• Advances in concrete construction
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• 제15권4호
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• pp.241-249
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• 2023

The unsteady mixed convection Casson type MHD nanofluid flow in the stagnation point with motile microorganism around a spinning sphere is investigated. Time dependent flow dynamics is considered. Similarity transformations have been employed to transfer the governing partial differential structure into ordinary differential structure. The impact of distinct parameters is examined via tables and graphs. The impact of rotational parameter (spin) on profiles of velocity profiles, temperature and concentration is revealed for unsteady mixed convection Casson type MHD nanofluid flow. It is observed that it is clear that rotational parameter has a great effect on non-dimensional primary velocity component but rotational parameter has a slight impact on non-dimensional secondary velocity component. The validity of the current investigation is authorized through comparing the existing outcomes with previous published literature.

• 한국자기학회:학술대회 개요집
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• 한국자기학회 2009년도 임시총회 및 하계학술연구발표회
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• pp.159-160
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• 2009

• 제어로봇시스템학회:학술대회논문집
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• 제어로봇시스템학회 1991년도 한국자동제어학술회의논문집(국내학술편); KOEX, Seoul; 22-24 Oct. 1991
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• pp.264-267
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• 1991

In this paper, a new application method of the Kalman filter to desigin a gyro is proposed. The role of a gyro is the estimation of an input rate with minimal error covariance. The size of the error covariance depends on gyro's parameters, which makes it possible to use the parameters of gyro to minimze the estimation error covariance. Numerical analysis shows that the error covariance becomes smaller as the spin axis momentum becomes larger and the damping coefficient smaller, but production cost must be considered. Through numerical analysis the parameter set for an acceptable - performance gyro with small cost can be selected.

• Journal of Astronomy and Space Sciences
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• 제20권4호
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• pp.351-358
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• 2003

회전안정화 로켓 모터를 이용하는 우주 비행체의 자세 불안정 현상을 수치적 실험을 통하여 연구하였다. 이전 연구에서는 해석적 방법을 통하여 주어진 우주 비행체에 대한 정상해를 구하고 실제 발생했던 공진과 유사한 공진조건을 찾았으나 정상해 근방에서의 안정도 또는 파라미터 공간 전역에서의 안정도가 어떻게 변하는 지를 알 수가 없었다. 따라서, 본 연구에서는 이전 연구결과를 기초로 하여 주어진 파라미터 공간 전역에서 수치적 실험을 통하여 유동체의 파라미터 값에 따라 위성체의 자세 안정도가 어떻게 변화하는지를 관찰하고, 시스템 설계에 필요한 파라미터들의 안정/불안정 영역을 결정하였다.

• EDISON SW 활용 경진대회 논문집
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• 제3회(2014년)
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• pp.183-195
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• 2014

Kinetically constrained models (KCM) have attracted interest as models that assign dynamic origins to the interesting dynamic properties of supercooled liquid. Signs of dynamic heterogeneity in the crossover model that linearly interpolates between the FA-like symmetric constraint and the East model constraint by asymmetric parameter b were investigated using Monte Carlo technique. When the asymmetry parameter was decreased sufficiently, smooth fragile-to-strong dynamic transition was observed in terms of the relaxation time, diffusion constant, Stokes-Einstein violation, and dynamic length scale. Competition between energetically favored symmetric relaxation mechanism and entropically favored asymmetric relaxation mechanism is behind such transition.

• Journal of Magnetics
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• 제16권3호
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• pp.206-210
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• 2011

We optimize a vector network analyzer ferromagnetic resonance (VNA-FMR) measurement system to study spin dynamics and Gilbert damping parameters of thin ferromagnetic films. In order to obtain accurate damping parameters, careful determination of the susceptibility line-width is required. The measured S-parameters are converted into the corresponding susceptibility through a calibration processes. From the line-width measurements, we can successfully extract the saturation magnetizations and Gilbert damping parameters of 5-, 8-, and 10-nm thick $Ni_{81}Fe_{19}$ (Py) films.

• Bulletin of the Korean Chemical Society
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• 제33권4호
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• pp.1235-1241
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• 2012

Aluminium (Al)-doped zinc oxide (AZO) thin films with different Al concentrations were prepared by the solgel spin-coating method. Optical parameters such as the optical band gap, absorption coefficient, refractive index, dispersion parameter, and optical conductivity were studied in order to investigate the effects of the Al concentration on the optical properties of AZO thin films. The dispersion energy, single-oscillator energy, average oscillator wavelength, average oscillator strength, and refractive index at infinite wavelength of the AZO thin films were found to be affected by Al incorporation. The optical conductivity of the AZO thin films also increases with increasing photon energy.

