• 제목/요약/키워드: Dispersion Radius

검색결과 68건 처리시간 0.03초

SPH 기법을 이용한 고속충돌 파편의 운동에너지와 분산거동 연구 (A Study on the Kinetic Energy and Dispersion Behavior of High-velocity Impact-induced Debris Using SPH Technique)

  • 사공재;우성충;김태원
    • 대한기계학회논문집A
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    • 제40권5호
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    • pp.457-467
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    • 2016
  • 본 연구에서는 입자완화 유체동역학기법을 이용하여 고속충돌에 의해 생성된 파편 및 파편운의 분산거동을 고찰하였다. 충격구와 표적판은 모두 알루미늄 소재를 대상으로 하였으며 해석을 통해 예측한 파편운의 장축 및 단축의 길이와 참고문헌의 실험값을 비교하여 기법의 타당성을 검증하였다. 검증된 SPH 기법을 기반으로 1.5~4 km/s의 속도 범위에서 고속충돌 및 파괴 해석을 수행하였으며 이에 따른 파편의 분산 거동을 운동에너지 관점에서 평가하였다. 표적판 뒤에 배치된 관측판상에 분포된 파편의 최대 분산반경은 충돌속도가 증가함에 따라 증가하였다. 충돌시 발생하는 파편의 분산 거동을 바탕으로 손상범위 예측을 위한 경험식을 도출하였고, 파편 운동에너지의 95 %는 최대분산반경의 50 % 이내에 집중됨을 확인하였다.

자갈 다공성매질에서 수리평균반경과 수리분산 매개변수의 상관성에 관한 실험적 연구 (An experimental study on the correlation of hydraulic mean radius and hydrodispersive parameters in rockfill porous media)

  • 한일영;이재정;김규범
    • 한국수자원학회논문집
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    • 제54권11호
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    • pp.863-873
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    • 2021
  • 다공성 매질에서 오염물 이동에 지배적인 기작인 역학적 분산은 공극 내 유속 차이에 의해서 발생한다. 종분산계수와 종분산지수는 이송확산 모형의 수리분산 매개변수이며, 실험을 통하여 얻어야만 한다. 수리평균반경은 공극 내 물의 흐름 양의 크기와 강도를 표현할 수 있으며, 매질의 물리적 특성인자를 이용하여 계산할 수 있다. 본 연구는 순간주입 추적자실험을 통하여 자갈 다공성매질에서 수리평균반경을 이용하여 종분산지수를 구할 수 있는 거듭제곱형의 경험식을 도출하였다. 경험식은 스케일상수 계산식이 포함되어 있어 이동거리에 따른 종분산지수의 산정이 가능하며, 소규모 유량의 균질한 자갈로 구성된 수로에 적용이 가능할 것으로 기대된다.

A Simple Mlodel for Dispersion in the Stable Boundary Layer

  • Sung-Dae Kang;Fuj
    • 한국환경과학회지
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    • 제1권1호
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    • pp.35-43
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    • 1992
  • Handling the emergency problems such as Chemobyl accident require real time prediction of pollutants dispersion. One-point real time sounding at pollutant source and simple model including turbulent-radiation process are very important to predict dispersion at real time. The stability categories obtained by one-dimensional numerical model (including PBL dynamics and radiative process) are good agreement with observational data (Golder, 1972). Therefore, the meteorological parameters (thermal, moisture and momentum fluxes; sensible and latent heat; Monin-Obukhov length and bulk Richardson number; vertical diffusion coefficient and TKE; mixing height) calculated by this model will be useful to understand the structure of stable boundary layer and to handling the emergency problems such as dangerous gasses accident. Especially, this simple model has strong merit for practical dispersion models which require turbulence process but does not takes long time to real predictions. According to the results of this model, the urban area has stronger vertical dispersion and weaker horizontal dispersion than rural area during daytime in summer season. The maximum stability class of urban area and rural area are "A" and "B" at 14 LST, respectively. After 20 LST, both urban and rural area have weak vertical dispersion, but they have strong horizontal dispersion. Generally, the urban area have larger radius of horizontal dispersion than rural area. Considering the resolution and time consuming problems of three dimensional grid model, one-dimensional model with one-point real sounding have strong merit for practical dispersion model.al dispersion model.

