• 지구물리와물리탐사
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• 제10권4호
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• pp.393-398
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• 2007

흑색 셰일이 존재하는 지역에서 탄성파 주시 토모그래피 탐사를 수행하였다. 흑색 셰일은 퇴적암 기원으로 속도 이방성을 가지는 것으로 알려져 있기 때문에, 주시 토모그래피를 적용하여 정확한 역산 모형을 도출하기 위하여 이방성을 역산 과정에 적용하였다. 속도 이방성 계수는 탐사에서 획득한 자료에 대하여 탄성파의 초동시간에 의한 직선파선으로 가정한 속도와 전파각이 형성하는 이방성 타원의 형태로부터 추출할 수 있었으며, 이로부터 수평방향의 전파속도가 수직방향의 전파속도보다 빠름을 확인할 수 있었다. 속도 이방성 계수는 역산 과정에 적용되어 실제 지질구조에 부합하는 속도 구조를 획득하였다. 속도 이방성을 고려한 역산은 동일한 지역에서 3개의 구간에서 수행하였고, 각각의 결과는 지표지질 및 시추결과와 비교하여 높은 유사성을 보여주었다.

• 오토저널
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• 제2권1호
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• pp.32-38
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• 1980

In the case of a automobile marking skid on road for a period of braking, in general, the automobile velocity just before rapid braking can be obtained by evaluating the coefficient of friction between tires and road. Up to now, the coefficient of friction has been derived from mean velocity measured by a time watch, but the automobile velocity obtained in this manner would be deviated from actual value considerably, due to errors arising from not only measuring time but other various factors. In this paper the presumption method of automobile velocity by accelerometer is presented so as to improve the accuracy of measurement, and to determine the velocity readily. The results obtained in this experiment show that the frictional coefficients between tires and road under the given experimental conditions are considered to take linear relation over the fixed velocity limits 30km/h to 50km/h while for the same limits of velocities the coefficients of friction by the time watch method are not valid ar low velocity range. It will be seen that the former is simple and reliable whilst the latter is cumbersome and unreliable.

• 지구물리와물리탐사
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• 제9권1호
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• pp.108-113
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• 2006

일반적인 물리탐사기법은 도심지 내에서 구조물, 전도성 지하매설물, 차량 등 인공 잡음으로 인하여 그 적용성에 많은 제약을 받는다. 특히 이 과업은 철도가 운행 중인 철로 하부의 지반 정보의 획득을 목적으로 하는데, 이를 위한 일반적인 물리탐사 적용이 어려웠으며 그 대안으로 선형배열 상시진동 탄성파탐사를 적용하였다. 상시진동 탐사(mircotremor survey)기법에는 철로를 운행하는 기차와 주변 도로의 차량에 의한 진동이 오히려 양호한 송신원으로 활용 될 수 있다. 선형배열 상시진동 탐사기법에서는 일반적인 굴절법 장비를 이용하여 일상적인 진동을 기록하고, 파동장의 변환을 수행하여 표면파의 분산곡선을 얻는다. 이후 발췌한 분산곡선에 대한 반복적인 수치모델링을 통하여 전단파 속도를 구한다. 이 과업에서는 기존 철로를 따라 하부의 터널심도까지의 전단파 속도를 전체 터널구간에 대하여 얻기 위하여 40 m 간격으로 선형배열을 이동하면서 자료를 획득하였다. 측선상의 시추를 통하여 회수한 코어를 이용한 실내시험을 통한 RMR 의 구성요소 중 하나인 일축압축강도와 전단파 속도와의 높은 상관관계를 확인하여 RMR이 전단파 속도와 연관성이 있음을 유추할 수 있었다. 시추공에서 수행한 SPS 검층에서 획득한 전단파 속도와 RMR의 비교한 결과 전단파 속도와 RMR이 높은 상관관계에 있음을 확인할 수 있었다. 상시진동 탐사기법을 통하여 획득한 전단파 속도 역시 RMR과의 양호한 상관관계를 나타냄을 알 수 있었다. 이러한 상관관계를 이용하여 도심지 철도터널 전체 구간에서 터널 설계시 필수적인 암반분류를 위한 RMR 추정이 가능하였다.

• Wind and Structures
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• 제38권4호
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• pp.231-244
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• 2024

As wind farms expand into low wind speed areas, an increasing number are being established in mountainous regions. To fully utilize wind energy resources, it is essential to understand the details of mountain flow fields. Reconstructing the wind speed field in complex terrain is crucial for planning, designing, operation of wind farms, which impacts the wind farm's profits throughout its life cycle. Currently, wind speed reconstruction is primarily achieved through physical and machine learning methods. However, physical methods often require significant computational costs. Therefore, we propose a Full Convolutional Neural Network (FCNN)-based reconstruction method for mountain wind velocity fields to evaluate wind resources more accurately and efficiently. This method establishes the mapping relation between terrain, wind angle, height, and corresponding velocity fields of three velocity components within a specific terrain range. Guided by this mapping relation, wind velocity fields of three components at different terrains, wind angles, and heights can be generated. The effectiveness of this method was demonstrated by reconstructing the wind speed field of complex terrain in Beijing.

