• 제목/요약/키워드: near-zero

검색결과 424건 처리시간 0.03초

영자왜 마몰퍼스 자성박막의 인덕턴스효과 (Inducdance Effects of Zeromagnetostrictive Amorphous Magnetic Films.)

  • 서강수;임재근;정승우;신용진
    • 한국전기전자재료학회:학술대회논문집
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    • 한국전기전자재료학회 1997년도 추계학술대회 논문집
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    • pp.136-139
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    • 1997
  • In this paper, we inveatigate frequency dependance of inductance effects of FeCoB amorphous magnetic films. First, amorphous magnetic film having near zero magnetostriction is the basic composition of (Fe$_{1-x}$ / $Co_{x}$)$_{79}$Si$_2$B$_{19}$ with x=0.94, 0.95 and in order to decrease magnetio . anisotropy, the film was annealed in 28$0^{\circ}C$/30min, 40$0^{\circ}C$/30min, 40$0^{\circ}C$/1hr with near crystallization temperature under non-magnetic field. As result of investigation, in case of x=7.95 than x=0.94, we could have obtained high values, which inductance ratios in the low frequency was 488%. And Quality factor Q was under 0.7 in all sample, in case of annealed in 28$0^{\circ}C$/30min, we could have obtained highest value, which x=0.9fl is about 0.62 in 400[kHz], and in case of x=0.95 was about 0.35 in 1[MHz].z].].

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면외변형하의 이방성 띠판에 대한 동적계면균열 (Dynamic Interfacial Crack in Bonded Anisotropic Strip Under Out-of-Plane Deformation)

  • 박재완;최성렬
    • 대한기계학회논문집A
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    • 제25권6호
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    • pp.949-958
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    • 2001
  • A semi-infinite interfacial crack propagated with constant velocity in two bonded anisotropic strips under out-of-plane clamped displacements is analyzed. Using Fourier integral transform the problem is formulated and the Wiener-Hopf equation is derived. By solving this equation the asymptotic stress and displacement fields near the crack tip are obtained, where the results get more general expressions applicable not only to isotropic/orthotropic materials but also to the extent of the anisotropic material having one plane of elastic symmetry for the interfacial crack. The dynamic stress intensity factor is obtained as a closed form, which is decreased as the velocity of crack propagation increases. The critical velocity where the stress intensity factor comes to zero is obtained, which agrees with the lower value between the critical values of parallel crack merged in the material 1 and 2 adjacent to the interface. Using the near tip fields of stresses and displacements, the dynamic energy release rate is also obtained as a form of the stress intensiy factor.

Three-dimensional Numerical Prediction on the Evolution of Nocturnal Thermal High (Tropical Night) in a Basin