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TURBULENCE IN THE OUTSKIRTS OF THE MILKY WAY

  • Sanchez-Salcedo, F.J.;Santillan, A.;Franco, Jose
    • 천문학회지
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    • 제40권4호
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    • pp.171-177
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    • 2007
  • In external galaxies, the velocity dispersion of the atomic hydrogen gas shows a remarkably flat distribution with the galactocentric radius. This has been a long-standing puzzle because if the gas velocity dispersion is due to turbulence caused by supernova explosions, it should decline with radius. After a discussion on the role of spiral arms and ram pressure in driving interstellar turbulence in the outer parts of galactic disks, we argue that the constant bombardment by tiny high-velocity halo clouds can be a significant source of random motions in the outer disk gas. Recent observations of the flaring of H I in the Galaxy are difficult to explain if the dark halo is nearly spherical as the survival of the streams of tidal debris of Sagittarius dwarf spheroidal galaxy suggests. The radial enhancement of the gas velocity dispersion (at R > 25 kpc) due to accretion of cloudy gas might naturally explain the observed flaring in the Milky Way. Other motivations and implications of this scenario have been highlighted.

Spectroscopic observation of the massive high-z (z=1.48) galaxy cluster SPT-CL J2040-4451 using Gemini Multi-Object Spectrographs

  • Kim, Jinhyub;Jee, Myungkook J.;Kim, Seojin F.;Ko, Jongwan
    • 천문학회보
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    • 제44권1호
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    • pp.74.2-74.2
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    • 2019
  • Mass measurement of high-redshift galaxy clusters with high accuracy is important in constraining cosmological parameters. Extremely massive clusters at high redshift may impose a serious tension with the current ΛCDM paradigm. SPT-CL J2040-4451 at z=1.48 is considered one such case given its redshift and mass estimate inferred from the SZ data. The system has also been confirmed to be indeed massive from a recent weak-lensing (WL) analysis. Comparison of the WL mass with the spectroscopic result may provide invaluable information on the dynamical stage of the system. However, the existing spectroscopic coverage of the cluster is extremely poor; only 6 blue star-forming galaxies have been found within the virial radius, which results in highly inflated and biased velocity dispersion. In this work, we present a spectroscopic analysis of the member candidates using Gemini Multi-Object Spectrographs (GMOS) observation in Gemini South. The observation was designed to find early-type member galaxies within the virial radius and to obtain reliable velocity dispersion. We explain our selection scheme and preliminary results of the spectra. We also compare the dynamical mass estimate inferred from the velocity dispersion with the WL mass.

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지파 도파관을 이용한 마이크로파 출력 실험 연구 (A Study of Microwave Output Experiment of Slow Wave Waveguide)

  • 김원섭
    • 전기학회논문지P
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    • 제58권4호
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    • pp.465-468
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    • 2009
  • The dispersion relation and the characteristic of propagation are measured. The measurements of the dispersion relation are observed by a plunger method employed in slow plasma density by pumping microwaves on the axis are observed in plasma loaded slow wave structure. In case of small incident microwave powers the well known plasma density cavity are observed. At the axial positions of minimal radius in the waveguides, the maxima og the electron density, the plasma potential and the RF electric field are observed in cases of high-power microwaves.

켈빈 식과 이의 나노 계에서의 구실 (Kelvin Equation and Its Role in Nano Systems)

  • 임경희
    • 한국응용과학기술학회지
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    • 제23권1호
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    • pp.54-62
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    • 2006
  • Kelvin equation is revisited, which accounts for important phenomena observed frequently in nano-dispersion systems. They include vapor pressure increase for curved interfaces, nucleation, capillary condensation, Ostwald ripening and so on. The smaller the radius of curvature is, the more significant Kelvin equation becomes. Therefore, its meaning, curvature effect, and importance are examined and discussed.

