• 소성∙가공
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• 제27권1호
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• pp.12-17
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• 2018

This paper outlines the research findings on the microstructure and mechanical properties of AZ31 Mg alloy fabricated by differential speed rolling (DSR) with respect to processing variables such as temperature, roll speed ratio (RSR), and deformation route. The resultant microstructure of the sample, deformed by 2-pass DSRs at 473 K, comprised finer grains with more uniform distribution than those at 573 and 623 K. This was due to active recrystallization, which was expected to appear during DSR at temperatures higher than 573 K. When the sample was deformed via DSR with RSR of 1:4 for the upper and lower rolls at 453 K, the values of yield and ultimate tensile strength were observed to be higher than their counterpart with RSR of 1:1. The application of sample rotation around the longitudinal axis would give rise to an excellent combination of tension strength (~330 MPa) and ductility (~20 %) at ambient temperatures. This is discussed based on its uniform fine grained structure and the softening of basal texture.

• 대한금속재료학회지
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• 제49권2호
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• pp.128-136
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• 2011

Equal channel angular pressing (ECAP) with intermediate heat treatment was employed to optimize the strength of Cu-15 wt.%Ag. Changes in microstructure, electrical properties and mechanical properties were studied as a function of pressing methods and heat treatment. ECAPed Cu-15wt.%Ag exhibited ultrafine-grained microstructures with the shape and distribution of Ag-rich lamellae dependent on the processing routes. For route A in which the sample was pressed without rotation between each pass, the initial dendrites of Ag-rich phase were elongated along the shear direction and developed into elongated filaments. For route C in which the sample was rotated by 180 degree after each pass, the morphology of initial dendrites of Ag-rich phase was not much modified and the networked structure remained even after 8 passes of ECAP. For route Bc in which the sample was rotated by 90 degree after each pass, the initial dendrites became finer by fragmentation with no pronounced change of the shape and distribution of Ag-rich lamellae. The strength of Cu-15wt.%Ag ECAPed using route Bc was found to be greater than those ECAPed using route A, suggesting that the substructural strengthening is more effective in strengthening than the interface strengthening.

• 천문학회보
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• 제45권1호
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• pp.33.2-33.2
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• 2020

Our HI monster sample is a set of local HI-rich galaxies identified by the ALFALFA survey (Arecibo Legacy Fast Survey ALFA) at z<0.08. Intriguingly, they are also found with a relatively large molecular gas reservoir compared to the galaxies with similar stellar mass and color, yet their star formation rate is quite comparable to normal spirals. This makes our HI monsters good candidates of galaxies in the process of gas accretion which may lead to the stellar mass growth. One feasible explanation for their relatively low star formation activity for a given high cool gas fraction is the gas in monsters being too turbulent to form stars as normal spirals. In order to verify this hypothesis, we probe the molecular gas kinematics of 10 HI monsters which we observed using the Atacama Large Millimeter/sub-millimeter Array (ALMA). We utilize the tilted ring model to investigate what fraction of the molecular gas in the sample is regularly and smoothly rotating. In addition, we model the molecular gas disk using the GALMOD package of the Groningen Image Processing System (GIPSY) and compare with the observations to identify the gas which is offset from the 'co-planar differential rotation'. Based on the results, we discuss the possibility of gas accretion in the sample, and the potential origin of non-regularly rotating gas and the inefficient star formation.

• 임산에너지
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• 제19권2호
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• pp.69-78
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• 2000

다릅나무의 입지별 생장특성을 알아보기 위해 강원도 평창군 중왕산 지역에서 30m×30m 크기의 조사구 28곳을 선정하여 식생 및 환경조사를 실시하였으며, 그 중 해발고가 약 100m 간격으로 있는 5곳의 조사구에서 각각 다릅나무 2그루씩을 선택하여 수간석해를 하였다. 그 결과, ⑴ 다릅나무의 수고 생장은 모든 입지에서 평균 10년까지 평균 수고 생장량이 급격한 증가를 보이다가 점차 감소하는 경향을 보였으며, 특히 해발 1,020m 이상에서 수고생장이 크게 감소하였다. ⑵ 다릅나무는 유리한 환경에서 매우 빠른 초기 수고생장과 재적 생장을 보여 물질 생산력이 높은 것으로 나타나 층층나무와 거제수나무와 같은 초기침입수종이 가지는 생장전략을 보여주었다. ⑶ 천연림에서 다릅나무의 경제적 벌기령은 50년 이상인 것으로 나타났으며, 특히 해발 840m에서는 경제적 벌기령이 60년 이상으로 나타나 고지대에 비해 더 우수한 생장을 보여주고 있었다. ⑷ 다릅나무는 수령 40년 이상에서도 경쟁목의 고사 등으로 주변 환경이 개선되면 재적생장량이 크게 증가하는 특성을 보였다.

• 천문학회보
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• 제42권2호
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• pp.42.1-42.1
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• 2017

We present the results from an extensive spectroscopic survey of the central region of the nearby galaxy cluster Abell 2199 (A2199) at z=0.03. By combining 775 new redshifts from the MMT/Hectospec observations with the data in the literature, we construct a large sample of 1624 galaxies with measured redshifts at R<30', which redsults in high spectroscopic completeness at $r_{petro,0}$<20.5 (77%). We use these data to study the kinematics and clustering of galaxies, focusing on the comparison with those of the intracluster medium (ICM) from Suzaku X-ray observations. We identify 406 member galaxies of A2199 at R<30' using the caustic technique. The velocity dispersion profile of cluster members appears smoothly connected to the stellar velocity dispersion profile of the cD galaxy. The luminosity function is well fitted with a Schechter function at $M_r$<-15. The radial velocities of cluster galaxies generally agree well with those of the ICM, but there are some regions where the velocity difference between the two is about a few hundred kilometers per second. The cluster galaxies show a hint of global rotation at R<5' with $v_{rot}=300-600kms^{-1}$, but the ICM in the same region does not show such rotation. We apply a friends-of-friends algorithm to the cluster galaxy sample at R<60' and identify 32 group candidates, and examine the spatial correlation between the galaxy groups and X-ray emission. This extensive survey in the central region of A2199 provides an important basis for future studies of interplay among the galaxies, the ICM, and the dark matter in the cluster.

