• 한국환경과학회지
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• 제16권5호
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• pp.541-548
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• 2007

A three-dimensional linear model and the Advanced Regional Prediction System (ARPS) were used to simulate parabola-shaped disturbances and clouds in the lee of a bell-shaped mountain. The ARPS model was compared in the x-y plane against the linear model's analytic solution. Under similar conditions with the linear theory, the ARPS produced well-developed parabola-shaped mountain disturbances and confirmed the features are accounted for in the linear regime. A parabola-shaped cloud in the lee of an isolated bell-shaped mountain was successfully simulated in the ARPS after 6 hours of integration time with the prescribed initial and boundary conditions, as well as a microphysical scheme.

• 한국전자파학회논문지
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• 제21권10호
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• pp.1184-1193
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• 2010

국제적으로 전자파 적합성에 대한 규제 주파수가 보다 높은 주파수로 상향 조정되어 1 GHz 이상의 주파수로 확장되고 있다. 1 GHz 이상에서의 복사 방출 특성은 기존의 1 GHz 이하의 주파수에 비해 전계 강도가 낮고, 복사 패턴이 날카롭고 경사지는 등 매우 다른 복사 특성을 가진다. 본 논문에서는 이중 쇄기형 혼 안테나를 급전기로 사용하는 옵셋 파라볼라 안테나 시스템을 사용하여 1 GHz 이상의 주파수 대역에서 보다 효과적인 측정이 가능함을 확인하였다. 먼저 옵셋 파라볼라 안테나 시스템의 안테나 인자와 전기장 균일도를 계산할 수 있는 간단한 모델을 제시하였으며, 나아가서 표준 노이즈 소스와 제안된 안테나 시스템을 이용하여 1 GHz 이상의 주파수에서 실제적인 복사 방출 및 복사 내성을 평가하였다. 이러한 실험을 통해서 제안된 안테나 시스템이 기존에 널리 사용되고 있는 이중 쇄기형 혼 안테나에 비해 보다 높은 이득과 전력 효율, 그리고 보다 넓은 전기장 균일도를 가지며, 따라서 1 GHz 이상의 전자파 적합성 평가에 효과적으로 이용될 수 있음을 확인하였다.

• 한국산업정보학회논문지
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• 제8권1호
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• pp.18-25
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• 2003

본 논문에서는 비디오 편집 모델에 기반한 디졸브 모델의 특성에 따른 디졸브 검출 방법을 제안한다. 제안된 방법은 각각의 디졸브 구간이 가지는 특성을 반영하기 때문에 디졸브 검출에 적응적이다. 제안된 방법은 2단계로 구성된다. 첫 번째 단계에서는 디졸브 구간의 후보 영역을 찾는다. 동영상의 각 프레임의 분산으로 얻어지는 분산 곡선에서 디졸브 구간은 아래로 볼록한 포물선으로 나타난다. 따라서 분산 곡선의 1차와 2차 미분을 이용하여 디졸브 구간에 대응하는 포물선의 후보 영역을 찾는다. 두 번째 단계에서는 각각의 후보 영역에 대해 디졸브 영역을 검증한다. 후보 영역에서 디졸브 모델에 대응하는 포물선의 골의 분산을 추정하여 디졸브를 판별한다. 골의 분산은 이웃한 두 장면의 분산의 함수로 나타남으로 다양한 분산에서 나타나는 디졸브를 적응적으로 검출할 수 있다. 제안된 방법은 다양한 디졸브를 포함하는 동영상을 대상으로 기존의 방법과 비교 실험하였다. 실험 결과 제안한 방법은 분산의 변화에 상관없이 디졸브를 정확히 검출하였으며 기존의 방법 보다 우수한 결과를 얻었다.

• Computers and Concrete
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• 제31권2호
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• pp.163-171
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• 2023

Face gear transmission is widely used in aerospace shunt-confluence transmission system. Tooth wear is one of the main factors affecting its bearing transmission performance. Furthermore, the installation errors of face gear are inevitable. In order to study the wear mechanism of face gear tooth surface with installation errors, based on tooth contact analysis numerical method and Archard wear theory, the UMESHMOTION subroutine in ABAQUS is developed.Combining with Arbitrary Lagrangian-Eulerian adaptive mesh technology, the finite element mesh wear model of abraded face gear pair is established.The preprocessing conditions are set to generate the inp files.Then,the inp files for each corner are imported and batch processed in ABAQUS.The loading tooth contact problem at each rotation angle is solved and the load distribution coefficient among gear tooth, tooth root bending stress, tooth surface contact stress and loaded transmission error are obtained. Results show that the tooth root wear is the most serious and the wear at the pitch cone is close to 0.The wear law of tooth surface along tooth width direction is convex parabola and the wear law along tooth height direction is concave parabola.

• 한국농공학회지
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• 제42권5호
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• pp.78-83
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• 2000

When a sea-dike is constructed on soft soils, it is much difficult to calculate ground deformation caused by forced displacements. In this study , a series of laboratory model tests have been performed to investigate the ground deformation under a constructed sea-dike on soft soils. Construction sequence of sea-dike embankment was assumed such as constructed by quarry first and followed by soils adjacent to quarry embankment. as test data and displacement in subsoils have been analyzed, it seems that deformation is caused by general shear failure. the shape of ground deformation caused by forced displacements was well defined be parabola . Upon comparing profiles and depth of forced displacement from the model test to those based on stress-baring capacity method commonly used, it has been found that deformation prediction using stress-bearing capacity method was not exact at the edge of loading.

