• Title/Summary/Keyword: High Velocity

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Science High-School Students Understanding of Velocity & Acceleration and of the Motion of Bob When Tension is Removed in a Simple Pendulum

  • Kim, Young-Min;Jeong, Seong-Oh
    • Journal of The Korean Association For Science Education
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    • v.26 no.5
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    • pp.611-619
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    • 2006
  • The aims of this study are to investigate science high school students' understanding of velocity and acceleration of a simple pendulum bob, and to investigate their understanding of inertia and gravitational force in the motion of a pendulum bob when the tension is removed. For the study, 46 students that had already studied the physical, concepts in simple pendulum were sampled from a science high school in a large city in Korea. For a comparison with general high school students' conceptions, 49 students were sampled from a general high school in the same city. The test tool for the investigation consisted of four drawing and simple-answering type questions developed by the authors. The outcomes of the study revealed that a substantial number of science high school students have misconceptions concerning acceleration in pendulum motion, and that many of them do not understand the relationship between force and acceleration. In addition, the results of the study showed that more than 30% of the students drew the path of a bob going along the tangential direction at the highest point of the motion, and approximately 20% of them drew the path of a bob falling straight down at the lowest point of the motion.

Experimental Studies on Eye Injury Risks by Different BB Pellet Materials (BB Pellet 재질에 따른 안구 손상 위험성에 관한 실험적 연구)

  • Kim, Hyung-Suk;Park, Dal-Jae
    • Journal of the Korean Society of Safety
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    • v.27 no.2
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    • pp.20-24
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    • 2012
  • Experimental studies were performed to investigate the eye injury risks by different BB pellet materials. Four different BB pellet materials were used: plastic (P), silicon (S), rubber (R) and plastic covered with silicon (SR). The BB pellet images penetrating into the gelatine simulant were recorded by a high-speed video camera. The results obtained from the different pellet materials were discussed in terms of impact velocity and penetration depth; threshold velocity and projectile sectional density; eye injury risks by normalized energies. It was found that the P pellets caused higher impact velocity while the lower was SR pellets. The penetration depth and threshold velocity of the pellets were dependent on the impact velocity of the pellets, and the P pellets resulted in the higher eye injury risk while the lower was SP.

Prediction of velocity and attitude of a yacht sailing upwind by computational fluid dynamics

  • Lee, Heebum;Park, Mi Yeon;Park, Sunho;Rhee, Shin Hyung
    • International Journal of Naval Architecture and Ocean Engineering
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    • v.8 no.1
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    • pp.1-12
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    • 2016
  • One of the most important factors in sailing yacht design is accurate velocity prediction. Velocity prediction programs (VPP's) are widely used to predict velocity of sailing yachts. VPP's, which are primarily based on experimental data and experience of long years, however suffer limitations when applied in realistic conditions. Thus, in the present study, a high fidelity velocity prediction method using computational fluid dynamics (CFD) was proposed. Using the developed method, velocity and attitude of a 30 feet sloop yacht, which was developed by Korea Research Institute of Ship and Ocean (KRISO) and termed KORDY30, were predicted in upwind sailing condition.

Observational Constraints on the Formation of the Milky Way's Disk

  • Han, Doori;Lee, Young Sun;Kim, Youngkwang;Beers, Timothy C.
    • The Bulletin of The Korean Astronomical Society
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    • v.42 no.2
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    • pp.51.4-52
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    • 2017
  • We present the derived kinematic characteristics of low-${\alpha}$ thin-disk and high-${\alpha}$ thick-disk stars in the Milky Way, investigated with a sample of about 33,900 G- and K-type dwarfs from the Sloan Extension for Galactic Understanding and Exploration (SEGUE). Based on the level of ${\alpha}$-element enhancement as a function of [Fe/H], we separate our sample into thin- and thick-disk stars and then derive mean velocity, velocity dispersion, and velocity gradients for the U, V and W velocity components, respectively, as well as the orbital eccentricity distribution. There are notable gradients in the V velocity over [Fe/H] in both populations: -23 km s-1 dex-1 for the thin disk and +44 km s-1 dex-1 for the thick disk. The velocity dispersion of the thick disk decrease with increasing [Fe/H], while the velocity.

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Characteristics of Laminar Lifted Flame in High Temperature Coflow (고온 동축류에서 층류 화염의 부상특성)

  • Kim, Kil-Nam;Won, Sang-Hee;Cha, Min-Suk;Chung, Suk-Ho
    • Journal of the Korean Society of Combustion
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    • v.7 no.2
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    • pp.1-6
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    • 2002
  • Characteristics of laminar lifted flames of propane highly-diluted with nitrogen have been investigated at various temperatures of coflow air. At various fuel mole fractions, the base of laminar lifted flames has the structure of tribrachial (or triple) flame. The liftoff heights are correlated well with the stoichiometric laminar burning velocity considering initial temperature at a given coflow velocity. It shows that lifted flames are stabilized on the basis of the balance mechanism between local flow velocity and the propagation speed of tribrachial flame, regardless of the temperature of coflow and fuel mole fraction. Lifted flames exist for a jet velocity even smaller than the stoichiometric laminar burning velocity, and liftoff velocity increases more rapidly than stoichiometric laminar burning velocity as coflow temperature increases. These can be attributed to the buoyancy effect due to the density difference.

