ramus position and posterior facial height, ramus was long and located posterior. Compare with maxillary depth and maxillary height, maxilla was located posterior and inferior. The distance between the upper molar and PTV was short, the amount of distalization is limited. Maxillary and mandibular incisor were more protruded and also lower lip was more protruded to esthetic line 4. In comparison between 9 and 11 years old, growth changes of facial depth, mandibular plane angle, corpus length and upper molar position were larger than that of Japanese and Caucasians.

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나카가미 페이딩 채널에서 전력 및 전송률 적응화 직접 대역확산 부호분할 다중접속 통신시스템을 위한 최적 칩률에 관한 연구 (Optimal Chip Rate of Power and Rate Adapted DS/CDMA Communication Systems in Nakagami Fading Channels)

  • 이예훈
    • 한국통신학회논문지
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    • 제35권2A호
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    • pp.128-133
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    • 2010
  • 본 논문에서는 나카가미 페이딩 채널 환경에서 전력 혹은 전송률 적응화 된 직접 대역확산 부호분할 다중접속 통신시스템에서의 최적 칩률에 관하여 연구한다. 주파수 효율을 최대화하는 최적의 칩률은 다중경로 세기 프로파일과 직접파 성분, 그리고 적응화 방식에 의해 결정됨을 알았다. 전송률 적응화 방식에서의 최적의 칩률은 채널 파라미터에 상관없이 다중경로 지연 확산 $1/T_m$ 보다 적다. 이 결과는 전송률 적응화 방식에서는 상관 수신기가 RAKE 수신기보다 더 높은 주파수 효율을 얻을 수 있다는 것을 의미한다. 반면에 전송 전력 적응화 방식에서는 최적의 칩률과 그에 상응하는 RAKE 수신기의 탭 수가 다중경로 세기 프로파일과 직접파 성분에 관한 함수임을 알 수 있었다.

황기 육계의 배합에 따른 면역활성 비교 (Comparative analysis on immune response of combination with Astragali Radix and Cinnamomi Cortex)

  • 정다영;하혜경;이호영;이남헌;신현규
    • 대한본초학회지
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    • 제26권4호
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    • pp.187-194
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    • 2011
  • Objective : Astragali Radix (AR) and Cinnamomi Cortex (CC) are used to enhance immune response in Asian traditional medicine. Immuno-potentiation of the combination of AR and CC were evaluated on the cellular and humoral immune response using murine macrophage cell line (RAW 264.7) and OVA-immunized mice. Methods : This study was designed to investigate the immuno-potentiative effects of AR, CC, and AR with CC on nitric oxide synthesis in RAW 264.7 cells and proliferation and production levels of Intereukin-2 (IL-2) in mouse splenocytes. In addition, we evaluated the plasma-specific antibody responses and splenocyte proliferation on ovalbumin (OVA)-immunized mice treated with herbal extracts. Results : Combination treatment with AR and CC increased nitric oxide synthesis in RAW 264.7 cells and IL-2 level in splenocytes (p<0.001). Combination of AR and CC significantly enhanced the Concanavalin A- (Con A ; T cell mitogen) and lipopolysaccharide-(LPS ; B cell mitogen) induced splenocyte proliferation on the OVA-immunized mice. Combination of AR and CC also significantly enhanced plasma levels of OVA-specific IgG (p<0.01), IgG1 (p<0.05) and total IgM (p<0.01) compared with the OVA-immunized control group. Conclusion : These results suggest that combination of AR and CC could be used as therapeutic profile on activation of immune response.

