• 제목/요약/키워드: 1D Simulations

검색결과 822건 처리시간 0.027초

1.5V 2mW 96dB Peak SNDR, 오디오용 $\sum\Delta$ Modulator 설계 (Design of a 1.5V 2mW 96dB Peak SNDR $\sum\Delta$ Modulator for Audio Applications)

  • 이강명;이상훈;박종태;유종근
    • 대한전자공학회:학술대회논문집
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    • 대한전자공학회 2000년도 추계종합학술대회 논문집(2)
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    • pp.156-159
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    • 2000
  • This paper presents a low-voltage, low-power $\Sigma$Δ modulator for audio applications. It use a simple second-order fully-differential switched-capacitor structure with a sampling frequency of 12.5 MHz and oversampling ratio of 256. It operates from a single 1.5V Bower supply and dissipates 2 ㎽. Extensive simulations using 0.25 ${\mu}{\textrm}{m}$ CMOS Process parameters show that it achieves 96㏈ peak SNDR in a 22 KHz bandwidth.

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A Study of Kinetic Effect on Relativistic Shock using 3D PIC simulation

  • 최은진;민경욱;최청림
    • 천문학회보
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    • 제37권1호
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    • pp.67.1-67.1
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    • 2012
  • Shocks are evolved when the relativistic jets in active galactic nuclei (AGNs), black hole binaries, supernova remnants (SNR) and gamma-ray bursts (GRBs) interact with the surrounding medium. The high energy particles are believed to be accelerated by the diffusive shock acceleration and the strong magnetic field is generated by Weibel instability in the shock. When ultrarelativistic electrons with strong magnetic field cool by the synchrotron emission, the radiation is observed in gamma-ray burst and the near-equipartitioned magnetic field in the external shock delays the afterglow emission. In this paper, we performed the 3D particle-in-cell (PIC) simulations to understand the characteristics of these relativistic shock and particle acceleration. Forward and reverse shocks are shaped while the unmagnetized injecting jet interacts with the unmagnetized ambient medium. Both upstream and downstream become thermalized and the particle accelerations are shown in each transition region of the shock structures.

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음향 압축기 설계를 위한 축대칭 공명튜브 내부음장의 수치해석 및 특성연구 (Numerical Analysis of Nonlinear Acoustic Characteristics in Axisymmetric Resonant Tubes for Sonic Compressors)

  • 전영두;김양한
    • 한국소음진동공학회:학술대회논문집
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    • 한국소음진동공학회 2001년도 춘계학술대회논문집
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    • pp.1009-1014
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    • 2001
  • A numerical investigation on nonlinear oscillations of gas in an axisymmetric resonant tube is presented. When a tube is oscillated at a resonant frequency, acoustic variables such as density, velocity, and pressure undergo very large perturbation, often described as nonlinear oscillation. In order to analyze these phenomena, axisymmetric 2-D nonlinear governing equations have been derived and solved numerically. Numerical simulations were accomplished for cylindrical, conical, and 1/2 cosine-shape tubes, which have same volume and length. For conical and 1/2 cosine-shape tubes, very large variation of pressures can be induced without shock formation except the cylindrical tube. In addition, the results well agree to those of 1-D simple model analysis.

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초음속 습공기 유동에서 비정상 공동유동의 진동 (The Unsteady Cavity Flow Oscillation in Supersonic Moisture Air Stream)

  • 신춘식;이종성;김희동
    • 한국추진공학회:학술대회논문집
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    • 한국추진공학회 2008년도 제31회 추계학술대회논문집
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    • pp.341-344
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    • 2008
  • Numerical simulations have been carried out for a supersonic two-dimensional flow over open, rectangular cavities (length-to-depth ratios are L/D = 1.0) in order to investigate the effect of non-equilibrium condensation of moist air on supersonic flows around the cavity for the flow Mach number 1.83 at the cavity entrance. In the present computational investigation, a condensing flow was produced by an expansion of moist air in a Laval nozzle. The results obtained showed that in the case with non-equilibrium condensation for L/D = 1.0, amplitudes of oscillation in the cavity became smaller than those without the non-equilibrium condensation. Furthermore, the occurrence of the non-equilibrium condensation reduced the peaks of power spectrum density and the frequency of the flow field oscillation increased in comparison with the case of $S_0$ = 0.

