• 천문학회보
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• 제43권1호
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• pp.33.1-33.1
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• 2018

The differential rotational properties of early-type galaxies (ETGs) revealed by integral field spectroscopy surveys is arguably one of the most exciting findings in the galaxy evolution study during the past decade. Numerical studies have shown that galaxy mergers under various configurations can reproduce the observed distribution of ETG spin. However, we suggest an alternative scenario for the spin evolution of a large fraction of ETGs. Using the Horizon-AGN simulation, we follow the spin evolution of 10037 color-selected ETGs more massive than 1010 Msun that are divided into four groups: cluster centrals (3%), cluster satellites (33%), group centrals(5%), and field ETGs (59%). We find a strong mass dependence of the slow rotator fraction, fSR, and the mean spin of massive ETGs. Although the environmental dependence is not clear in the fSR, it is visible in the mean value of the spin parameter. The environmental dependence is driven by the satellite ETGs whose spin gradually decreases as their environment becomes denser. Galaxy mergers appear to be the main cause of total spin changes in 94% of central ETGs of halos with Mvir > 1012.5 Msun, but only 22% of satellite and field ETGs. We find that non-merger induced tidal perturbations better correlate with the galaxy spin-down in satellite ETGs than mergers. Given that the majority of ETGs are not central in dense environments, we conclude that non-merger tidal perturbation effects played a key role in the spin evolution of ETGs observed in the local (z < 1) universe.

• 천문학회보
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• 제38권1호
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• pp.34.2-34.2
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• 2013

Spin distribution of dark matter halos in a cosmological N-body simulation is well fitted by a log-normal distribution, but the origin of the log-normal like shape is still unknown. To understand the evolution of spin and the origin of spin distribution, we have studied the change of the angular momentum of simulated halos through their merging histories. First, we traced merging histories of the dark matter halos and measured the probability distribution of the angular momentum changes from a series of simulations. We were able to fit the angular momentum changes with the Gaussian distribution in spaces of M, spin, ${\Delta}M$. Using the simulated merging trees and the distribution of angular momentum changes during the merging events, we can recover the spin distribution of halos over the various mass scales.

• 한국기계가공학회지
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• 제10권6호
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• pp.146-151
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• 2011

Wax spin coating is a part of several wafer handling processes in the silicon wafer polishing station. It is important to ensure the wax layer free of contamination to achieve the high degree of planarization on wafers after wafer polishing. Three-dimensional air flow characteristics in a wax spin coater are numerically investigated using computational fluid dynamics techniques. When the bottom of the wax spin coater is closed, there exists a significant recirculation zone over the rotating ceramic block. This recirculation zone can be the source of wax layer contamination at any rotational speed and should be avoided to maintain high wafer polishing quality. Thus, four air suction ducts are installed at the bottom of the wax spin coater in order to control the air flow pattern over the ceramic block. Present computational results show that the air suction from the bottom is quite an effective method to remove or minimize the recirculation zone over the ceramic block and the wax coating layer.

• Bulletin of the Korean Chemical Society
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• 제14권1호
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• pp.21-29
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• 1993

For the study of relaxation processes in complex spin system, a general master equation, which can be used to simulate a vast range of pulse experiments, has been formulated using the Liouville representation of quantum mechanics. The state of a nonequilibrium spin system in magnetic field is described by a density vector in Liouville space and the time evolution of the system is followed by the application of a linear master operator to the density vector in this Liouville space. In this master equation the nuclear spin relaxation due to intramolecular dipolar interaction or randomly fluctuating field interaction is explicitly implemented as a relaxation supermatrix for a strong coupled two-spin (1/2) system. The whole dynamic information inherent in the spin system is thus contained in the density vector and the master operator. The radiofrequency pulses are applied in the same space by corresponding unitary rotational supertransformations of the density vector. If the resulting FID is analytically Fourier transformed, it is possible to represent the final nonstationary spectrum using a frequency dependent spectral vector and intensity determining shape vector. The overall algorithm including relaxation interactions is then translated into an ANSIFORTRAN computer program, which can simulate a variety of two dimensional spectra. Furthermore a new strategy is tested by simulation of multiple quantum signals to differentiate the two relaxation interaction types.

