• Title/Summary/Keyword: thermal history

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Thermal Chemical Vapor Deposition of Graphene Layers

  • Kwon, Kyoeng-Woo;Do, Woo-Ri;Hwang, Jinha
    • Proceedings of the Korean Vacuum Society Conference
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    • 2013.02a
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    • pp.644-644
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    • 2013
  • Graphene is a two-dimensional sp2 layer material. Despite the short history in the empirical synthesis of the graphene layers, the academic/industrial unique features have brought highly significant interest in research and development related to graphene-related materials. In particular, the electrical and optical performances have been targeted towards pre-existing microelectronicand emerging nanoelectronic applications. The graphene synthesis relies on a variety of processing factors, such as temperature, pressure, and gas ratios involving H2, CH4, and Ar, in addition to the inherent selection of copper substrates. The current work places its emphasis on the role of experimental factors in growing graphene thin films. The thermally-grown graphene layers are characterized using physical/chemical analyses, i.e., four point resistance measurements, Raman spectroscopy, and UV-Visible spectrophotometry. Ultimately, an optimization strategy is proposed in growing high-quality graphene layers well-controlled through empirical factors.

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Dynamic responses of laminated beams under a moving load in thermal environment

  • Akbas, Seref D.
    • Steel and Composite Structures
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    • v.35 no.6
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    • pp.729-737
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    • 2020
  • The goal of this study is to investigate dynamic responses of laminated composite beams under a moving load with thermal effects. The governing equations of problem are derived by using the Lagrange procedure. The transverse-shear strain and rotary inertia are considered within the Timoshenko beam theory. The material properties of laminas are considered as the temperature dependent physical property. The differential equations of the problem are solved by the Ritz method. The solution step of dynamic problem, the Newmark average acceleration method is used in the time history. A compassion study is performed for accuracy of used formulations and method. In the numerical results, the effects of velocity of moving load, temperature values, the fiber orientation angles and the stacking sequence of laminas on the dynamic responses of the composite laminated beam are investigated.

Process Simulation of Investment Casting for Large Gas Turbine Component (대형 가스터빈 부품의 정밀주조 응고해석)

  • Seo, Seong-Mun;Jo, Chang-Yong;Lee, Jae-Hyeon;Choe, Seung-Ju
    • 연구논문집
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    • s.29
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    • pp.173-183
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    • 1999
  • The vacuum investment casting process for a large gas turbine component, Inner Preswirl Support (IPS), was simulated by using commercial FEM package ProCAST(TM) with view factor radiation method. The solid fraction in mushy zone was directly measured by Differential thermal analysis(DTA-DSC mode). Three types gating design. considering liquid flow and heat release through it. were proposed. Solidification had begun at the ribs or thin sections of the IPS casting and advanced further through the upper and lower gates. The computed temperature gradient G and G/R values at 70% solidified temperature were used for prediction of microshrinkage formation during casting. The effect of mold preheat on the thermal history of the casting displayed minute effect on the microshrinkage formation.

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STUDY ON NUMERICAL ANALYSIS AND TURBULENCE MODELS FOR ARC DISCHARGES IN HIGH-VOLTAGE INTERRUPTERS (초고압 차단부 아크방전 수치해석 및 난류모델에 관한 연구)

  • Lee, J.C.
    • Journal of computational fluids engineering
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    • v.15 no.3
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    • pp.9-15
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    • 2010
  • In this study, we calculated arc discharges and flow characteristics driven by arcs in a thermal puffer chamber, which is one of most outstanding high-voltage interrupters, for understanding the complex physics and the probability of thermal breakdown. The four main parts of arc model for this virtual-reality are radiation, PTFE ablation, Cu evaporation, and turbulence. Among these important parts the turbulence model can be critical to the reliability of computation results during the whole arcing history because the plasma flow is affected by high heat energy and mass momentum. Two turbulence models, the Prandtl's mixing length model and the standard $k-\varepsilon$ model, are applied for these calculations and are compared with pressure-rise inside chamber and arc voltage between the contacts as well as flow characteristics near current zero.

Prediction of Temperature and Moisture Distributions in Hardening Concrete By Using a Hydration Model

  • Park, Ki-Bong
    • Architectural research
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    • v.14 no.4
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    • pp.153-161
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    • 2012
  • This paper presents an integrated procedure to predict the temperature and moisture distributions in hardening concrete considering the effects of temperature and aging. The degree of hydration is employed as a fundamental parameter to evaluate hydro-thermal-mechanical properties of hardening concrete. The temperature history and temperature distribution in hardening concrete is evaluated by combining cement hydration model with three-dimensional finite element thermal analysis. On the other hand, the influences of both self-desiccation and moisture diffusion on variation of relative humidity are considered. The self-desiccation is evaluated by using a semi-empirical expression with desorption isotherm and degree of hydration. The moisture diffusivity is expressed as a function of degree of hydration and current relative humidity. The proposed procedure is verified with experimental results and can be used to evaluate the early-age crack of hardening concrete.

