• 한국해안해양공학회지
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• 제2권4호
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• pp.190-199
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• 1990

3층 구조를 갖는 대륙붕 외해역에서의 취역류 예측을 위한 Galerkin 해를 Eigenfunction 전개를 통해 유도하였다. 수심변화를 결정짖는 연식난류확산 계수가 층간에 불연속적으로 변화토록 정의되므로 내적분 정의시 층별적분이 등장한다. Eigenfunction 및 Eigenvalue 산출을 위해 B-spline 함수전개가 이용되는데 정확한 계산을 위해서는 난류활동이 극도로 저하되는 Pycnocline 내에 많은 Knot들을 배정함이 필요한 것으로 나타났다. 비록 Eigenfunction이 층간에 급격한 변화를 가지나 여전히 해수표면부터 해저편간의 전 구간에 걸쳐 정의되는 연속함수이므로 Gibbs 효과에 따른 해의 진동현상이 표층하, 특히 Pycnocline 내에서 출현하였다.

• 수산해양기술연구
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• 제52권4호
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• pp.347-355
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• 2016

In this study, a new designed propeller was applied on 24 ton class squid jigging vessel to reduce of fuel consumption. The selected squid jigging boat was under construction at the shipyard to determine the resistance of the hull through the model experiment. The propeller design was carried out by using the experimental data and ITTC procedures. Sea trials were performed by measuring the speed and the horsepower required by the condition of five power levels of engine load, namely 70%, 80%, 90%, MCR and maximum engine power. The speed and delivered horse power were compared between the conventional propeller and the new design propeller. Delivered horse power by installing the new propeller takes 90% engine load at start-up conducted by decreased 9.06%. The measuring speed is increased up to the 0.6 knots in the low-speed range to high range. This study showed that only the design and installation of a new propeller can improve the propulsion efficiency of the boats; furthermore, reduce fuel costs can be achieved at the same time by improving the increased cruising speed.

• 수산해양기술연구
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• 제13권2호
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• pp.21-26
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• 1977

대서양(大西洋) Africa 연안어장(沿岸漁場)에서 조업중(操業中)인 태창수산(太倉水産) 소속(所屬) Stern trawl 선(船) No. 85 PARTO(499S)에서 사용(使用)하고 있는 PT-4 형(型) 어구(漁具)의 조정한계(調整限界) 및 적정(適正)한 예망속도(曳網速度)와 주기(主機)의 운전상태(運轉狀態)를 판단(判斷)하기 위(爲)하여 warp에 작용(作用)하는 장력(張力)을 측정(測定)한 결과(結果)를 요약(要約)하면 다음과 같다. 1. 어구조정(漁具調整)의 한계(限界)는 warp에 작용(作用)하는 장력(張力)의 크기가 약(約) 7,500kg, 강약(强弱)의 범위(範圍)가 약(約) 1,000kg을 초과(超過)하지 않는 것이 효과적으로 판단(判斷)했다. 2. 예망속도(曳網速度)는 주기(主機)의 효과적인 운전상태(運轉狀態)와 어획성능(漁獲性能)을 고려(考慮)하여 $3.6{\sim}4.0$ knot로 판단(判斷)했다. 3. 주기(主機)의 운전상태(運轉狀態)는 유량소모(油量消耗)가 급증(急增)하는 r. p. m. 290, propeller pitch 각도(角度) 13.8를 초과(超過)하지 아니하고 $13.5^{\circ}{\sim}13.8^{\circ}$를 사용(使用)하는 것이 효과적으로 판단(判斷)했다.

• 천문학회지
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• 제48권2호
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• pp.113-123
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• 2015

We present observational results from optical long-slit spectroscopy of parsec-scale jets of DG Tau. From HH 158 and HH 702, the optical emission lines of Hα, [O i] λλ6300, 6363, [N ii] λλ6548, 6584, and [S ii] λλ6716, 6731 are obtained. The kinematics and physical properties (i.e., electron density, electron temperature, ionization fraction, and mass-loss rate) are investigated along the blueshifted jet up to 650′′ distance from the source. For HH 158, the radial velocity ranges from −50 to −250 km s⁻¹. The proper motion of the knots is 0.′′196 − 0.′′272 yr⁻¹. The electron density is ∼10⁴ cm⁻³ close to the star, and decreases to ∼10² cm⁻³ at 14′′ away from the star. Ionization fraction indicates that the gas is almost neutral in the vicinity of the source. It increases up to over 0.4 along the distance. HH 702 is located at 650′′ from the source. It shows ∼ −80 km s⁻¹ in the radial velocity. Its line ratios are similar to those at knot C of HH 158. The mass-loss rate is estimated to be about ∼ 10⁻⁷ M_⊙ yr⁻¹, which is similar to values obtained from previous studies.