• 한국정보처리학회:학술대회논문집
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• 한국정보처리학회 2016년도 춘계학술발표대회
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• pp.493-496
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• 2016

차량 전장용 소프트웨어의 안정성을 플랫폼 단계에서 테스트 및 검증을 수행하면 많은 비용이 소요된다. 본 연구에서는 플랫폼 단계에서 차량용 내장형 소프트웨어를 테스트하기 이전에 Spin 모델 검증기를 활용하여 전장용 소프트웨어의 기본단위인 타스크들의 행위를 모의 실험함으로써 시스템의 설계오류를 검증할 수 있는 도구를 개발하였다. 본 연구에서는 운영체제와 환경설정 및 제어 프로그램이 수행할 타스크들을 모델로 구축하고, 모델 검증 도구 Spin을 이용하여 타스크의 상태변화를 확인할 수 있었으며, NuSMV를 이용한 방식과 비교하여 다양한 장점들을 확인하였다.

• Journal of Magnetics
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• 제5권3호
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• pp.90-98
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• 2000

The change in the magnetic properties of a spin-valve multilayer with the structure IrMn (9 m)/CoFe (4 nm)/Cu (2.6 nm)/CoFe (2 nm)/NiEe (6 nm) is investigated as a function of the size and the aspect ratio. At a fixed aspect ratio (the length/width ratio) of 2, the magnetostatic interactions begin to affect the magnetic properties substantially at a spin-valve length of 5 $\mum$, and, at a length of 1 $\mum$, they become even more dominant. In the case of a fixed multilayer size (2.4 $\mum$) which is indicated by the sum of the length and the width, magnetization change occurs by continuous spin-reversal and M-H loops are characterized by no or very small hysteresis at aspect ratios smaller than unity, At aspect ratios greater than unity, magnetization change occurs by spin-flip resulting in squared hysteresis loops. A very large changes in the coercivity and the bias field is observed, and these results are explained by two separate contributions to the total magnetostatic interactions: the coercivity by the self-demagnetizing field and the bias field by the interlayer magnetostatic interaction field.

• 정보저장시스템학회논문집
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• 제2권3호
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• pp.178-183
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• 2006

A Blu-ray disc, which has a more than 25GB optical capacity, has been known as a promising next-generation optical disc format. It commonly has a 1.1 mm thick substrate and a 0.1 mm thick cover layer for beam transmitting and the protection of the reflecting surface. The cover layer is generally formed by the spin coating process. However, in conventional spin coating, small bumps are formed along the rim of the disc, which results in the fatal reading error. Numerical simulation of the thin film flow behaviors during spin coating with the commercial solver and optimal spinning conditions was obtained. Thickness distribution of the cover layer according to the variation of substrate's edge shape could be calculated as well. By modifying the shape of the substrate edge shape, the bumps along the disc rim could be minimized, and it was proved that the chamfered edge, around $5{\sim}10$ degree, is the simplest and most effective way to minimize the bumps.

• 반도체디스플레이기술학회지
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• 제10권1호
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• pp.1-6
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• 2011

In this paper, the air flow induced by the rotating flat disk is numerically investigated in a hope to better understand the air flow structures inside the wax spin coater for a silicon wafer polishing station. Due to the complex inner geometry of actual spin coater such as the casing around the rotating ceramic block and servo motor, recirculation of air flow is inevitably found on the coating target if the internal space of spin coater is closed at the bottom and it could be the possible source of contamination on the wax coating. By numerical flow simulation, we found that it is necessary to install the air vent at the bottom and to apply the sufficient air suction in order to control the path of air flow and to eliminate the air recirculation zone above the spinning surface of coating target.