• Journal of Advanced Marine Engineering and Technology
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• 제28권3호
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• pp.441-450
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• 2004

The velocity distribution of gas molecules from the experimental results was confirmed as the same with the Maxwell-Boltzmann's theoretical results within the experimental error. This study is on the realization of the Maxwell-Boltzmann's velocity distribution of gas molecules by the molecular dynamics(MD) method. The Maxwell-Boltzmann's velocity distribution of gas molecules is extremely important to confirm the equilibrium state because the properties of a thermodynamic system shall be obtained from the system's equilibrium configuration in the MD method. This study is the first trial in the successive researches to calculate the properties of a thermodynamic system by the computer simulations. We confirmed that the maxwell-boltzmann's velocity distribution is developed in some transient time after starting a simulation and dependent on the size of a system. Also it is found that the velocity distribution has no relation with an initial configuration of gas molecules.

• Journal of Electrical Engineering and Technology
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• 제13권5호
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• pp.2067-2073
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• 2018

This paper will present the design of a novel-type velocity-controllable electromagnetic coil launcher (EMCL). By studying the influence of initial capacitor voltage on the velocity of an EMCL, the launcher voltage can be set to precisely adjust the velocity of projectile launching. The simulation of voltage and velocity in relation to time is obtained by Maxwell software. The experimental data show that for the launch accuracy to be achievable, the actual precision is 2%. Because of the excellent performance of Velocity-controllable EMCL, it can replace the air gun and applied to split Hopkinson pressure bar (SHPB).

• 한국해양학회지
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• 제12권2호
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• pp.67-74
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• 1977

With the serial observation data and the tidal records at Busan and Izuhara from 1966 to 1973, the geostrophic current velocity and its relation to the difference of mean sea level of both sides were studied in order to estimate indirectly the average current velocity from the tidal observations. The results shows that the current velocity is estimated by the relationship V=4.016(H-98.3) with the 95% confidence limits of V 4.2 cm/sec. Ther relationship between the observed current velocity and the simultaneous daily mean sea level difference shows a similar result, V=4.717(H-99.6). The two equations were applied to the evaluation of annual variations of current velocity from the average monthly mean sea level data of both stations.

• 대한기계학회논문집B
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• 제20권10호
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• pp.3282-3292
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• 1996

Flow velocity was measured using a hot wire anemometer. Turbulence intensity was in proportion to mean flow velocity regardless of swirl velocity. And integral length scale has proportional relation with swirl velocity regardless of measurement position. Flame speed calculated by radius of visualized flame was increased and then decreased according to lapse of time from spark. Maximum flame speed was increased according to increase of turbulence intensity. Burning speed and flame transport effect increased with increase of swirl velocity, but ratio of burning speed to flame speed decreased with increased of swirl velocity. Mass fraction burned versus volume fraction burned was increased in proportion to the increase of turbulence intensity, caused by increase of combustion promotion effect according to increase of turbulence intensity and scale.

• 천문학회지
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• 제49권5호
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• pp.193-198
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• 2016

Early-type galaxies (ETGs) are supposed to follow the virial relation $M=k_e{\sigma}^2R_e/G$, with M being the mass, σ_* being the stellar velocity dispersion, R_e being the effective radius, G being Newton's constant, and k_e being the virial factor, a geometry factor of order unity. Applying this relation to (a) the ATLAS^3D sample of Cappellari et al. (2013) and (b) the sample of Saglia et al. (2016) gives ensemble-averaged factors 〈k_e〉 = 5.15 ± 0.09 and 〈k_e〉 = 4.01 ± 0.18, respectively, with the difference arising from different definitions of effective velocity dispersions. The two datasets reveal a statistically significant tilt of the empirical relation relative to the theoretical virial relation such that $M{\propto}({\sigma}^2_*R_e)^{0.92}$. This tilt disappears when replacing R_e with the semi-major axis of the projected half-light ellipse, a. All best-fit scaling relations show zero intrinsic scatter, implying that the mass plane of ETGs is fully determined by the virial relation. Whenever a comparison is possible, my results are consistent with, and confirm, the results by Cappellari et al. (2013). The difference between the relations using either a or R_e arises from a known lack of highly elliptical high-mass galaxies; this leads to a scaling (1 - ϵ ) ∝ M^0.12, with ϵ being the ellipticity and $R_e=a\sqrt[]{1-{\epsilon}}$. Accordingly, a, not R_e, is the correct proxy for the scale radius of ETGs. By geometry, this implies that early-type galaxies are axisymmetric and oblate in general, in agreement with published results from modeling based on kinematics and light distributions.

• E2M - 전기 전자와 첨단 소재
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• 제10권3호
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• pp.268-273
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• 1997

In this paper the transient electron transport in GaAs bulk is simulated by using ensemble Monte Carlo method. To analyze the transient electron transport the 10000 electrons in the .GAMMA. valley are simulated simultaneously for 10 picoseconds. The electric field-velocity relation is obtained. The high impurity density reduces the negative differential resistance effect. The result of transient average velocity shows the electron velocity in the transient state is faster than that in the steady state. This transient velocity overshoot is caused by the intervalley scattering mechanism. And we confirmed the fact that the energy relaxation time is longer than the momentum relaxation time.