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<100>방향 실리콘 단결정에서의 저 에너지 붕소 이온 주입 공정에 대한 3차원 몬테 카를로 시뮬레이션 및 마스크 효과 (Three-dimensional monte carlo simulation and mask effect of low-energy boron ion implantation into <100>single-crystal silicon)

  • 손명식;이준하;송영진;황호정
    • 전자공학회논문지A
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    • 제32A권8호
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    • pp.94-106
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    • 1995
  • A three-dimensional(3D) Monte Carlo simulator for boron ion implantation into <100>single-crystal silicon considering the mask structure has been developed to predict the mask-dependent impurity doping profiles of the implanted boron at low energies into the reduced area according to the trend of a reduction in the size of semiconductor devices. All relevant important parameters during ion implantation have been taken into account in this simulator. These are incident energy, tilt and rotation of wafer, orientation of silicon wafer, presence of native silicon dioxide layer, dose, wafer temperature, ion beam divergence, masking thickness, and size and structure of open window in the mask. The one-dimensional(1D) results obtained by using the 3D simulator have been compared with the SIMS experiments to demonstrate its capabilities and confirem its reliability, and we obtained relatively accurate 1D doping profiles. Through these 3D simulations considering the hole structure and its size, we found the mask effects during boron ion implantation process.

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레일리 페이딩 채널에서 차등 변조기법을 이용한 선택적 복호 후 재전송 중계 네트워크의 성능 분석 (Performance Analysis for Selection Decode-and-Forward Relay Networks with Differential Modulation over Rayleigh Fading Channels)

  • 공형윤;보 뉘엔 �o 바오
    • 한국통신학회논문지
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    • 제35권1A호
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    • pp.1-9
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    • 2010
  • 본 논문을 통해 i.n.d 레일리 패이딩 체널에서 서로 다른 변조/복조 기법을 사용하는 중계기들로 구성된 선택적 복호 후 재전송 네트워크의 성능평가를 보여준다. 본 논문은 i.i.d와 i.n.d 레일리 패이딩 채널 모두에서 선택적 복호 후 전송 프로토콜이 최대 다이버시티를 얻을 수 있다는 것을 보여준다. 또한 SC(selection combining)기법을 사용하는 시스템과 MRC(maximal ratio combining)기법을 사용하는 시스템의 성능을 비교하여 결합기술의 효과를 연구하였다. 높은 SNR에서 시뮬레이션 결과와 수식적 분석 결과가 정확하게 일치하는 것을 보여준다.

ACCELERATION OF COSMIC RAYS AT COSMIC SHOCKS

  • KANG HYESUNG
    • 천문학회지
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    • 제36권1호
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    • pp.1-12
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    • 2003
  • Nonthermal particles can be produced due to incomplete thermalization at collisionless shocks and further accelerated to very high energies via diffusive shock acceleration. In a previous study we explored the cosmic ray (CR) acceleration at cosmic shocks through numerical simulations of CR modified, quasi-parallel shocks in 1D plane-parallel geometry with the physical parameters relevant for the shocks emerging in the large scale structure formation of the universe (Kang & Jones 2002). Specifically we considered pancake shocks driven by accretion flows with $U_o = 1500 km\;s^{-l}$ and the preshock gas temperature of $T_o = 10^4 - 10^8K$. In order to consider the CR acceleration at shocks with a broader range of physical properties, in this contribution we present additional simulations with accretion flows with $U_o = 75 - 1500 km\;s^{-l}$ and $T_o = 10^4K$. We also compare the new simulation results with those reported in the previous study. For a given Mach number, shocks with higher speeds accelerate CRs faster with a greater number of particles, since the acceleration time scale is $t_{acc}\;{\propto}\;U_o^{-2}$. However, two shocks with a same Mach number but with different shock speeds evolve qualitatively similarly when the results are presented in terms of diffusion length and time scales. Therefore, the time asymptotic value for the fraction of shock kinetic energy transferred to CRs is mainly controlled by shock Mach number rather than shock speed. Although the CR acceleration efficiency depends weakly on a well-constrained injection parameter, $\epsilon$, and on shock speed for low shock Mach numbers, the dependence disappears for high shock Mach numbers. We present the 'CR energy ratio', ${\phi}(M_s)$, for a wide range of shock parameters and for $\epsilon$ = 0.2 - 0.3 at terminal time of our simulations. We suggest that these values can be considered as time-asymptotic values for the CR acceleration efficiency, since the time-dependent evolution of CR modified shocks has become approximately self-similar before the terminal time.