대단위발전소의 대기오염물질 확산에 관한 모델링 및 평가에 관한 연구 (Modeling and Evaluation on the Dispersion of Air Pollutants in the Large Scale Thermal Power Plant)

  • 전상기;이성철
    • 환경영향평가
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    • 제6권2호
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    • pp.81-92
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    • 1997
  • This paper presents the results from the comparison analysis and evaluation between the air pollutant dispersion modeling results and the observation data in the area within a 10 km radius from the Boryong thermal power plants. The observation data used in this study were the air pollutant concentrations which had been continuously measured from 8 locations around the Boryong power plants by TMS(tele-monitoring system) for 3 months from September to November, 1996. The short-term and long-term predictions were carried out using ISC3 model and LPDM(Lagrangian Panicle Dispersion Model). The results of ISC3 modeling in a short-term showed highly as 0.7 in a correlation coefficient, but in a long-term showed just 0.54. On the other hand, LPDM showed 0.78 in a correlation coefficient for a long-term, but in a short-term showed highly value than the observation concentrations.

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시추공경과 공내검층기가 분산곡선에 미치는 영향에 대한 비교 연구 (A comparative study of borehole size and tool effect on dispersion curves)

  • 조유준;김종만;김영화
    • 지구물리와물리탐사
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    • 제12권1호
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    • pp.154-162
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    • 2009
  • 단극 및 쌍극 음원을 이용하여 S파속도 결정에 큰 영향을 미치는 분산특성을 연구하였다. 이를 위하여 동일한 물성을 가지면서 공경을 달리하는 3종류의 시추공모형(${\Phi}520\;mm$. ${\Phi}150\;mm$and ${\Phi}76\;mm$)을 중심으로 이른 분산곡선을 구하고 공경과 공내검층기 존재 유무에 따른 분산 특성의 변화를 비교 분석하였다. 분산곡선의 형태는 단극음원에서 시추공 내의 공내검층기 유무에 크게 영향을 받지 않고 비슷하게 나타난 반면에 쌍극음원에서는 공내검층기 유무가 큰 차이를 보였다. 반면에 절단주파수에서는 쌍극음원에 비하여 단극음원에서 공내검층기 유무에 따른 차이가 크며 특히 소구경 시추공에서 큰 차이를 보여 단극음원을 이용한 토목시추공 음파검층에서 주파수 선택이 매우 중요한 변수가 될 수 있음을 보였다. 수치모델링결과, 절단주파수와 시추공경과의 관계는 기존에 알려진 일반적인 반비례 관계보다는 지수함수적으로 감소하는 관계임을 확인하였으며, 분산모드의 종류나 공내검층기 유무에 상관없이 각 환경에 있어서의 절단주파수 값을 지수함수로 표시할 수 있었다. 특정 시추공 환경에서의 분산곡선 및 분산특성들은 과거 연구결과들로부터 비교적 잘 알려져 있지만 분산곡선의 직접 비교에 의하여 분산특성에 미치는 시추공경과 공내측정기 영향을 보다 구체적으로 밝힐 수 있었다.

A Simple Model for Dispersion in the Stable Boundary Layer

  • Kang Sung-Dae;Kimura Fujio;Lee Hwa-Woon;Kim Yoo-Keun
    • Environmental Sciences Bulletin of The Korean Environmental Sciences Society
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    • 제1권1호
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    • pp.35-43
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    • 1997
  • Handling the emergency problems such as Chemobyl accident require real time prediction of pollutants dispersion. One-point real time sounding at pollutant source and simple model including turbulent-radiation process are very important to predict dispersion at real time. The stability categories obtained by one-dimensional numerical model (including PBL dynamics and radiative process) are good agreement with observational data (Golder, 1972). Therefore, the meteorological parameters (thermal, moisture and momentum fluxes; sensible and latent heat; Monin-Obukhov length and bulk Richardson number; vertical diffusion coefficient and TKE; mixing height) calculated by this model will be useful to understand the structure of stable boundary layer and to handling the emergency problems such as dangerous gasses accident. Especially, this simple model has strong merit for practical dispersion models which require turbulence process but does not takes long time to real predictions. According to the results of this model, the urban area has stronger vertical dispersion and weaker horizontal dispersion than rural area during daytime in summer season. The maximum stability class of urban area and rural area are 'A' and 'B' at 14 LST, respectively. After 20 LST, both urban and rural area have weak vertical dispersion, but they have strong horizontal dispersion. Generally, the urban area have larger radius of horizontal dispersion than rural area. Considering the resolution and time consuming problems of three dimensional grid model, one-dimensional model with one-point real sounding have strong merit for practical dispersion model.

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