• Journal of the Society of Naval Architects of Korea
• /
• v.28 no.2
• /
• pp.95-103
• /
• 1991

A series of experiments were performed to see the dependence of the response characteristics of vortex-induced vibration of flexible cylinders on mass rations for marine applications. Experiments were conducted in the $60cm{\times}60cm$ test section of the cavitation tunnel at the Korea Research Institute of Ships and Ocean Engineering using 5 test rods of 60cm length and 6mm diameter with different mass ratios. It was confirmed quantitatively from the experiments that the low mass ratio cylinders have much broader flow velocity range of large amplitude vibrations than high mass ratio ones.

• Journal of Astronomy and Space Sciences
• /
• v.21 no.2
• /
• pp.83-92
• /
• 2004

The absolute dimensions of low mass contact binary, GR Vir and HV Aqr were obtained using WD program from the published spectroscopic and photometric observational data. The evolutionary status of this type of system including GR Vir and HV Aqr has been considered. The primary stars of low mass contact binary system were located on the Terminal Age Main-sequence and secondary stars were located under the Zero Age Main-sequence in H-R diagram.

• Proceedings of the Korean Nuclear Society Conference
• /
• 1998.05a
• /
• pp.577-583
• /
• 1998

직접 접촉에 의한 응축 열전달은 혼합증기의 레이놀즈수, 비응축 가스(공기)의 질량비, 액막의 레이놀즈수, 그리고 액막의 과냉 정도에 따라 영향을 받게 된다. 이러한 변수들의 영향을 고찰하기 위하여 본 연구에서는 수평면으로부터 87˚ 기울어진 수직 사각 덕트에서 직접 접촉 응축 열전달 실험을 수행하였다. 위의 각 실험 변수에 따른 평균 열전달 대수의 변화를 고찰하였으며, 실험결과로부터 혼합증기 레이놀즈수, 비웅축 가스의 질량비, 액막 레이놀즈수, 그리고 제이콥수를 변수로 하여 직접 접촉 응축 열전달에 대한 평균 누셀트수에 대한 실험 상관식을 도출하였다. 혼합증기의 직접 접측 웅축 열전달에 대한 평균 열전달 계수는 비응축 가스의 질량비가 증가할수록 현저히 증가함을 보였으며, 액막의 과법 정도가 증가할수록 평균 열전달 계수는 감소하였다. 그리고 혼합증기의 레이놀즈수가 30,000 이상의 템위에서는 액막 레이놀즈수의 변화에 따라 평균 열전달 계수의 변화가 거의 없었다.

• Journal of Astronomy and Space Sciences
• /
• v.16 no.1
• /
• pp.31-40
• /
• 1999

With a total 761 contact binary systems in Svechnikov & Kuznetsova(1990)'s catalogue, their physical properties by the mass ratio are investigated - for the early CE type with a common radiative envelope and the late CW type with a common convective envelope. It is found that the early CE type shows a higher temperature difference($\mid$$DeltaT$$\mid$) between the primary and secondary components, and also longer period, than the late CW type. The mass ratio of the CW type are distributed in period, than the late CW type. The mass ratio of the CW type are distributed in smaller ranges, from 0.3 to 0.7, than the CE type. Further, the relation between mass ratio and luminosity for the CW type shows a well-defined linear relation, such as ratio and luminosity for the CW type shows a well-defined linear relation, such as $L_2/L_1$ = 0.01 = 0.89q. In the mass ratio-radii relation, it is confirmed that the physical difference of the CE and CW types is a result of the secondary radius. A new mass ratio-radii relation for the CW type is suggested for both the total radius $({gamma}_1/{gamma}_2$ and the radius ratio $({gamma}_2/{gamma}_1$, respectively.

• Transactions of the Korean Society of Mechanical Engineers B
• /
• v.39 no.10
• /
• pp.817-824
• /
• 2015

Experiments were carried out to investigate the flow and mass transfer characteristics of an orifice nozzle. Measurements of primary and suction flow rates, dissolved oxygen concentration, and electric power were obtained. Vertically injected mixed-jet images were captured by a direct visualization technique with a high speed camera unit. The mass ratio, volumetric mass transfer coefficient, and mass transfer performance were calculated using the measured data. As the primary flow pressure increases, the mass ratio decreases slightly, while the volumetric mass transfer coefficient and electric power increase. As the primary flow pressure increases and the mass ratio decreases, the mass transfer rate increases because of the fine bubbles and wider distribution of the bubbles.