• 대한전기학회:학술대회논문집
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• 대한전기학회 1999년도 추계학술대회 논문집 전문대학교육위원 P
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• pp.10-12
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• 1999

Optical properties of $Zn_2AgGaSe_4$ and $Zn_2AgGaSe_4$:$Co^{2+}$ crystals are investigated in the visible and near-infrared regions at 298K. The direct band gap at 298K is 1.630eV for the $Zn_2AgGaSe_4$ and 1.567eV for the $Zn_2AgGaSe_4$:$Co^{2+}$ crystals, respectively. In the optical absorption and PAS spectrum of the $Zn_2AgGaSe_4$:$Co^{2+}$, we observed five impurity absorption peaks at $4220cm^{-1}$, $5952cm^{-1}$, $12422cm^{-1}$, $12987cm^{-1}$ and $14184cm^{-1}$. These impurity absorption peaks are attributed to the electronic transitions between the split energy levels of $Co^{2+}$ ions with Td symmetry of $Zn_2AgGaSe_4$ host lattice. The crystal field parameter Dq, the Racah parameter B and the spin-orbit coupling parameter $\lambda$ are given by $442cm^{-1}$, $425cm^{-1}$ and $440cm^{-1}$, respectively.

• 한국신재생에너지학회:학술대회논문집
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• 한국신재생에너지학회 2011년도 춘계학술대회 초록집
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• pp.124.1-124.1
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• 2011

결정질 태양전지에서 도핑(Doping)은 반도체(Semiconductor)의 PN 접합(Junction)을 형성하는 중요한 역할을 한다. 도핑은 반도체에 불순물(Dopant)을 주입하는 공정으로 고온에서 진행되며 온도는 중요한 변수(Parameter)로 작용한다. 본 연구에서는 여러 가지 도핑 방법 중 SOD(Spin-On Dopant)를 이용하여 온도에 따른 도핑 결과와 특성을 분석 하였다. P-type 웨이퍼(Wafer)에 SOD를 이용하여 불순물을 증착 후 Hot-plate에서 15분간 Baking 하였다. Baking된 웨이퍼는 노(Furnace)에 넣고 $860^{\circ}C{\sim}880^{\circ}C$까지 $10^{\circ}C$씩 가변하였다. 각각의 조건에 대해 Lifetime과 Sheet Resistance을 측정하였고, 그 결과 $880^{\circ}C$에서의 Lifetime이 $23.58{\mu}s$로 $860^{\circ}C$에 비해 235.8% 증가하여 가장 우수 하였으며, Sheet Resistance 또한 $68{\Omega}$/sq로 $860^{\circ}C$에서 가장 우수하게 측정되었다. SOD의 속도 가변에 따른 특성 변화를 보기 위해 온도는 $880^{\circ}C$에 고정한 후 속도를 3000rpm~4500rpm까지 500rpm간격으로 1시간동안 실험한 결과 rpm 속도에 따른 lifetime 변화는 거의 없었으며, Sheet Resistance는 3000rpm에서 $63{\Omega}$/sq로 가장 우수 하였다. 본 연구를 통해 온도와 Spin rpm에 따른 특성을 확인한 결과 온도가 높을 때 Sheet Resistance가 가장 안정화 되며, lifetime이 더욱 우수한 것을 확인할 수 있었다.

• 천문학회지
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• 제29권1호
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• pp.19-30
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• 1996

We have examined consequences of strong tidal encounters between a neutron star and a normal star using SPH as a possible formation mechanism of isolated recycled pulsars in globular clusters. We have made a number of SPH simulations for close encounters between a main-sequence star of mass ranging from 0.2 to 0.7 $M_\bigodot$ represented by an n=3/2 poly trope and a neutron star represented by a point mass. The outcomes of the first encounters are found to be dependent only on the dimensionless parameter $\eta'{\equiv}(m/(m+ M))^{1/2}(\gamma_{min}/R_{MS})^{3/2}(m/M)^{{1/6)}$, where m and M are the mass of the main-sequence star and the neutron star, respectively, $\gamma_{min}$ the minimum separation between two stars, and $R_{MS}$ the size of the main-sequence star. The material from the (at least partially) disrupted star forms a disk around the neutron star. If all material in the disk is to be acctreted onto the neutron star's surface, the mass of the disk is enough to spin up the neutron star to spin period of 1 ms.