CHEMICAL EVOLUTION IN VeLLOs

  • Lee, Jeong-Eun
    • Journal of The Korean Astronomical Society
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    • v.40 no.4
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    • pp.83-89
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    • 2007
  • A new type of object called "Very Low Luminosity Objects (VeLLOs)" has been discovered by the Spitzer Space Telescope. VeLLOs might be substellar objects forming by accretion. However, some VeLLOs are associated with strong outflows, indicating the previous existence of massive accretion. The thermal history, which significantly affects the chemistry, between substellar objects with a continuous low accretion rate and objects in a quiescent phase after massive accretion (outburst) must be greatly different. In this study, the chemical evolution has been calculated in an episodic accretion model to show that CO and $N_2H^+$ have a relation different from starless cores or Class 0/I objects. Furthermore, the $CO_2$ ice feature at $15.2{\mu}m$ will be a good tracer of the thermal process in VeLLOs.

A Study on the Convection Heat Transfer Coefficient in Concrete at Early Ages (초기재령 콘크리트의 외기대류계수에 관한 연구)

  • 김진근;전상은;양은익;송영철;방기성
    • Proceedings of the Korea Concrete Institute Conference
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    • 1997.10a
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    • pp.151-156
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    • 1997
  • The setting and hardening of concrete is accompanied by nonlinear temperature distribution caused by developing heat of cement hydration. expecially at early ages, nonlinear temperature distribution has a large influence n the crack evaluation. So the need to predict the exact temperature history in concrete has led to the examination thermal properties. In this study, the convection heat transfer coefficient is experimentally investigated which is one of the thermal properties in concrete. Furthermore, the result of the experiment is compared with those of analysis by the program which is developed in KAIST. As a result of comparison, the analytical results are in good approximation with experimental data.

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Thermal History Analysis and Solid Fraction Prediction of Gas-Atomized Alloy Droplets during Spray Forming (분무성형 공정에서 분무액적의 열이력 해석 및 고상분율 예측)

  • 이언식
    • Journal of Powder Materials
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    • v.1 no.1
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    • pp.85-94
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    • 1994
  • In order to predict droplet velocity and temperature profiles and fractional solidification with flight distance during spray forming, the Newtonian heat transfer formulation has been coupled with the classical heterogeneous nucleation and the specific solidification process. It has been demonstrated that the thermal profile of the droplet in flight is significantly affected by process parameters such as droplet size, initial gas velocity, undercooling. As the droplet size and/or the initial gas velocity increase, the onset and completion of solidification are shifted to greater flight distances and the solidification process also extends over a wider range of flight distances. The amounts of solid fractions formed during recoalescence, segregated solidification and eutectic solidification are insensitive to droplet size and initial gas velocity whereas those are strongly affected by the degree of undercooling. There are good linear relations between the undercooling and the corresponding solid fractions generated during recoalesced, segregated and eutectic stages.

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Examination and Measures on Failure of Hydraulic Oil Supply Pipe of Control Valve of Steam Turbine in 200MW Thermal Power Plant (200MW급 화력발전소 고압터빈 제어밸브 압유배관의 절손 원인과 대책)

  • Kim, Yeon-Whan;Lee, Young-Shin;Kim, Hee-Soo;Lee, Hyun;Kim, Sung-Hwi
    • Proceedings of the Korean Society for Noise and Vibration Engineering Conference
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    • 2002.05a
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    • pp.569-576
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    • 2002
  • A case history is presented pertaining to piping fatigue by vibrations and sustain stresses in the hydraulic oil supply system for control valves in a 200MW thermal power plant that ultimately resulted in pipe rupture. The Piping was designed to supply the hydraulic oil for turbine control valves. Testing and analyses were performed on the system to develop solution to repair work on failures.

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THERMAL PROPERTIES OF SMALL GRAINS WITH FLUCTUATING TEMPERATURE UNDER DIFFUSE INTERSTELLAR RADIATION FIELD

  • Hong, Seung-Soo
    • Journal of The Korean Astronomical Society
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    • v.12 no.1
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    • pp.27-34
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    • 1979
  • Temperature history of very small interstellar dust particles is followed under diffuse interstellar radiation. Because of extremely small thermal capacities of these grains with sizes ranging from a few tens to hundred Angstroms in radii, they are to experience strong fluctuations in temperature whenever they are hit by interstellar ultraviolet photons. Fluctuating temperature can inhibit these smaller component of interstellar dust from growing into core-mantle particles of submicron sizes by continuously evaporating atoms and molecules adsorbed on their surface. This is interpreted as a possible physical reason for the bimodal nature in grain size distribution. A brief discussion is also given to the far infrared emission properties of such small grains in diffuse interstellar dust clouds.

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