Investigation of the Performance of Spectral Domain Optical Doppler Tomography with High-speed Line Scanning CMOS Camera and Its Application to the Blood Flow Measurement in a Micro-tube

  • Park, Cheol Woo;Lee, Changho;Lim, SooHee;Ni, Aleksey;An, Jin Hyo;Lee, Ho;Bae, Jae Sung;Kim, Jeehyun
    • Journal of the Optical Society of Korea
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    • 제16권2호
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    • pp.174-180
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    • 2012
  • In this study, the feasibility of spectral domain optical Doppler tomography for measuring blood flow characteristics in a micro-tube was demonstrated through several experiments. The use of an SD-ODT system in blood flow measurement can provide high resolution images (5 microns resolution). We prepared three capillary tubes to reveal the effect of different concentrations of hematocrit ratio (HR). One tube serves as the control. The two other tubes contained different concentrations of HR (5%, 25%). Three different capillary tube inlet flow velocities were tested in the present study. The Reynolds number (Re) which is based on the capillary tube inner diameter ranges from Re=6 to 48. We calculated a Doppler shift of the power spectrum of the temporal interference fringes with Kasai autocorrelation function to achieve the velocity profile of the flow. As a result, SD-ODT systems could not detect the cell depletion layer in the present study due to the limitation of spatial resolution. Nevertheless, these systems were proven to be capable of observing the RBCs of blood.

행성상 성운 NGC 7009, NGC 7027의 모델 연구

  • 이선주;형식
    • 한국지구과학회:학술대회논문집
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    • 한국지구과학회 2010년도 춘계학술발표회 논문집
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    • pp.121-121
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    • 2010
  • 행성상 성운 NGC 7009와 NGC 7027의 모델을 연구하기 위해 1998년 8월 14일부터 16일 까지 3일간의 Keck I HIRES의 분광 관측 자료를 이용하였다. 사용한 파장 영역은 $3250{\AA}{\sim}8725{\AA}$이고, H I, He I, He II, C II, C III, N II, N III, [N II], [O I], [O II], [O III], [S II], [S III], [Cl III], [Cl IV], [Ar III], [Ne III] 등의 방출선을 얻었다. 본 연구에서는 이러한 방출선의 선윤곽(line profile)을 IRAF와 StarLink/Dipso를 이용해 분석하여 성분을 구하였는데 H I, He I, He II, [O III], [C III], [N II] 등 대부분은 2개로 분리되었고, [S II], [Ar III]의 경우에는 3개로 분리되었다. 후자의 경우 구각(shell)의 단순한 팽창뿐만 아니라 다른 제3의 방향으로 팽창하고 있는 성분이 존재함을 의미한다. 비교적 S/N가 양호한 선들의 FWHM(Full Width at Half Maximum)을 측정하여 팽창속도를 구한 후 이 선들이 생성에 기여한 지역의 온도 또는 이온화 에너지 (IP)에 대한 팽창속도의 변화를 조사하였다. 또한 두 행성상 성운의 물리적 특성과 화학 원소 함량을 결정하기위해 광이온 모델 Tlusty Code와 CLOUDY를 사용하여 NGC 7009의 선행연구 Hyung & Aller(1995), Kwitter & Henry(1998)와 비교하였고, NGC 7027은 Zhang & Liu(2005), Middlemass(1990)와 비교하였다. NGC 7009과 NGC 7027의 수소 밀도($N_H$)를 $8,000cm^{-3}$으로 가정했을 때, NGC 7009의 중심별의 온도는 77,000K이고, 구각(shell)의 크기는 0.031~0.044pc이며 장축에 대해서만 결과를 나타내었다. NGC 7027의 경우, 중심별의 온도는 180,000K이고, 구각(shell)의 크기는 0.015~0.02pc으로 판단된다.

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슬로싱 충격현상 해석을 위한 모형실험과 수치해석 적용에 관한 비교 연구: PIV vs. CFD (Comparative Study on Sloshing Impact Flows between PIV and CFD)

  • 양경규;김지응;김상엽;김용환
    • 한국해양공학회지
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    • 제29권2호
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    • pp.154-162
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    • 2015
  • In this study, experimental and numerical methods were applied to observe sloshing impact phenomena. A two-dimensional rectangular tank filled with water and air was considered with a specific excitation condition that induced a hydrodynamic impact without an air pocket at the top corner of the tank. High-speed cameras and a pressure measurement system were synchronized, and a particle image velocimetry (PIV) technique was applied to measure the velocity field and corresponding pressure. The experimental condition was implemented in a numerical computation to solve incompressible two-phase flows using a Cartesian-grid method. The discretized solution was obtained using the finite difference and constraint-interpolation-profile (CIP) methods, which adopt a fractional step scheme for coupling the pressure and velocity. The tangent of the hyperbola for interface capturing (THINC) scheme was used with the weighed line interface calculation (WLIC) method to capture the interface between the air and water. The calculated impact pressures and velocity fields were compared with experimental data, and the relationship between the local velocity and pressure was investigated based on the computational results.

