• 천문학논총
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• 제7권1호
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• pp.39-50
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• 1992

A velocity inhomogeneity, which is the regional preponderence of either radial or tangential orbits, is searched with the new technique proposed by Kim (1992) for Coma, Hydra I, and Abell 2256 cluster of galaxies. Conspicuous inhomogeneities are found in the Coma and A2256 which X-ray isophotes are indicative for their underlying potentials being ellipitcal in shape, Even in their central regions, zones that are dominated by radial orbits are clearly distinguishable from that of the tangential orbits, and defining the cluster 'equator' as the direction of maximum elongation of the X-ray isophotes, radial orbits dominate along this direction whereas tangential orbits dominate the 'polar' zones. Merger events that are evidenced in X-ray observations occur in the equatorial zones of Coma and A2256, suggesting preponderence of radial orbits in the zones, which is in good agreement with their velocity structures. On the other hand, the inhomogeneity in Hydra I turns out to be insignificant in the central regions and this is just what is expected from a cluster whose X-ray isophotes is nearly circular. The velocity distribution in regions further out, however, shows significant inhomogeneity and this seems to support the previous results that this cluster is likely to have substructures and velocity anisotropy.

• Ocean and Polar Research
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• 제44권4호
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• pp.287-296
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• 2022

High-frequency (HF) radar measures sea surface currents from the radio waves transmitted and received by antenna on land. Since the data quality of HF radar measurements sensitively depend on the radio wave environment around antenna, Antenna Pattern Measurements (APM) plays an important role in evaluating the accuracy of measured surface currents. In this study, APM was performed by selecting the times when the background noise level around antenna was high and low, and radial data were generated by applying the ideal pattern and measured pattern. The measured antenna pattern for each case was verified with the current velocity data collected by drifters. The radial velocity to which the ideal pattern was applied was not affected by the background noise level around antenna. However, the radial velocity obtained with APM in the period of high background noise was significantly lower in quality than the radial velocity in a low noise environment. It is recomended that APM be carried out in consideration of the radio wave environment around antenna, and that the applied result be compared and verified with the current velocity measurements by drifters. If it is difficult to re-measure APM, we suggest using radial velocity in generating total vector with the ideal pattern through comparative verification, rather than poorly measured patterns, for better data quality.

• 한국전자파학회논문지
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• 제27권6호
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• pp.521-530
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• 2016

기상레이다는 전자기파를 대기 중에 방사하여 목표물에 부딪혀서 되돌아오는 후방산란 신호를 수신하는 기상장비이다. 기상청의 기상레이다는 도플러 관측 기능을 가지고 있기 때문에 목표물의 시선속도를 산출할 수 있다. 그러나 기상레이다의 넓은 관측 반경을 확보하려면 관측 속도 범위가 작아져 이를 넘어서는 시선속도는 접힘 현상이 발생한다. 따라서 최대 관측 반경을 유지한 채 관측 속도 범위를 넓히기 위해서는 high PRF와 low PRF 두 개의 서로 다른 PRF로 신호를 송 수신하는 dual PRF(Pulse Repetition Frequency) 모드 기능을 이용해야 한다. Dual PRF 모드를 이용하면 high와 low PRF로 관측된 두 최대 속도의 최소공배수만큼 관측 속도 범위를 넓힐 수 있다. 이를 위해 본 연구에서는 high PRF와 low PRF로 관측된 시선속도의 차이값과 이에 대한 오차를 고려한 분류 기준을 만들고, 분류된 영역별로 보정 인자를 산출하여 시선속도 펼침을 수행하는 시선속도 접힘 풀기 알고리즘을 개발하였다. 이를 용인테스트베드레이다에 적용한 결과, 기존에 산출되는 시선속도보다 개선된 성능을 보였다.

