• 소음진동
• /
• 제2권1호
• /
• pp.33-39
• /
• 1992

The problem of sound radiation from infinite elastic beams under the action of harmonic point forces is studied. The reaction due to fluid loading on the vibratory response of the beam is taken into account. The beam is assumed to occupy the plane z = 0 and to be axially infinite. The beam material and the elastic foundation re assumed to be lossless and Bernoulli-Euler beam theory including a tension force (T), damping coefficient (C) and stiffness of foundation $(\kappa_s)$ will be employed. The non-dimensional sound power is derived through integration of the surface intensity distribution over the entire beam. The expression for sound power is integrated numerically and the results are examined as a function of wavenumber ratio$(\gamma)$ and stiffness factor$(\Psi)$. Here, our purpose is to explain the response of sound power over a number of non-dimensional parameters describing tension, stiffness, damping and foundation stiffness.

• 소음진동
• /
• 제3권3호
• /
• pp.245-251
• /
• 1993

The problem of sound radiation from infinite elastic beams under the action on harmonic moving line forces is studies. The reaction due to fluid loading on the vibratory response of the beam is taken into account. The beam is assumed to occupy the plane z=0 and to be axially infinite. The beam material and elastic foundation are assumed to be lossless and Bernoulli-Euler beam theory including a tension force (T), damping coefficient (C) and stiffness of foundation $(\kappa_s)$ will be employed. The non-dimensional sound power is derived through integration of the surface intensity distribution over the entire beam. The expression for sound power is integrated numerically and the results examined as a function of Mach number (M), wavenumber ratio$(\gamma{)}$ and stiffness factor $(\Psi{)}$. Here, our purpose is to explain the response of sound power over a number of non-dimensional parameters describing tension, stiffness, damping and foundation stiffness.

• Structural Engineering and Mechanics
• /
• 제54권4호
• /
• pp.623-648
• /
• 2015

A numerical approach is presented for the analysis of the forced vibration of a rigid surface foundation with arbitrary shape. In the analysis, the foundation is discretized into a number of sub squaree-lements. The dynamic response within each sub-element is described by the Green's function, which is obtained by the Fourier-Bessel transform and Precise Integration Method (PIM). Incorporating the displacement boundary condition and force equilibrium of the foundation, it obtains a system of linear algebraic equation in terms of the contact forces within each sub-element. Solving the equation leads to the desired dynamic impedance functions of the foundation. Numerical results are obtained for foundation not only with simple geometrical configurations, such as rectangular and circular foundation, but also the case of irregularly shaped foundation. Several comparisons between the proposed approach and other methods are made. Very good agreement is reached. Also, parametric studies are carried out on the dynamic response of foundation. Addressed in this study are the effects of Poisson's ratio, material damping and contact condition of soil-foundation interface. Several conclusions are drawn the significance of the factors.

• 천문학회보
• /
• 제44권1호
• /
• pp.81.1-81.1
• /
• 2019

Linear sausage oscillations of a cylinder embedded in a plasma with an azimuthal magnetic field, created by a current on the surface of the cylinder, are studied. Such a plasma configuration could be applied to modelling demonstrate that the lowest radial harmonic of the sausage mode is in the trapped regime for all values of the parallel wave number. In the long-wavelength limit, phase and group speeds of this mode are equal to the Alfven speed in the external medium. It makes the oscillation period to be determined by the ratio of the parallel wavelength, e.g., double the length of an oscillating loop, to the external Alfven speed, allowing for its seismological estimations. The application of the results obtained to the interpretation of long-period (longer than 20-30 s) oscillations of emission intensity detected in solar coronal structure, gives reasonable estimations of the external Alfven speed. Cutoff values of the parallel wavenumber for higher radial harmonics are determined analytically. Implications of this finding to the observational signatures of fast magnetoacoustic wave trains guided by the plasma non-uniformity are discussed.