• Journal of Magnetics
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• 제22권2호
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• pp.291-298
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• 2017

In this paper, the distribution of internal magnetic induction intensity of oil-film bearing twined solenoids was proposed. The magnetic field was generated by solenoids and magnetized bearing. The magnetized bearing was simplified as solenoid model. The mathematical model of magnetic induction intensity at any point of finite solenoid was deduced. Through experiment method, the distribution of the internal magnetic induction intensity of oil-film bearing and the magnetizing current formula of bearing was obtained. Further, the magnetic induction intensity distribution of magnetization bearing was solved successfully. The results showed that the magnetic induction was a second-degree parabola with open upwards along the axial plane and the distribution of magnetic induction intensity was opposite to the rule of magnetic induction intensity generated by solenoids. In addition, the magnetic flux density increased linearly with the increase of current.

• 한국항만학회지
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• 제8권2호
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• pp.67-77
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• 1994

A time-domain numerical model is developed to examine the performance of a wave energy focusing structure in combined waves and a current. With the current assumed to be slow and the structure fully submerged, the wave-current interaction problem is reduced to a wave scattering problem in a uniform current. The diffraction of incident waves around a narrow berm is considered. The shape of the berm is defined by a parabola, imitating that of an optical reflector. The energy focus is achieved by reflecting the incident waves through a predetermined focal point. Through the numerical simulations, the numerical model is shown to be effective in modeling the wave-current interaction problem, and the current speed and direction are shown to affect significantly the location, amplitude and sharpness of the focus.

• 한국전자파학회논문지
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• 제8권1호
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• pp.73-82
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• 1997

본 논문은 77 GHz대의 차량용 레이다 안테나에 응용이 가능한 파라볼라 안테나, 렌즈 안테나,$32\times8$ 마이크로 스트립 페치 안테나 등에 대한 설제 및 실험 결과를 다루었다 파라볼라 안테나는 f /D=0.263 및 $7cm\times10cm$의 크기로 설계하였으며, 피드 안테나는 도파관 WR12를 개방한 개방 도파관 형태로 사용하였다. 렌즈 안테나 는 f /D=0.5 및 직경 lOcm로 하여 양딸록 및 반볼록 구조에 대하여 실험하였다. 그리고 페치 어레이 안테나는 페치 안테나에 대한 전송선로 모멜을 이용하여 설계하였다 .. 3개의 안테나에 대한 3 dB 빔폭, 방사 패턴, 이득 등 은 이론치와 실험치가 잘 일치하는 결과를 얻었으나, 페치 어레이 안테나인 경우에 피드 망 및 마이크로스트립 동축선-도파관 전이에 따른 손설로 인하여 이득이 약 25 dB 정도 감소를 보였다.

• Journal of Electrical Engineering and Technology
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• 제10권2호
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• pp.625-633
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• 2015

The effect of altitude on thermal conduction, surface temperature, and thermal radiation of partial arc was investigated on the basis of molecular gas dynamics to facilitate a deep understanding of the pollution surface discharge mechanism. The DC flashover model was consequently modified at high altitude. The validity of the modified DC flashover model proposed in this paper was proven through a comparison with the results of high-altitude simulation experiments and earlier models. Moreover, the modified model was found to be better than the earlier modified models in terms of forecasting the flashover voltage. Findings indicated that both the thermal conduction coefficient and the surface thermodynamics temperature of partial arc had a linear decrease tendency with the altitude increasing from 0 m to 3000 m, both of which dropped by approximately 30% and 3.6%, respectively. Meanwhile, the heat conduction and the heat radiation of partial arc both had a similar linear decrease of approximately 15%. The maximum error of DC pollution flashover voltage between the calculation value according to the modified model and the experimental value was within 6.6%, and the pollution flashover voltage exhibited a parabola downtrend with increasing of pollution.

• Journal of Astronomy and Space Sciences
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• 제28권3호
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• pp.163-172
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• 2011

An intensive analysis of 185 timings of WZ Cep, including our new three timings, was made to understand the dynamical picture of this active W UMa-type binary. It was found that the orbital period of the system has complexly varied in two cyclical components superposed on a secularly downward parabola over about 80y. The downward parabola, corresponding to a secular period decrease of $-9.{^d}97{\times}10^{-8}y^{-1}$, is most probably produced by the action of both angular momentum loss (AML) due to magnetic braking and mass-transfer from the massive primary component to the secondary. The period decrease rate of $-6.^{d}72{\times}10^{-8}y^{-1}$ due to AML contributes about 67% to the observed period decrease. The mass flow of about $5.16{\times}10^{-8}M_{\odot}y^{-1}$ from the primary to the secondary results the remaining 33% period decrease. Two cyclical components have an $11.^{y}8$ period with amplitude of $0.^{d}0054$ and a $41.^{y}3$ period with amplitude of $0.^{d}0178$. It is very interesting that there seems to be exactly in a commensurable 7:2 relation between their mean motions. As the possible causes, two rival interpretations (i.e., light-time effects (LTE) by additional bodies and the Applegate model) were considered. In the LTE interpretation, the minimum masses of $0.30M_{\odot}$ for the shorter period and $0.49M_{\odot}$ for the longer one were calculated. Their contributions to the total light were at most within 2%, if they were assumed to be main-sequence stars. If the LTE explanation is true for the WZ Cep system, the 7:2 relation found between their mean motions would be interpreted as a stable 7:2 orbit resonance produced by a long-term gravitational interaction between two tertiary bodies. In the Applegate model interpretation, the deduced model parameters indicate that the mechanism could work only in the primary star for both of the two period modulations, but could not in the secondary. However, we couldn't find any meaningful relation between the light variation and the period variability from the historical light curve data. At present, we prefer the interpretation of the mechanical perturbation from the third and fourth stars as the possible cause of two cycling period changes.