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A study of seismic velocity and amplitude variation around underground cavity (지하 공동에 대한 탄성파 속도 및 진폭 변화에 관한 연구)

  • Lee, Sang-Chul;Oh, Seokhoon;Sohn, Kwon-Ik;Suh, Baek-Soo
    • Journal of Industrial Technology
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    • v.27 no.A
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    • pp.9-14
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    • 2007
  • This study was designated to clarify the aspect of the wave propagation around the cavity. The change of traveltime and amplitude of the seismic wave was observed according to the various wave velocities of the cavity. The seismic wave detour or penetrate the cavity depending on the seismic velocity of the in-filled material. Generally, seismic wave detours toward high velocity zone around the cavity, and when the velocity of the cavity material reaches to 80 % of the base rock, the wave penetrates the cavity. The traveltime of the detouring seismic wave is not sensitive to the change of the cavity velocity, but as the velocity of the cavity increases, the fall of the amplitude was reduced. The penetrating wave showed the steeply increasing amplitude due to the reiteration of the detouring wave.

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A Study of Slow Wave Instability on High Power Generator (대 출력 발생장치의 지파불안정성 연구)

  • Kim, Won-Sop;Kim, Jong-Man
    • Proceedings of the KIEE Conference
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    • 2011.07a
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    • pp.2109-2109
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    • 2011
  • High power microwave sources operating in relativistic regions, high current reletivistic electron beams are obtained by using cold cathodes with the help of explosive emission. For these relativistic devices, the pulsed power and magnetic field systems are very large and heavy. The phase velocity of electromagnetic mode should be showed down close to the beam velocity, ensuring enough beam coupling with electromagnetic modes. By using the annular electron beam, a weakly relativistic oversized bwo consisting of rectangularly corrugated cylindrical waveguide is demonstrated.

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INTERACTION OF HIGH VELOCITY CLOUDS WITH MAGNETIZED DISKS: THREE-DIMENSIONAL NUMERICAL SIMULATIONS

  • SANTILLAN ALFREDO;FRANCO JOSE;KIM JONGSOO
    • Journal of The Korean Astronomical Society
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    • v.37 no.4
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    • pp.233-235
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    • 2004
  • High-velocity clouds are flows of neutral hydrogen, located at high galactic latitudes, with large velocities ($[VLSR]{\ge} 100 km/s$) that do not match a simple model of circular rotation for our Galaxy. Numerical simulations have been performed for the last 20 years to study the details of their evolution, and their possible interaction with the Galactic disk. Here we present a brief review of the models that have been already published, and describe newly performed three-dimensional magnetohydrodynamic simulations.

The Application of P/M Advanced Techniques to Sintered Gears

  • Chongxi, Bao;Zhouqiang, Shen;Zhengping, Shu
    • Proceedings of the Korean Powder Metallurgy Institute Conference
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    • 2006.09b
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    • pp.987-988
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    • 2006
  • The processes of P/M affect the properties of sintered gears. The different techniques of P/M lead to the different properties of sintered gears. This paper summarizes new progress in powder metallurgy for sintered gears. These progresses include warm compaction, high velocity compaction, sinter hardening, high temperature sintering, infiltration, CNC powder press and surface densification etc.

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A Study on the Techniques to Evaluate Carbody Accelerations after a Train Collision (충돌 후 열차의 차체 가속도 평가 기법 연구)

  • Kim, Joon-Woo;Koo, Jeong-Seo
    • Transactions of the Korean Society for Noise and Vibration Engineering
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    • v.20 no.5
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    • pp.477-485
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    • 2010
  • In this study, we suggested several approaches to evaluate the collision acceleration of a carbody under the article 16 of the Korean rolling stock safety regulations. There are various methods to evaluate the rigid body accelerations such as the displacement comparison method by double integration of filtered acceleration data, the velocity comparison method by direct integration of filtered acceleration data, and the analysis method of a velocity-time curve. We compared these methods one another using the 1D dynamic simulation model of Korean high-speed EMU composed of nonlinear springs or bars, dampers, and masses. From the simulation results, the velocity-time curve analysis method and the displacement comparison method are recommended to filter high frequency oscillations and evaluate the maximum and average accelerations of a carbody after a train collision.