• 한국음향학회지
• /
• 제14권2호
• /
• pp.62-72
• /
• 1995

실험 및 모의실험을 통하여 무차원파수(ka)와 상대어드미턴스(AZ)들이 균일 및 비균일 공극분포를 가지는 다공관 및 다공형 소음기의 음향학적 특성을 대표적으로 표현할 수 있는 물리적 인자임을 확인하였다. 구체적으로는 다공관에 분포한 공극의 임피던스와 여러가지 배열형태를 가지는 다공관의 투과손실을 실험적으로 측정하였으며 이를 통하여 다공관의 투과손실은 ka와 상대어드미턴스 AZ의 함수임을 확인하였다. 다공형 소음기의 투과손실 또한 실험적으로 측정하였으며 Sullivan의 모델을 기초로 한 수치해석방법과의 비교를 통하여 제시된 다공형 소음기 모델의 타당성을 입증하였다.

• 천문학회보
• /
• 제39권2호
• /
• pp.78.1-78.1
• /
• 2014

An ionization front (IF) surrounding an H II region is a sharp interface through which a cold neutral gas makes transition to a warm ionized phase by absorbing UV photons from central massive stars. We investigate the structure and instability of a plane-parallel D-type IF threaded by magnetic fields parallel to the front. We find that magnetic fields increase the maximum propagation speed of the IFs, while reducing the expansion factor, defined as the density ratio of neutral to ionized phases. IFs become unstable to distortional perturbations due to gas expansion across the fronts, exactly analogous to the Darrieus-Landau instability of ablation fronts in terrestrial flames. The growth rate of the IF instability is proportional linearly to the perturbation wavenumber as well as the upstream flow speed. The IF instability is stabilized by gas compressibility and becomes completely quenched when the front is D-critical. The instability is also stabilized by magnetic pressure when the perturbations propagate in the direction perpendicular to the fields. When the perturbations propagate in the direction parallel to the fields, on the other hand, it is magnetic tension that reduces the growth rate, completely suppressing the instability when ${\beta}$ < 1.5, with ${\beta}$ denoting the square of the ratio of the sound speed to the Alfven speed in the pre-IF region. When the front experiences an acceleration, the IF instability cooperates with the Rayleigh-Taylor instability to make the front more unstable. We discuss potential effects of IF instability on the evolution and dynamics of IFs in the interstellar medium.

• E2M - 전기 전자와 첨단 소재
• /
• 제10권7호
• /
• pp.706-712
• /
• 1997

AlN(Aluminium Nitride) thin films were prepared using by RF sputtering method on the Si(100) and Si(111) substrates as the parameters of the substrate temperature, RF power, sputtering duration and the $N_2$/Ar ratio and investigated by X-ray diffraction, IR spectrometry, n&k analyzer. For the Si(100) substrate, the AlN thin films of (101) orientation were obtained under the conditions of room temperature and the nitrogen of 60 vol.%. For the Si(111) substrate, the (002) AlN thin films were obtained under the nitrogen of 100 vol.%. In case of the thin film prepared in the condition of above 60 vol.% of the nitrogen, the average value of the surface roughness of the film was 151$\AA$. From the changes of the half widths of E$_1$[TO] phonon bands at the wavenumber of 680$cm^{-1}$ /, it were compared of the crystallinities of the films which were grown under the different conditions. The thicknesses of AlN films were decreased dramatically in the region of the nitrogen of 40~60 vol.%. Its due to the nitridation of the Al target surface and getting low of the sputtering yield by the $N_2$/Ar ratio being increased.