• 한국음향학회지
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• 제42권1호
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• pp.25-31
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• 2023

능동소나를 이용하여 수중물체의 속도를 추정하려면 Continuous Wave(CW) 펄스를 이용하는 것이 일반적이나, 수중물체의 속도가 느리고 근거리의 해양에서는 잔향음의 영향으로 수중물체의 속도 추정이 용이하지 않다. 2017년도에 Wang 연구진은 이를 극복하고자 수중물체의 속도에 의한 도플러 변이에 둔감한 광대역 신호인 Hyperbolic Frequency Modulation(HFM) 펄스 두 개를 상반된 스윕방향으로 이용하였다. 두 펄스 간 송신 시간간격과 탐지시간 차이의 변화를 통하여 수중물체 속도 추정이 가능하다는 것을 시뮬레이션으로 제시하였다. 하지만 동일한 대역을 이용하므로 상호상관성에 의해서 수중물체 탐지 성능이 영향을 받을 수 밖에 없다. 상호상관성에 의한 수중물체 탐지 성능저하를 방지하기 위하여 대역이 분리된 상반된 스윕방향의 두 HFM 펄스 이용을 제안한다. 본 논문에서는 상반된 스윕방향의 두 대역 HFM을 이용하여 수중물체의 시선속도 추정에 관한 이론을 도출하였고, 펄스길이와 대역폭이 1 s와 400 Hz인 HFM 펄스로 시뮬레이션을 수행하였다. 제안한 방법을 이용하여 수중물체의 시선속도를 추정하면 약 6 %의 오차로 표적 속도 추정이 가능하다는 것을 시뮬레이션을 통하여 확인하였다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 1992년도 한국우주과학회보 제1권1호
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• pp.15-15
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• 1992

AQ Cassiopeiae (BD+61`0242, uv=10, Sp=B3+Bg) is a totally eclipsing binary system with the obital period of about 12 days. 71 was observed for 15 nights in 1985 with the1.8-m telescope at the DAO, employing a Reticon and a three-stage image tube attached to the spectrograph. And also, photometric observations of AQ Cas had been made inUBv for six years from 1982 to 1988 at Yonsei University Observatory(YUO). This work includes UBV observations obtained at YUO as a part of The Ten-Year Observing Program(1982-1992). Double lined radial, velocity curves and Ufv light curves of AQC as are constructed. The light curves and radial velocity curves show a strong evidence of circumstellar matter or mass stream. It is clear at the phases of just outside externaleclipse contacts, particularly at phase 0.8-0.9, shown in Figures 1 and 2. A solution by combining the radial velocity and photometric curves of the binary was obtained with the Wilson-Devinney Code. We found that the system is semi-detached with the coolcomponent filling its Roche lobe. The absolute dimensions of AQ Cas are calculated. The result shows that this system consists of two massive and subgiant stars.

• 대한기계학회논문집B
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• 제25권12호
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• pp.1813-1820
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• 2001

The purpose of this study was to investigate the significant characteristics in atomization process of industrial etching spray fur the design or Precise pressure-swirl nozzles. The experiment was carried out with different viscosities and densities of the liquid. The macro characteristics of liquid spray, such as the spray angle and breakup process were captured by PMAS and the micro characteristics of liquid spray. such as droplet size and velocity measurements were obtained by PDA. The droplet axial and radial velocity and SMD were measured along axial and radial direction. The RMS of two velocities was measured along radial direction. It was found that the fluid with higher kinematic viscosity resulted in the larger SMD and the lower mean droplet velocity. And we could divide breakup processes into three regions that is atomization, non-dilution and dilution one in spray of pressure-swirl nozzle. The radial as well as axial velocity of droplet played an important role in the atomization process of higher kinematic viscosity fluid.

• 대한기계학회논문집A
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• 제20권1호
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• pp.1-13
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• 1996

The measurement of radial directional natural frequency ina passenger car tire rotating under the load is studied. In order to obtain theoretical matural frequency and mode shape, the ploane vibration of a tire is modeled to that of circular beam. By esing the Tieking method based on Hamiltons's principle, theoretical results are determined by considering tension horce due to tire inflation pressure, retational velocity and tangential, radial stiffness. Radial directional modal parameters varying with the inflation pressure, load, rotational velocity are experimentally determined by using frequency response function method. The results show that experimental conditions canbe considered as the parameters which shift the natural frequency.