• Investigative Magnetic Resonance Imaging
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• 제4권1호
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• pp.42-51
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• 2000

목적: Projection-type Fast Spin Echo (PFSE) 영상 기법은 일반적인 Fast Spin Echo (FSE) 기법과 비교하여 환자의 움직임과 혈류에 강한 장점이 있는 반면. $T_2$ 대조도(contrast)를 조절하기가 어려운 단점이 있다. 본 연구에서는 PFSE의 대조도를 이론적으로 분석하였고 컴퓨터 모의실험을 통하여 다양한 effective echo time (TE) 을 갖는 일반적인 FSE와 비교, 분석하였다. 또한 인체 실험을 통하여 제안한 PFSE 영상기법으로 움직 임과 혈류에 강인한 $T_2$ 강조 영상을 얻을 수 있음을 보였다. 대상 및 방법: 본 연구에서는 1.OT 전신 MRI 시스템에서 새로운 k-space의 배치를 갖는 PFSE 펠스 시권스를 구현하여, PFSE와 FSE 방식의 $T_2$ 대조도를 컴퓨터 모의설험과 인체 실험을 통하여 비교, 분석하였다. 컴퓨터 모의실험에서는 서로 다른 $T_2$ 값을 갖는 팬텀을 구현하여 다양한 effective TE에 대한 FSE 영상과 PFSE 영상을 재구성하여 대조도를 비교하였다. 인체 설험에서는 multi-slice $T_2$ 강조 두부 영상을 PFSE와 FSE로 얻어 영상기법간의 $T_2$ 대조도를 비교하였다. 결과: 이론적인 분석에서 PFSE의 $T_2$ 대조도는 effective TE가 80-l00ms 정도의 FSE 영상과 등가하게 나타나 $T_2$ 강조 영상을 얻을 수 있을 것으로 판단되었다. 컴퓨터 모의실험에서 PFSE 재구성 영상은 effective TE가 96ms인 FSE 영상과 대조도가 비슷하게 나타났다. 인체 실험에 서도 PFSE 영상은 effective TE가 96ms인 FSE 영상과 비슷하게 나타났으며. PFSE 방법이 FSE 방법에 비하여 움직 엄과 혈류와 관련한 artifact에 강인함을 확인 할 수 었었다. 결론: PFSE 기법은 k-space의 극좌표계에서 서로 다른 각도를 갖는 여러 line틀을 다중 스핀 에코 기법으로 측정하는 방식이다. PFSE기법은 FSE와 비교하여 환자의 움직임과 혈류에 강한 장점이 있는 반면, $T_2$ 대조도를 조절하기가 어려운 단점이 있다. 본 연구에서는 PFSE 방식으로 FSE와 대등한 $T_2$ 대조도 ($T_2$ 강조 영상)를 얻을 수 있음을 이론과 컴퓨터 모의실험 밝히고, 인체 실험을 통하여 확인하였다.

• 한국자기공명학회논문지
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• 제22권3호
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• pp.54-63
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• 2018

Nymphaea tetragona, also known as waterlilies, is aquatic plant in the family of Nymphaeceae. Three flavonoids(3, 4, and 5) and one mixed flavonoids were separated from this plant. The mixed flavonoid consisted of two flavonoids; a well-known quercetin(1) and a new natural flavonoid(2). The latter also has two chiral centers and their configurations were established by ROESY experiment. Two glycoflavonoids were determined as isoquercetin and quercetin-3-O-${\beta}$-xyropyranosyl-($1{\rightarrow}2$)-${\beta}$-galactopyroside. The $^1H$ NMR spectra for 4 and 5 dissoloved in $DMSO-d_6$ solvent showed resonance proximity and and severely overlap in the glycoside region, hindering the determination of the configurations of the stereogenic centers of the sugar moieties. This problem was solved through the spin simulation. Here, the exact NMR parameters for the sugar moieties of 4 and 5 were listed.