• 한국정밀공학회지
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• 제22권2호
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• pp.60-69
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• 2005

In electrostatic suspension system of thin plates like a silicon wafer or an aluminum disk for hard disk applications, the lateral restoring force exerted on a suspended object plays an important role since the lateral motion of the suspended object, owing to the inherently stable restoring forces, can be passively stabilized without any active control of it. This paper reports about the measurement apparatus of the lateral restoring force originating from a relative translation of the suspended object with respect to the electrodes-for-suspension. An approximate calculation of the lateral force in disk-shaped objects, the structure of the measurement apparatus, a measurement method, stabilization condition and the guideline in designing the measurement apparatus are described. Experimental results obtained by using a 3.5-inch aluminum disk as a suspended object are presented as well in order to assess the magnitude of lateral force and stiffness, and also verify the usefulness of the measurement apparatus.

• 정보저장시스템학회논문집
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• 제1권2호
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• pp.169-174
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• 2005

Current information storage devices read/write data on the rotating disk. The axial vibration of a rotating disk should be suppressed for the successful operation of the device. Information storage devices widely used in these days adopt relatively thick disk which is stiff enough to suppress axial vibration under allowable limit. However, the thickness of the disk is going to be thinner and thinner as the small form factor of the devices is getting preferred by the consumer. In this study, a stabilizer system, which is composed with 8 air bearings, is proposed for suppressing the axial vibration of a $95{\mu}m$ thick PC disk in a non-contacting manner. The performance of the stabilizer system is simulated by numerical computation and then confirmed its results through a series of experiment. A thin and flexible disk has various vibration modes when it rotates in high speed. The stabilizer system generates positive as well as negative pressure due to the rotation of flexible disk so that the force due to the pressure distribution pushes and pulls rotating disk in a non-contacting manner. The balance between positive and negative pressure forces can be obtained by adjusting the area and the slope of the air bearing surface. The axial vibration of the flexible disk of 120mm diameter is suppressed successfully from over $1000{\mu}m$ to $30{\mu}m$ peak-to-peak value at the rotational speed of 5,000rpm.

• 천문학회보
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• 제43권1호
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• pp.36.2-36.2
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• 2018

Radiative transfer models were developed to understand the optical polarizations in edge-on galaxies, which are observed to occur even outside the geometrically thin dust disk, with a scale height of ~0.2 kpc. In order to reproduce the vertically extended polarization structure, we find it is essential to include a geometrically thick dust layer in the radiative transfer model, in addition to the commonly-known thin dust layer. The models include polarizations due to both dust scattering and dichroic extinction which is responsible for the observed interstellar polarization in the Milky Way. It is found that the magnetic fields in edge-on galaxies are in general vertical (or poloidal) except the central part, where the magnetic fields are mainly toroidal. We also find that the polarization level is enhanced if the clumpiness of the interstellar medium, and the dichroic extinction by vertical magnetic fields in the outer regions of the dust lane are included in the radiative transfer model. The predicted degree of polarization outside the dust lane was found to be consistent with that (ranging from 1% to 4%) observed in NGC 891.

• Bulletin of the Korean Chemical Society
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• 제23권3호
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• pp.399-403
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• 2002

The complex of iron(II) tris(3-Br-phen) (3-Br-phen; 3-bromo-1,10-phenanthroline) was prepared as a precursor of electropolymerization and the crystal structure of [Fe(3-Br-phen)3]($PF_6$)2${\cdot}$CH3CN with a distorted octahedral geometry has been investigated. The reductive electropolymerization of $>[Fe(3-Br-phen)3]^{2+}$ complex onto the surface of a glassy carbon electrode and indium tin oxide (ITO) optically transparent electrode were performed in acetonitrile at room temperature. Thin film of poly-$>[Fe(3-Br-phen)3]^{2+}$ formed was adherent, electroactive and stably deposited on a glassy carbon disk electrode. The thin metallopolymeric film formed was also confirmed by absorption spectroscopy.

• 대한조선학회지
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• 제12권2호
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• pp.13-34
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• 1975

Analytical solutions for the transient temperature distribution and quasi-static thermal stresses which arise in a thin circular disk of finite radius subjected to an instantaneous point source acting in its interior have been obtained. And the solutions have been extended to the case of a moving heat source with the aid of the Duhamel's superposition integral. The solutions given are in the form of double infinite serieses, and their numerical results have been compared with the experimental temperature histories. It can be found out that the theoretical histories of thermal stresses show a good agreement with the experimental results and the theoretical histories of thermal stresses show a good qualitative agreement with a physical phenomena. The solutions can be applied to the problems such as a flame hardening of the cylindrical machine elements and a circular patch welding or a circular cutting of the structural member.