The drivers and energetics of ionized gas outflows in powerful Type 2 AGN in the local Universe

  • Karouzos, Marios;Woo, Jong-Hak;Bae, Hyun-Jin
    • 천문학회보
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    • 제41권1호
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    • pp.37.2-37.2
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    • 2016
  • There exist scaling relations that link the mass of supermassive black holes with both the velocity dispersion and the mass of the central stellar cusp of their host galaxies. This implies that galaxies co-evolve with their central black holes, potentially through the feedback from actively accreting supermassive black holes (AGN). We use integral field spectroscopy data from the 8.2m Gemini-North telescope to investigate ionized gas outflows in luminous local (z<0.1) Type 2 AGN. Our sample of 6 galaxies was selected based on their [OIII] dust-corrected luminosity (>$10^{42}erg/s$) and signatures of outflows in the [OIII] line profile of their SDSS spectra. These are arguably the best candidates to explore AGN feedback in action since they are < 1% of a large local type 2 AGN SDSS sample selected based on their [OIII] kinematics. Expanding on previously reported results concerning the kinematic decomposition and size determination of these outflows, here we report their photoionization properties and energetics. We find strong evidence that connect the extreme kinematics of the ionized gas with AGN photoionization. The kinematic component related to the AGN-driven outflow is clearly separated from other kinematic components, such as gravitation- or stellar-driven motions, on the velocity and velocity dispersion diagram. Our spatially resolved kinematic analysis reveals that up to 90% of the mass and kinetic energy of the outflow is contained within the central kiloparcec of the galaxy. The total mass and kinetic energy of the outflow correlate well with the AGN bolometric luminosity, resulting in energy conversion efficiencies between 0.01% and 1%. Intriguingly, we detect ubiquitous signs of ongoing circumnuclear star formation. Their small size, the centrally contained mass and energy, and the universally detected circumnuclear star formation cast doubts on the potency of these AGN-driven outflows as agents of negative feedback.

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하악지시상분할절단술에 의한 하악전돌증 수술후 상순의 변화에 관한 연구 (A STUDY ON THE CHANGE OF THE UPPER LIP AFTER SAGITTAL SPLIT RAMUS OSTEOTOMY)

  • 우순섭;위현철;이영수;심광섭
    • Maxillofacial Plastic and Reconstructive Surgery
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    • 제21권1호
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    • pp.35-40
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    • 1999
  • Recently, sagittal split ramus oseotomy and intraoral vertical ramus osteotomy have been commonly performed for the correction of mandibular prognathism, occurred to abundant oriental people. Many authors have studied the soft tissue change after orthognathic surgery, especially between mandibular hard tissues and soft tissue of lower lip, but the study of upper lip change is comparatively little. Therefore, we studied the 12 patients, operated only sagittal split ramus osteotomy without genioplasty or maxillary osteotomy in department of oral and maxillofacial surgery, Hanyang university hospital from 1996. 1. 1. to 1998. 7. 20. Preoperative and postoperative cephalometric view was measured to know the change of upper lip position and shape after mandibular setback. The result were obtained as follows. 1. The ratio of upper lip change amount to lower incisor horizontal movement was 15.1%. 2. The ratio of lower facial profile between Sn-Stm and Stm-Mes was changed from 1 : 2.352 to 1 : 2.069 after operation. 3. Post-operative upper lip was flattened 72.4% compared with pre-operative one. 4. The vermilion zone of the upper lip increased 56 % horizontally, 5.8% vertically after operation. 5. The vermilion zone ratio of the lower lip to the upper lip was changed from 1 : 1.253 to 1 : 1.348. 6. The distance between esthetic line and Ls was changed from -3.958mm to -1.15mm.

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