• Journal of Astronomy and Space Sciences
• /
• v.26 no.1
• /
• pp.1-8
• /
• 2009

We present new B, V, and R CCD photometric light curves for the low mass ratio contact binary FP Boo. A new photometric solution and absolute physical dimensions of the system were derived by applying the Wilson-Devinney program to our observed light curves and to previously published Rucinski et al.'s radial velocity curves. From the H-R diagram of 24 low mass ratio contact binary system including FP Boo, the evolutionary stage of FP Boo was found to coincide with those of the general low mass ratio contact binary systems. The light curves obtained in this season show a small asymmetry in their shapes.

• Journal of the Earthquake Engineering Society of Korea
• /
• v.15 no.2
• /
• pp.53-60
• /
• 2011

When designing building structures, dynamic serviceability is one of the most important items. Much research is being carried out on machine vibrations that affect inside residents and expensive equipment in the building structure. The vibration effect generally depends on the mass ratio, and an adequate mass ratio is determined by comparison with the serviceability limit according to the criteria. This study investigates the evaluation of vibration serviceability by using ISO 2631 to confirm the propriety of adequate mass ratios and it is verified that the application of a complicated FE model to model the real large shaking table facility with the mathematical model simulated as a SDOF system. The weighted RMS value is then compared with the comfort limit given by ISO 2631. As a result, the analysis of the numerical model is consistent with analysis of the FE model. Moreover, it is found that the adequate mass ratio of the concrete foundation and shake table, considering the self-weight of the real facility, should be less than 0.013. It is also confirm that the sample facility is satisfies the requirement of an adequate mass ratio.

• Transactions of the Korean Society of Mechanical Engineers
• /
• v.10 no.1
• /
• pp.43-49
• /
• 1986

The stability behavior of the cantilever beam carrying several masses and subjected to a follower force at its free end is investigated. The effects of the location and the mass ratio of the concentrated masses on the stability of the system are discussed. An optimal location of the concentrated mass is determined to give maximum critical follower force. Discontinuities of the flutter load are observed for the system with more than two concentrated masses.

• Bulletin of the Korean Space Science Society
• /
• 2003.10a
• /
• pp.21-21
• /
• 2003

접촉쌍성 가운데 질량비(q=m$_2$/m$_1$)가 0.2이하로 매우 작은 접촉쌍성은 그리 흔한 접촉 쌍성이 아니다. 현재까지 이러한 질량비가 작은 접촉쌍성들이 30개 정도가 알려져 있으며 이 가운데도 절대량이 잘 알려진 별들은 14개 정도에 불과하다. 이러한 원인은 이 별들에 대한 분광관측이 이루어져 있지 않기 때문이다. 따라서 이러한 접촉쌍성의 진화 상태를 보다 확실하게 이해하기 위하여 이러한 별들의 절대량을 얻는 것이 요구된다. 이번 연구에서는 Cereda at al.(1988)에 의하여 측광관측(B & V) 결과만 이루어진 후 궤도 요소가 알려져 있지 않은 GR Vir의 관측 자료와 함께 최근 Rucinski & Lu(1999)가 발표된 분광관측 결과를 이용하여 WD 프로그램을 적용하여 이 별의 궤도요소와 함께 절대량을 얻고 이로부터 이 별의 진화 상태를 조사하였다.

• Journal of Korea Water Resources Association
• /
• v.32 no.4
• /
• pp.417-426
• /
• 1999

A series of numerical experiments is performed to compare the characteristics of outflow hydrograph using linear and nonlinear Muskingum-Cunge methods for two cases: (a) sinusoidal inflow hydrographs and (b) rainfall inputs. The nonlinear method shows the steepening of the rising limb, coupled with a corresponding flattening of the receding limb. The linear method conserves mass exactly. In contrast, the nonlinear method is subject to a gain and a loss of mass. The loss of mass and the subsidence of peak outflow increases with a mild slope, a small baseflow $q_b$ and a large peak inflow to baseflow ratio $q_p/q_b$. A shock wave and associated numerical instability results in the increase of mass for a steep slope and a large $q_p/q_b$ ratio. While the linear method depends on the reference flow per unit-width, the nonlinear method depends on a baseflow and the $q_p/q_b$ ratio. It is found that, unlike for the sinusoidal inflow, the outflow for the rainfall inputs conserves mass fairly exactly in the nonlinear method.