• 한국정밀공학회:학술대회논문집
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• 한국정밀공학회 2004년도 춘계학술대회 논문요약집
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• pp.140-140
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• 2004

마이크로 기술을 대변하는 Micro-Electro-Mechanical-Systems (MEMS)와 반도체, 각종 micro-sensor 및 actuator 등은 실리콘 위에 박막 코팅한 재료를 주로 사용하고 있다. 따라서 1 Um 이하의 박막코팅에 의해 원하는 성능을 얻으려는 시도가 널리 진행되고 있다 Hard Disk Drive (HDD)의 Head-Disk Interface (HDI)와 MEMS 접촉면에서는 발생하는 마찰 및 마멸에 대한 문제 등은 중요한 고려대상이다. 특히 코팅 층의 표면 파손 현상은 코팅 층의 파손 특성과 코팅 층과 기판 사이의 결합상태가 큰 영향을 미친다.(중략)

• 천문학회지
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• 제34권4호
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• pp.265-269
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• 2001

We present preliminary numerical simulations of tilted-disk accretion around a rotating black hole. Our goal is to explore whether hydrodynamic instabilities near the Bardeen-Petterson radius could be responsible for generating moderate-frequency quasi-periodic oscillations in X-ray binaries. We review the relevant general relativistic hydrodynamic equations, and discuss preliminary results on the structure and dynamics of a thin, Keplerian disk.

• 한국자기학회:학술대회 개요집
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• 한국자기학회 1999년도 춘계연구발표회 논문개요집
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• pp.128-129
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• 1999

• 한국전자파학회논문지
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• 제18권1호
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• pp.62-75
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• 2007

본 논문은 단위 방사 소자의 이득을 증가시키기 위한 성형 빔 안테나에 관한 것이다. 제안하는 안테나 구조는 크게 여기 소자와 다층 원형 도체 배열 구조로 구성된다. 광대역에 걸쳐 전자파 전력이 다층 원형 도체 배열로 방사하기 위한 여기 소자로 스택 마이크로스트립 패치 소자가 사용되었으며, 고이득 빔 성형을 위한 지향 소자의 역할을 담당하는 다층 원형 도체 배열 소자들은 여기 소자 위에 주기적으로 유한하게 적층되었다. 제안하는 안테나가 고이득 특성을 얻기 위해서는 여기 소자와 다층 원형 도체 배열 소자들 간의 효율적인 전력 결합이 이루어져야 하며, 이를 위해 주어진 설계 규격에 따라 여기 소자 및 다층 원형 도체 배열 소자들의 설계 변수들은 함께 최적화되어야 한다. 본 연구에서는 고이득 성형 빔 안테나는 $9.6{\sim}10.4\;GHz$ 주파수 대역 및 선형 편파 조건하에서 최적화 설계되었으며, 또한 안테나의 다층 원형 도체 배열 소자들을 구현하는 2가지 방법 즉, 얇은 유전체 필름을 이용하는 방법과 유전체 폼을 이용하는 방법들도 제안되었다. 특히, 유전체 필름을 이용하는 안테나에 대해서는 컴퓨터 시뮬레이션 과정을 통해, 원형 도체 배열 소자들의 적층 수에 따른 안테나의 전기적인 성능 변화들을 보여주었다. 유전체 필름(Type 1)과 유전체 폼(Type 2)을 이용한 2종류의 안테나 시제품들을 제작하였으며, 얇은 유전체 필름을 이용한 안테나 시제품에 대해선 시뮬레이션 된 전기적 성능 결과와 비교를 위해 원형 도체 배열 적층 수에 따른 안테나의 전기적인 성능 변화들을 실험하였다. 측정된 이득 성능은 시뮬레이션 이득 성능과 거의 유사한 결과를 보여주었으며, 원형 도체 적층 수에 따라 안테나 이득 변화는 주기성을 보였다. 10 GHz 중심 주파수에서 측정된 Type 1 안테나의 전기적 성능은 원형 도체 배열을 10개 적층(disk10)하였을 때, 15.65 dBi의 최대 안테나 이득과 11.4 dB 이상의 입력 반사 손실 성능을 보여 주었으며, 다층 원형 도체 배열 구조에 의해 약 5 dB의 이득 향상 효과를 얻을 수 있었다. 또한, 원형 도체를 12개 적층하였을 때, 외곽 유전체 링 효과에 의해 Type 1 안테나는 Type 2 안테나보다 상대적으로 약 1.35 dB 만큼 이득이 더 높았으며, 각 안테나의 3 dB 빔 폭은 각각 약 $28^{\circ}$와 $36^{\circ}$로 측정되었다.

• 천문학회보
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• 제36권2호
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• pp.111.2-111.2
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• 2011

While many astrophysical disks are vertically stratified and obey a polytropic equation of state, most studies on gravitational instability (GI) of flattened systems consider isothermal, razor-thin disks by taking vertical averages of disk properties. We investigate local GI of rotating pressure-confined polytropic disks with resolved vertical stratification by performing linear stability analysis. We find that the GI of vertically-stratified disks is in general a combination of conventional razor-thin Jeans modes and incompressible modes. The incompressible modes that dominate in the limit of the maximal disk compression require surface distortion and are an unstable version of terrestrial water waves. Disks with a steeper equation of state are found to be more Jeans unstable because they tend to have a smaller vertical scale height as well as a steeper temperature gradient corresponding to lower pressure support. GI depends more sensitively on the vertical temperature than density distribution. The density-weighted, harmonic mean, rather than the simple mean, of the adiabatic sound speed well describes the dispersion relation of horizontal modes, and thus is appropriate in the expression for Toomre Q stability parameter of razor-thin disks. We generalize Q into vertically-stratified disks, and discuss astrophysical application of our work.