분산 시뮬레이션에서의 Coverage 분석에 관한 연구 (Quality of Coverage Analysis on Distributed Stochastic Steady-State Simulations)

  • 이종숙;박형우;정해덕
    • 정보처리학회논문지A
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    • 제9A권4호
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    • pp.519-524
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    • 2002
  • 본 논문에서는 분산 시뮬레이션 기법 중에 하나인 MRIP(Multiple Replications In Parallel) 시나리오에서 각종 순차적인 시뮬레이션 분석 방법들의 성능을 측정할 수 있는 포함범위(Coverage)에 대한 신뢰구간(confidence intervals) 및 속도향상(Speedup)에 대해 살펴보았다. F-분포를 기반으로 한 신뢰구간에 대한 추정기(estimator)를 단일 프로세서와 다중 프로세서 상에서 참조모델(reference model)로 $M/M/1/{\infty},\;M/D/I/{\infty}과\;M/H_{2}/1/{\infty}$큐잉 시스템을 활용하여 정상상태(steady-state)에서의 평균치를 추정하는 시뮬레이션에 적용하였다. 순차적인 포함범위 분석을 위해서는 수많은 시뮬레이션 실행(Run)들이 요구되는데, MRIP 분산 시뮬레이션 시나리오에서 다중 프로세서를 이용하여 시뮬레이션을 수행하여 최종 시뮬레이션 결과를 얻는데 걸리는 신간을 감소시켰다. 또한, LNA으로 연결된 분산 컴퓨팅 시스템에 시뮬레이션을 동시에 수행시킴으로써 쉽게 필요한 수의 시뮬레이션 실행결과(Run)를 수집할 수 있다. 이는 샘플의 수가 증가됨으로써 좀더 신뢰도가 높은 최종 신뢰구간을 시뮬레이션 수행자가 얻을 수 있게 해준다.

샌드위치판재의 U-bending 공정에서 굽힘하중식의 검증 (Verification of load equations for sandwich plates during U-bending)

  • 성대용;정창균;심도식;양동열;정완진
    • 한국소성가공학회:학술대회논문집
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    • 한국소성가공학회 2008년도 추계학술대회 논문집
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    • pp.435-438
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    • 2008
  • To verify the load equations, the load-stroke curves of the load equation that were analytically derived for sandwich plates were compared with those of the simulations in the case of the total thickness of 3 mm, the thickness of the face sheets of 0.5 mm, a gap between attachment points of 1.5 mm, and a thickness of the core element of 0.8 mm. The results of the comparisons showed that the overall analytic loads enable the prediction of the numerical loads irrespective of the change of the clearance, the radius of the die, and the radius ratio.

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Numerical Investigation of an Unconditionally Stable Compact 2D FDTD Based on the Alternating-Direction Implicit Scheme

  • Saehoon Ju;Jeongnam Cheon;Kim, Hyung-Hoon;Kim, Hyeongdong
    • Journal of electromagnetic engineering and science
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    • 제3권1호
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    • pp.39-44
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    • 2003
  • An unconditionally stable compact 2D Alternating-Direction Implicit (ADI) FDTD method for calculating dispersion characteristics of waveguide structures is proposed. The numerical stability and numerical dispersion relation of the proposed method are also presented and discussed. Numerical wavelengths for the dominant and higher order modes in a hollow waveguide are obtained from numerical simulations and compared with those from the analytical dispersion relation. The numerical results show that the proposed scheme has the potential to successfully analyze a class of waveguides having locally fine geometry with reduced numerical costs.