  • Choi, Hyo;Kim, Jeong-Woo
    • International Union of Geodesy and Geophysics Korean Journal of Geophysical Research
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    • 제25권1호
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    • pp.57-81
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    • 1997
  • Numerical prediction of nocturnal thermal high in summer of the 1995 near Taegu city located in a basin has been carried out by a non-hydrostatic numerical model over complex terrain through one-way double nesting technique in the Z following coordinate system. Under the prevailing westerly winds, vertical turbulent fluxes of momentum and heat over mountains for daytime hours are quite strong with a large magnitude of more than $120W/\textrm{m}^2$, but a small one of $5W/\textrm{m}^2$ at the surface of the basin. Convective boundary layer (CBL) is developed with a thickness of about 600m over the ground in the lee side of Mt. Hyungje, and extends to the edge of inland at the interface of land sea in the east. Sensible heat flux near the surface of the top of the mountain is $50W/\textrm{m}^2$, but its flux in the basin is almost zero. Convergence of sensible heat flux occurs from the ground surface toward the atmosphere in the lower layer, causing the layer over the mountain to be warmed up, but no convergance of the flux over the basin results from the significant mixing of air within the CBL. As horizontal transport of sensible heat flux from the top of the mountain toward over the basin results in the continuous accumulation of heat with time, enhancing air temperature at the surface of the basin, especially Taegu city to be higher than $39.3^{\circ}C$. Since latent heat fluxes are $270W/\textrm{m}^2$ near the top of the mountain and $300W/\textrm{m}^2$ along the slope of the mountain and the basin, evaporation of water vapor from the surface of the basin is much higher than one from the mountain and then, horizontal transport of latent heat flux is from the basin toward the mountain, showing relative humidity of 65 to 75% over the mountain to be much greater than 50% to 55% in the basin. At night, sensible heat fluxes have negative values of $-120W/\textrm{m}^2$ along the slope near the top of the mountain and $-50W/\textrm{m}^2$ at the surface of the basin, which indicate gain of heat from the lower atmosphere. Nighttime radiative cooling produces a shallow nocturnal surface inversion layer with a thickness of about 100m, which is much lower than common surface inversion layer, and lifts extremely heated air masses for daytime hours, namely, a warm pool of $34^{\circ}C$ to be isolated over the ground surface in the basin. As heat transfer from the warm pool in the lower atmosphere toward the ground of the basin occurs, the air near the surface of the basin does not much cool down, resulting in the persistence of high temperature at night, called nocturnal thermal high or tropical night. High relative humidity of 75% is found at the surface of the basin under the moderate wind, while slightly low relative humidity of 60% is along the eastern slope of the high mountain, due to adiabatic heating by the srong downslope wind. Air temperature near the surface of the basin with high moisture in the evening does not get lower than that during the day and the high temperature produces nocturnal warming situation.

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다중 안테나 다중 사용자 환경에서 최대 전송율에 근접하는 선형 precoding 기법 (A Near Optimal Linear Preceding for Multiuser MIMO Throughput Maximization)

  • 장승훈;양장훈;장규환;김동구
    • 한국통신학회논문지
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    • 제34권4C호
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    • pp.414-423
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    • 2009
  • 본 논문은 최대 전송률에 가까운 성능을 보이는 선형 preceding 기법을 제안한다. MMSE preceding은 ZF preceding 방식보다 우수한 평균 자승 오차 성능을 가진다. 반면 MMSE preceding 방식의 전송률은 낮은 SNR 범위에서는 ZF 방식에 비해 개선된 성능을 보여주지만 높은 SNR에서는 오히려 성능 열화현상을 보인다. 이와 같은 사실에 착안하여 본 논문에서는 최대 전송률에 근접하는 선형 preceding 기법을 제안한다. 제안된 방식은 ZF precoding방식에서 사용되는 역행렬 연산을 전송율이 최대화될 수 있도록 정규화하는 방식이고 이를 위한 간단한 수치 알고리즘이 제안된다. 또한 그 과정에서 낮은 복잡도를 가지는 간단한 전력 재할당에 의한 정규화 방식이 제안된다. 시뮬레이션과 성능분석을 통해 제안된 방식이 모든 SNR 범위에서 기존의 ZF preceding 방식과 MMSE preceding방식보다 높은 전송률을 가짐을 보인다. 또한 제안된 방식은 채널 추정 오차가 존재하는 경우에도 기존의 선형 preceding 방식들과 비교하여 성능 이득을 유지하면서 채널 추정 오차에 강인함을 가진다.

메탄올을 환원제로 사용하는 과잉산소 분위기에서 $La_2O_3$ 촉매를 이용한 NO의 환원에 관한 연구 (Catalytic Reduction of Nitric Oxide in Oxygen-Rich Exhaust with Methanol over $La_2O_3$ Catalysts)