• 천문학회보
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• 제36권2호
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• pp.104.1-104.1
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• 2011

We present a catalog of infrared supernova remnants (SNRs) in the Large Magellanic Cloud (LMC). We have searched the Spitzer archival data for infrared counterparts to all 45 known SNRs in the LMC, and identified 21 which is 47% of the known SNRs. Seven of them are newly detected: SNR 0450-70.9, SNR in N4, N103B, DEM L241, DEM L249, DEM L316A, and DEM L316B. All newly discovered SNRs show emission at several IRAC 3.4, 4.5, 5.8, and 8.0 micron bands and/or MIPS 24 and 70 micron bands. Most SNRs show shell structures. We derive infrared fluxes of these newly detected SNRs. The catalog contains general information of each SNR such as location, age, and SN type together with AKARI and/or Spitzer fluxes. For the entire SNR sample, we examine their infrared colors and the possible correlation of the infrared fluxes with the fluxes at other wavelengths. For the newly detected SNRs except the SNR in N4, we also performed follow-up imaging observations of [Fe II] 1.644 micron line using IRIS2 mounted on the Anglo Australian Telescope. Three out of six SNRs show [Fe II] emission corresponding to their infrared shells. [Fe II] knots are also detected in N103B which show good spatial correlation to infrared emission seen at Spitzer images as well as knotty $H{\alpha}$ emission. We investigate the characteristics and origin of the infrared emission in individual SNRs, and discuss the environmental and evolutionary effects.

• 한국공간구조학회논문집
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• 제12권2호
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• pp.45-53
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• 2012

본 논문은 비정형의 정확한 형상 설계와 구조해석을 위해 넙스 기저함수를 기반으로 한 변수들로 생성된 평연의 등기하 해석법과 해석 결과에 대한 후처리 방법을 제시한다. 제어점, 매듭값, 차수들로 구성되는 변수들을 인터페이스 기법을 통해 변화시킴으로써 다양한 기하 형상을 구축할 수 있다. 등기하 해석에 사용되는 기저함수는 기하형상 구축에 사용되는 함수와 동일하여 형상의 정확한 설계와 해석이 가능하다. 등기하 해석을 위한 요소망 생성을 위해 h-p-k refinement 과정을 수행함으로써 기존 형상의 변형없이 요소망을 생성하여 구조해석을 수행하였다. 해석에 의한 결과값인 제어점의 변위에 대한 시각화를 위해 IGES 포맷과 넙스기반 3D 설계 프로그램 라이노와의 인터페이스 과정을 수행하여 최종 변형 형상 표현을 위한 후처리 방법을 제시한다.

• 복식
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• 제61권8호
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• pp.114-126
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• 2011

Many varieties in folk costumes have inspired fashion designs for a long time. Each country, with a unique style of its own reflects their own traditions, beliefs, customs and morals into their traditional costumes. The traditional methods of creating different ways of drapery methods by using only a rectangular piece of cloth have been passed down from generation to generation and it is still used today. This way of styling has been developed mainly in the Middle East, Asia and Africa and the modifiable ways of creating drapery wearing methods are as follows. The first modifiable styling method is changing the purpose of wearing costumes according to the needs and the wants of the person who wears it. The second method is exposing the knots on the surface of the garments and by doing this, there was no visible difference on the aesthetic formation and it did not alternate for a long time. This means that simple knot shapes have been used to tie edges of rectangular fabrics. The third method is a wrapping type of modifiable styling method, which has been used most commonly in folk costumes because there are lots of ways to wrap a rectangular cloth around the body. The fourth way is the fixed type of modifiable styling method and this method can only be noticed only in the Moroccan Izar using fibulas and belts to alter the shape of the Izar. The fifth method is the composite type of modifiable styling method. This method starts by cutting out cylindrical shapes of fabrics and then wraps or twists it to fit the body. The most significant character of modifiable styling methods in folk costumes is to use rectangular cloths, which varies only in ratio of length, width and sizes. Therefore, this study suggests that rectangular cloths can create enormous amounts of fashion styling which can be easily adapted and created in everyday fashion life.