• 지구물리와물리탐사
• /
• 제12권1호
• /
• pp.132-142
• /
• 2009

Tamar 열곡은 Tatmania의 Launceston 시를 관통하고 있고, Bass 해협의 지진 활동은 이 도시의 건물들에 피해를 입혔다. 두께가 0 m에서 250 m의 범위로 급격하게 변화하는 연약 퇴적물로 채워진 Tamar 열곡은 Launceston 시 내부와 열곡 위의 지표면 진동을 증폭시키면서 2차원적인 공진 양상을 유도하는 것으로 생각되고 있다. 공간적 평균 일관성 (SPAC), 주파수-파수 (FK), 수평과 수직 스펙트럼 비율을 이용하는 상시 진동 탐사법이 Tamar 열곡에 미치는 영향을 확인하기 위하여 여러 기법을 혼합하여 사용하였다. 일곱 개의 지점에서 수동 탄성파 탐사가 수행되었고, 횡파 속도의 심도 단면을 추정하기 위하여 SPAC을 분석하였으며, 대략 125 m 심도의 퇴적층 속도 단면의 정밀도를 향상시키기 위하여 HVSR을 결합하였다. 그 결과, 퇴적층의 두께가 Launceston 시에서 전체적으로 변화가 심하게 나타남을 확인하였다. 최상부층은 매우 연약한 제 4기의 충적층으로 구성되어 있으며, 횡파 속도는 50 m/s에서 125 m/s의 범위를 나타낸다. Tamar 열곡의 0 m에서 250 m 심도를 채우고 있는 제 3기의 퇴적층의 횡파 속도는 400 m/s에서 750 m/s로 변화한다. GUN과 KPK 측점해서 SPAC을 이용하여 획득한 결과는 FK 분석으로 해석된 분산 곡선과 잘 일치하였다. FK 해석은 SPAC 보다 좁은 주파수 대역에 한정되어서, 더 낮은 주파수 대역에서 횡파 속도가 높게 추정된 것으로 보인다. 층서 모델로 가정하여 측정된 HVSR은 SPAC에 의한 결과와 비교하였고, 횡파 느리기 단면에 추가적인 제한조건을 제공하였다. SPAC과 HVSR 분석을 결합한 결과에서는 GUN 측점의 지질구조가 층서 구조로 가정할 수 있음을 확인하였고, KPK 측점에서는 Tamar 열곡을 가로지르는 2차원적 공진 양상이 존재함을 확인하였다

• 소음진동
• /
• 제5권2호
• /
• pp.169-181
• /
• 1995

A theoretical model has been studied to describe the sound radiation analysis for structural vibration noise control of tire under the action of random moving line forces. When a tire is analyzed, it has been modeled as a curved beam with distributed springs and dash-pots which represent the radial, tangential stiffness and damping of tire, respectively. The reaction due to fluid loading on the vibratory response of the curved beam is taken into account. The curved beam is assumed to occupy the plane y = 0 and to be axially infinite. The material of curved beam and elastic foundation are assumed to be lossless, and governed by the law of Bernoulli-Euler beam theory. The expression for sound power is integrated numerically and its results examined as a function of Mach number(M), wavenumber ratio(.gamma.) and stiffness factor(.PSI.). The experimental investigation for structural vibration noise of tire under the action of random moving line forces has been made. Based on the STSF(Spatial Transformation of Sound Field) techniques, the sound power and sound radiation are measured. The experimental results show that operating condition, material properties and design factors of the tire have a great effect on the sound power and sound radiation characteristics.

• Nuclear Engineering and Technology
• /
• 제45권7호
• /
• pp.895-910
• /
• 2013

The reflood test data from the rod bundle heat transfer (RBHT) test facility showed that the grids in the upper portion of the rod bundle could become wet well before the arrival of the quench front and that the sizes of liquid droplets downstream of a wet grid could not be predicted by the droplet breakup models for a dry grid. To investigate the water droplet generation from a wet grid spacer, a viscous linear temporal instability model of the water sheet issuing from the trailing edge of the grid with the surrounding steam up-flow is developed in this study. The Orr-Sommerfeld equations along with appropriate boundary conditions for the flow are solved using Chebyshev series expansions and the Tau-Galerkin projection method. The effects of several physical parameters on the water sheet oscillation are studied by determining the variation of the temporal growth rate with the wavenumber. It is found that a larger relative steam velocity to water velocity has a tendency to destabilize the water sheet with increased dynamic pressure. On the other hand, a larger ratio of steam boundary layer to the half water sheet thickness has a stabilizing effect on the water sheet oscillation. Droplet diameters downstream of the spacer grid predicted by the present model are found to compare reasonably well with the data obtained at the RBHT test facility as well as with other data recently reported in the literature.