• 대한기계학회논문집B
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• 제24권10호
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• pp.1300-1308
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• 2000

The objectives of this study was to investigate the spray characteristics of single spray and twin spray in the overlap region such as mean axial velocity, mean radial velocity, mean droplet size and probability density function of droplet size. A phase doppler anemometer was used as the measurement system for droplet size and velocity. In case of single spray, injection pressure was varied from 0.2MPa to 0.7MPa. Mean axial velocity, mean radial velocity and droplet size were decreased as the distance below nozzle tip was increased. In case of twin spray, the spray characteristics were measured by varying the distance between two nozzles from 127mm to 155mm. In the overlap region, the boundary of the overlap region was determined by obtaining the distribution of mean axial and radial velocity. Droplet size was increased as the distance from nozzle tip was increased. It was found that the distribution of droplet size for twin spray in the overlap region was different to single spray.

• 동력기계공학회지
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• 제4권3호
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• pp.25-33
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• 2000

This study represents three-dimensional turbulent flow characteristics around an axial fan measured at the operating point ${\varphi}=0.32$, which is equivalent to the maximum flowrate region, by using three-dimensional fiber-optic type LDA system. This LDA system is composed of a 5 W Argon-ion laser, two optics in back-scatter mode, three BSA's, a PC, and a three-dimensional automatic traversing system. A kind of paraffin fog is used for laser particles in this study. Mean velocity profiles around an axial fan along the downstream radial distance show that the streamwise and the tangential components exist as a predominant velocity and have the maximum value at the radial distance ratio 0.8, while the radial component has a small scale distribution and its flow direction is inward except a part of blade tip. The turbulent intensity profiles show that the radial component exists the most greatly. And also the turbulent kinetic energy shows about 60% as a maximum value at the radial distance ratio 0.9. Moreover, the Reynolds shear stresses do not exist at upstream flow, but the streamwise and the radial components of them show about 20% as a maximum value at the radial distance ratio 0.9 at downstream flow.

• 지구물리와물리탐사
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• 제20권1호
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• pp.25-32
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• 2017

이 연구는 동아시아 지역의 지각과 상부맨틀의 3차원 SH파 속도구조 및 지진파 속도 방사 이방성을 알아보기 위하여 수행되었다. SH파 속도모델은 한국과 일본, 중국에 설치되어 있는 광대역 지진관측소에 기록된 지진자료로부터 러브파 군속도 분산 자료를 획득한 후 이를 역산하여 구하였다. 군속도 분산곡선은 총 3,369개의 파선경로에 대하여 다중필터기법을 사용하여, 접선 성분에 기록된 주기 3 ~ 150 초 범위의 러브파 군속도를 획득하였다. 획득한 군속도자료를 역산하여 깊이 100 km까지의 SH파 속도구조를 계산하였다. 10 ~ 40 km 깊이에서 동해지역은 일본지역보다 SH파 속도가 빠르게 나타난다. 고속도 이상이 나타나는 깊이로 판단할 때, 모호면의 깊이는 동해의 경우 10 ~ 20 km 사이, 한반도의 경우에는 35 km 부근에서 모호면이 존재한다고 생각된다. 50 km 깊이에서 동해지역은 강한 저속도 이상이 관측이 되고, 저속도 이상이 나타나는 깊이로 판단할 때, 50 km 부근에 암석권과 연약권의 경계가 존재한다고 생각된다. 연구지역 아래 50 ~ 100 km 깊이에서는 저속도 이상이 광범위하게 관측된다. 지진파 속도 이방성은 35 km 깊이 까지는 평균적으로 SH파의 속도가 빠른 양의 이방성을 보이며, 그보다 더 깊은 깊이에서는 평균적으로 SV파의 속도가 빠른 음의 이방성이 관측된다.