• Journal of the Korean Wood Science and Technology
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• 제32권6호
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• pp.57-66
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• 2004

To study the efficient usage of small diameter logs and woods containing defects such as knots, slope of the grain and decay, six types of finger-jointed woods with various finger profiles were made of poplar, pine and oak with different density. We investigated the effect of finger profile on static bending strength performances of finger-jointed woods. The efficiency of bending MOE, MOR and deflection showed the highest value in poplar finger-jointed wood with the lowest density of three species, and the lowest value in oak finger-jointed wood with the highest density of three species. The values markedly decreased with increasing finger pitch for finger-jointed wood glued with polyvinyl acetate (PVAc) resin for all tested species, whereas for the finger-jointed wood glued with resorcinol-phenol formaldehyde (RPF) resin, the influence of finger pitch on the efficiency of MOE was not found in all tested species, and those on the efficiency of MOR and deflection indicated the same trend as finger-jointed wood glued with PVAc resin in the case of pine and oak finger-jointed wood with higher densities. It was found that the values tended to decrease with increasing density of species on the whole and the desirable finger pitches were L (6.8 mm) for poplar, M (4.4 mm) for pine and S (3.5 mm) for oak in a view of economy. For finger-jointed wood glued with PVAc resin, the fitness between a tip and a root width of a pair of fingers δ of 0.5 mm indicated the highest efficiency of MOE for all species. And, the influence of δ on MOR was only found in oak finger-jointed wood glued with RPF resin and the desirable δ value for oak was 0.1 mm. However, it was found that the influence of δ on the strength performance was very small.

• 한국항공우주학회지
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• 제50권11호
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• pp.791-800
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• 2022

능동 진동 제어 시스템(Active vibration control system, AVCS)을 이용하여 헬리콥터 기체의 능동 진동 제어 시 우수한 진동 제어 성능을 얻기 위하여서는 진동 상쇄 하중 발생기의 개수, 위치 및 하중 방향의 조합의 최적화가 중요하다. 따라서 고려 가능한 모든 하중 발생기의 조합에 대하여 헬리콥터 기체에 대한 AVCS의 진동 제어 성능을 조사하기 위해 Exhaustive 시험 기법을 적용한 AVCS 프레임워크를 구축하였다. 로터 진동 하중 해석, 기체 진동 응답 해석 및 AVCS 시뮬레이션 연구를 수행하기 위해 DYMORE II, MSC.NASTRAN 및 MATLAB Simulink 등 다양한 프로그램을 사용하였다. 이를 이용하여 비행 속도 158 knots의 UH-60A 헬리콥터에 대한 AVCS 적용을 위한 CRFG 조합을 최적화하였다. 최적의 CRFG 조합이 적용된 AVCS를 통해 UH-60A 헬리콥터의 4P 기체 진동 응답을 능동 제어한 결과, 기체의 주요 위치에서 4P 기체 진동 응답이 19.35~98.07%만큼 감소될 수 있었다.

• 천문학회보
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• 제45권1호
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• pp.43.1-43.1
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• 2020

Cassiopeia A (Cas A) is a young supernova remnant (SNR) where we observe the interaction of SNR blast wave with circumstellar medium. From the early optical studies, dense, slowly-moving, N-rich "quasi-stationary flocculi" (QSF) have been known. These are probably dense CNO-processed circumstellar knots that have been engulfed by the SNR blast wave. We have carried out near-infrared, high-resolution (R=45,000) spectroscopic observations of ~40 QSF, and here we present the result on a QSF knot (hereafter 'Knot 24') near the SNR boundary of Cas A. The average [Fe II] 1.644 um spectrum of Knot 24 has a remarkable shape with a narrow (~8 km/s) line superposed on the broad (~200 km/s) line emitted from shocked gas. The spatial morphology and the line parameters indicate that Knot 24 has been partially destroyed by a shock wave and that the narrow line is emitted from the unshocked material heated/ionized by the shock radiation. This is the first detection of the emission from the pristine circumstellar material of the Cas A supernova progenitor. We also detected H Br gamma and other [Fe II] lines corresponding to the narrow [Fe II] 1.644 um line. For the main clump where we can clearly identify the shock emission associated with the unshocked material, we analyze the observed line ratios using a shock model that includes radiative precursor. The analysis indicates that the majority of Fe in the unshocked material is in the gas phase, not depleted onto dust grains as in the general interstellar medium. We discuss the non-depletion of Fe in QSF and its implications on the immediate progenitor of the Cas A supernova.