  • 김상환;유현주;박정규
    • 한국자동차공학회논문집
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    • 제13권2호
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    • pp.135-141
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    • 2005
  • Nitric oxide(NO) reduction by methanol was investigated over $La_2O_3$ catalysts in the presence and absence of oxygen. In the absence of $O_2$, $CH_3OH$ reduced NO to both $N_2$ and $N_2O$, with selectivity to $N_2$ formation decreasing from 81-88% at 623K to 47-71% at 723 K. With 1.2% $O_2$ in the feed, the rates were 4-8 times higher, but the selectivity to $N_2$ dropped from 50% at 623 K to 9% at 723 K. The specific activities with $La_2O_3$ for this reaction were higher than those for other reductants; for example, at 773 K with hydrogen a specific activity of $34\;{\mu}mol\;NO/sec{\cdot}m^2$ was obtained whereas that for methanol was $638\;{\mu}mol\;NO/sec{\cdot}m^2$. The Arrhenius plots were linear under differential reaction conditions, and the apparant activation energy was consistantly near 15 kcal/mol with $CH_3OH$. Linear partial pressure dependencies based on a power rate law were obtained and showed a near-zero order in $CH_3OH$ and a near-first order in $H_2$.

다중 셀 환경에서 적은 복잡도를 갖는 준 최적 하향 빔형성 (Simplified Near Optimal Downlink Beamforming Schemes in Multi-Cell Environment)

  • 양장훈;김동구
    • 한국통신학회논문지
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    • 제36권12C호
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    • pp.764-773
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    • 2011
  • 다중 안테나 전송은 단일 셀 환경에서 큰 성능 이득을 제공하는 반면에 다중셀 환경에서는 간섭에 의해서 다중 안테나의 이득이 많이 사라지게 된다. 또한, 다중셀 환경에서 효율적인 빔 형성 방법을 계산하는 것은 여전히 어려운 문제중에 하나이다. 먼저 이 논문에서는 다중셀 환경에서 점근적으로 낮은 SNR과 높은 SNR에서 최적의 하향링크 빔행성 방법이 MRT 빔형성과 ZF 빔형성임을 보인다. 둘째, 이 점근적 최적 빔 형성 결과를 이용하여 쌍대 역방향 문제로부터 얻어진 MMSE 빔형성 형태를 갖는 두가지의 준최적 하향 빔형성 방식을 제안한다. 각 빔 형성 방식에 대해서 복잡도에 띠라서 세가지의 다른 부클래스 알고리즘을 고려한다. 모의 실험을 통하여 제안된 준 최적 알고리듬은 복잡도와 성능 사이에 트레이드 오프를 제공함을 보인다.

나노크기의 교질상 영가철 및 자철석에 대한 수용상의 거동특성 (Characterization of Behavior of Colloidal Zero-Valent Iron and Magnetite in Aqueous Environment)

  • 이우춘;김순오;김영호
    • 한국광물학회지
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    • 제28권2호
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    • pp.95-108
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    • 2015
  • 광산배수가 지표에 노출되거나 주변 수계로 유입됨에 따라 나노크기의 철 교질물질이 형성되며, 이러한 철 교질물질은 심미적 오염을 발생시킬 뿐만 아니라 수생태계에도 악영향을 미친다. 이를 제어하기 위해 철 나노물질의 거동특성을 파악하는 것이 매우 중요한데, 아직까지 이에 대한 연구가 미흡하다. 본 연구는 영가철과 자철석을 이용하여 배경용액의 pH와 조성, 그리고 자연유기물에 따른 철 나노물질의 거동특성을 고찰하기 위해 수행되었다. 이를 위해 동적광산란분석기를 이용하여 철 나노물질의 입자크기와 표면 제타전위를 측정하였으며, DLVO (Derjaguin, Landau, Verwey, and Overbeek) 이론에 적용하여 응집 및 분산 등의 거동특성을 비교하였다. 철 나노물질은 영전하점 pH 근처에서는 입자간의 전기적 인력으로 인한 응집이 발생되며, 그보다 pH가 낮거나 높으면 전기적 반발력에 의해 분산이 잘되는 것을 확인하였다. 배경용액 내 양이온이 음이온보다 거동특성에 더 큰 영향을 끼치는 것을 확인하였으며, 특히 1가 양이온보다 2가 양이온이 입자표면간의 전기적인 인력 및 반발력에 더 큰 영향을 주는 것을 알 수 있었다. 수용상의 자연유기물은 철 나노물질을 코팅함으로써 표면을 음전하로 띠게 하여 분산이 잘 되게 하는 것을 확인하였다. 동일한 환경조건에서 자철석보다 영가철이 응집이 더 잘 되는 것으로 나타났는데, 이는 영가철의 낮은 안정성과 빠른 반응성으로 인해 철 산화물로 변질되기 때문인 것으로 판단된다.

