• 소음진동
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• 제11권3호
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• pp.437-442
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• 2001

In this study, the fracture phenomena of optical disks are discussed by theoretical and experimental approaches and then some recommendations are presented to prevent the fracture. Linear equations of motion are discretized by using the Galerkin approximation. From the discretized equations, the dynamic responses are computed by the generalized- time integration method. As a fracture criterion for optical disks, the critical crack length is presented. From experimental methods, the fracture procedure is analyzed. The fracture occurs when disks have crack on the inner radius of the disks. Since the crack growth and the fracture result from the stress concentration on the tip of the crack, a measure should be taken to overcome the stress concentration. This problem can be resolved by the structural modification of a disk. This study proposes 3 types of improved optical disks.

• Journal of Mechanical Science and Technology
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• 제16권12호
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• pp.1725-1732
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• 2002

Combined convection and radiation heat transfer in a circular tube with circumferential fins and circular disks is investigated for various operating conditions. Using a finite volume technique for steady laminar flow, the governing equations are solved in order to study the flow and temperature fields. The P- 1 approximation and the weighted sum of gray gases model (WSGGM) are used for solving the radiation transport equation. The results show that the total Nusselt number of combined convection and radiation is higher than that of pure convection. If the temperatures of the combustion gas and the wall in a tube are high, radiation becomes dominant. Therefore, it is necessary to evaluate the effect of radiation on the total heat transfer.

• 천문학회보
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• 제45권1호
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• pp.70.3-70.3
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• 2020

Previous numerical simulations on planet-disk interactions revealed a lot of interesting phenomena including the planetary migration and the formation of many sub-structures inside the disks. However, these simulations were limited to an isothermal or adiabatic equation of state which does not account for various heating and cooling processes in the disks. Recent studies showed that the behavior of the planet-disk interaction can be significantly influenced by the disk thermodynamics. We develop a radiative diffusion module based on the two-temperature flux-limited diffusion approximation accounting for viscous heating and the accretion feedback. In this presentation, we describe our radiative diffusion solver, present some test results, and discuss potential applications of the module to planet-disk interactions,

• 천문학회지
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• 제34권4호
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• pp.251-254
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• 2001

To examine the structure and dynamics of thick accretion disks, we use a two-dimensional viscous hydrodynamic code coupled with radiation transport. The $\alpha$-model and the full viscous stress-tensor description for the kinematic viscosity are used. The radiation transport is treated in the gray, flux-limited diffusion approximation. The finite difference methods used are based on an explicit-implicit method. We apply the numerical code to the Super-Eddington black-hole model for SS 433.@The result for a very small viscosity parameter a reproduces well the characteristic features of SS 433, such as the relativistic jets with $\~$0.26c, the small collimation degree of the jets, the mass-outflow rate of ${\ge}5{\times}10^{-7}M{\bigodot}yr^{-1}$, and the formation of the X-ray iron emission lines.

• 대한수학회보
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• 제49권2호
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• pp.235-247
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• 2012

We study sufficient conditions for function algebras generated by four smooth functions on a small closed bidisk near the origin in $\mathbb{C}$ to coincide with the space of continuous functions on the bidisk. This problem in one dimension has been studied by De Paepe and the second name author.

• 대한수학회보
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• 제39권4호
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• pp.687-704
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• 2002

We show that the class of inner chordarc domains is properly contained in the class of exterior quasiconvex domains. We also show that the class of exterior quasiconvex domains is properly contained in the class of John disks. We give the conditions which make the converses of the above results be true. Next , we show that an exterior quasiconvex domain satisfies certain growth conditions for the exterior Riemann mapping. From the results we show that the domain satisfies the Bernstein inequality and the integrated version of it. Finally, we assume that f is a function which is continuous in the closure of a domain D and analytic in D. We show connections between the smoothness of f and the rate at which it can be approximated by polynomials on an exterior quasiconvex domain and a $Lip_\alpha$-extension domain.

• 한국구조물진단유지관리공학회 논문집
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• 제10권3호
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• pp.185-196
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• 2006

파괴인성은 균열의 개시와 전파에 대한 재료 고유의 상수로서 파괴역학에서 가장 중요한 재료상수 중의 하나이다. 콘크리트의 모드 I 파괴인성 측정에 대하여 RILEM 기술 위원회 89-FMT는 2-파라메타 모델에 근거한 3점 휨 시험법을 제시하였다. 그러나 혼합모드에 대한 시험법은 아직까지 표준으로 제안된 방법이 없는 실정이며, 또한 RILEM에서 제안한 3점 휨 시험법은 실험법이 복잡하다. 따라서 본 연구에서는 굵은골재의 최대치수가 각각 20mm, 40mm이고, 동일한 설계기준강도를 가지는 콘크리트로써 다양한 크기의 브라질리언 디스크를 제작하였다. 그리고 브라질리언 디스크의 모드 I 파괴인성을 RILEM 3점 휨 시험결과와 비교하였다. 비교 결과, 굵은골재의 최대치수에 따른 브라질리언 디스크의 적정 크기(두께, 직경) 및 노치 길이 비를 제시하였다. 또한 모드 I 시험으로부터 결정된 치수의 브라질리언 디스크로 혼합모드 시험을 수행한 결과 디스크 시편은 혼합모드 파괴의 연구 및 시험에 유용함을 알 수 있었다. 모드 I 및 혼합모드 시험에서 브라질리언 디스크의 응력확대계수는 유한요소해석(FEA)으로 구하였으며 FEA의 결과를 검증하기 위하여 5개항 근사법(Five terms approximation)에 의한 결과와 비교하였다.