2차원 유체- 구조물-지반 상호작용해석 전산프로그램 (A Computer Program for 2-D Fluid-Structure-Soil Interaction Analysis)

  • 김재민
    • 한국지진공학회:학술대회논문집
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    • 한국지진공학회 2000년도 춘계 학술발표회 논문집 Proceedings of EESK Conference-Spring
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    • pp.427-434
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    • 2000
  • This paper presents a computer program for a 2-D fluid-structure-soil interaction analysis. With this computer program the fluid can be modeled by a spurious free 4-node displacement-based fluid element which uses rotational penalty and mass projection technique in conjunction with the one point reduced integration scheme to remove the spurious zero energy modes. The structure and near field soil are discretized by the standard finite elements while the unbounded far field soil are discretized by the standard finite elements while the unbounded far field soil is represented by the frequency dependent dynamic infinite elements. Sine this method models directly the fluid-structure-soil system it can be applied to the dynamci analysis of 2-D liquid storage structure with complex geometry. For the purpose of verification dynamic analyses for tanks on a rigid foundation and on compliant embankment are carried out. Comparison of the present results with those by ANSYS program shows good agreement.

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가스차단기 전류영점영역에서의 열유동특성에 관한 연구 (Thermal Flow Characteristics of Gas Circuit Breakers near Current Zero Period)

  • 이종철
    • 대한전기학회:학술대회논문집
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    • 대한전기학회 2004년도 하계학술대회 논문집 C
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    • pp.1772-1774
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    • 2004
  • Because the physics occurring during an interruption process is not well known, it is not easy to analyze the characteristics of a self-blast circuit breaker neither theoretically nor experimentally. Fortunately the available computational power and the numerical method improved recently make it possible to predict an interruption process as precisely and fast as possible. Therefore many researches using computational methods have been done for the interruption process of interrupters and applied to extend the information such as thermal and dielectric reignition. In this paper, we have simulated the interruption process of SF6 self-blast circuit breakers with the arc plasma during the fault interruption of a 10 kA current. The CFD program used here is coupled with the electromagnetic field analysis, the radiation model and the effects of turbulence. Through this work, we have get further information about the thermal performance as well as the behavior of the arc. The results have been compared with the measured arc voltage.

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Dependence of solar proton peak flux on 3-dimensional CME parameter

  • Park, Jinhye;Moon, Yong-Jae;Lee, Harim
    • 천문학회보
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    • 제40권1호
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    • pp.64.1-64.1
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    • 2015
  • In the present study, we examine the dependence of solar proton peak flux at SOHO and STEREO on 3-D CME parameters (radial speed, angular width, and longitudinal angular separation between its source region and the magnetic footpoints of spacecraft). For this we consider 38 proton enhancements of 16 SEP events observed by SOHO, STEREO-A, and/or B from 2010 August to 2013 June. As a result, we find that the enhancements are strongly dependent on these three parameters. The correlation coefficient between proton peak flux and CME speed is about 0.42 for the cases the footpoints are located inside the lateral boundaries of angular widths, while there is no correlation for the events outside the boundaries. The correlation coefficient between peak flux and angular separation is -0.51. We find that most of strong proton events occur when their angular separations are closer to zero, supporting that most of the proton fluxes are generated near the CME noses rather than their flanks.

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