• International Journal of Precision Engineering and Manufacturing
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• 제9권3호
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• pp.27-32
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• 2008

This paper describes a contact atomic force microscope (AFM) that can be used for high-speed precision measurements of microstructured surfaces. The AFM is composed of an air-bearing X stage, an air-bearing spindle with the axis of rotation in the Z direction, and an AFM probe unit. The traversing distance and maximum speed of the X stage are 300 mm and 400 mm/s, respectively. The spindle has the ability to hold a sample in a vacuum chuck with a maximum diameter of 130 mm and has a maximum rotation speed of 300 rpm. The bandwidth of the AFM probe unit in an open loop control circuit is more than 40 kHz. To achieve precision measurements of microstructured surfaces with slopes, a scanning strategy combining constant height measurements with a slope compensation technique is proposed. In this scanning strategy, the Z direction PZT actuator of the AFM probe unit is employed to compensate for the slope of the sample surface while the microstructures are scanned by the AFM probe at a constant height. The precision of such a scanning strategy is demonstrated by obtaining profile measurements of a microstructure surface at a series of scanning speeds ranging from 0.1 to 20.0 mm/s.

• 한국통신학회논문지
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• 제19권12호
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• pp.2409-2417
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• 1994

직교 이중회전 디지털 격차 필터는 고밀도 집적회로 실현에 아주 적합한 성질들을 가지고 있다. 예를 들면, 바로 옆의 프로세서들과만 연결되는 점, 규칙적인 구조를 갖는 점, 그리고 파이프라인화 할 수 있다는 점 등이다. 또한 이 필터들은 유한 워드 길이로 실현했을 때 좋은 수치적 성질을 갖는다는 것이 잘 알려져 있다. 비록 이 필터들은 '컬셋 분리 절차'를 이용하여 파이프라인화 될 수 있지만 이렇게 파이프라인화 된 필터는 귀환회로의 계산 시간에 의해 이 필터의 최대 데이터 처리속도가 제한된다는 단점이 있다. 본 논문에서는 귀환회로에 제한 받지 않고 원하는 만큼 데이타 속도를 높이거나 저파워 실현을 위한 직교 이중회선 디지탈 격차 필터의 새로운 파이프라인 방법을 제안하였다. 이 방법은 Schur 알고리즘, 필터 합성시 특정한 제약을 주는 필터 합성 방법, 그리고 다중 페이스 분해 방법에 근거하고 있다.

• 분석과학
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• 제15권6호
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• pp.529-533
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• 2002

광학이성질체 분리 컬럼, 시료처리 및 농축 컬럼이 부착된 컬럼스위칭-HPLC를 이용하여 뇨시료에서 미량의 플루비프로펜 광학이성질체를 분리 정량하는 방법을 연구하였다. 분리된 각 이성질체의 고유광회전도를 구하고, d-이성질체 및 l-이성질체를 확인하였다. 이들의 검정선의 농도범위는 각각 $0.11{\sim}5.4{\mu}g/mL$이었으며, 검출한계는 d-이성질체의 경우 $0.027{\mu}g/mL$이고, l-이성질체의 경우 $0.031{\mu}g/mL$이며, 날자간 및 날자내의 정밀도의 CV값은 각각 1.84% 이하였다. 본 분석법은 플루비프로펜 약물을 복용한 살마의 뇨중에 존재하는 플루비프로펜의 분석에 적용하였다.

• 한국전자파학회논문지
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• 제15권7호
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• pp.669-676
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• 2004

등 간격 선형 어레이로 입사하는 광대역 인코히어런트 신호의 도래각을 효율적으로 추정하는 새로운 알고리즘을 제안한다. 변환행렬을 구성하기 위하여 CSM 방법이 초기 추정각을 요구하는 반면에 제안된 방법은 전혀 초기 추정각을 필요로 하지 않는다. 이 방법의 연산과정은 먼저 신호부각 방법에 의하여 중심주파수에서의 신호 부공간을 추정 한 다음 신호 부공간 회전 방법을 통한 직교변환행렬을 구성하는 것이다. 시뮬레이션 결과 제안된 방법이 CSM 방법보다 표본바이어스 면에서 우수한 성능을 제공함을 알 수 있었다.

• 천문학회보
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• 제41권2호
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• pp.62.2-62.2
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• 2016

We present a newly developed algorithm based on a Bayesian method for 2D tilted-ring analysis of disk galaxies which operates on velocity fields. Compared to the conventional ones based on a chi-squared minimisation procedure, this new Bayesian-based algorithm less suffers from local minima of the model parameters even with high multi-modality of their posterior distributions. Moreover, the Bayesian analysis implemented via Markov Chain Monte Carlo (MCMC) sampling only requires broad ranges of posterior distributions of the parameters, which makes the fitting procedure fully automated. This feature is essential for performing kinematic analysis of an unprecedented number of resolved galaxies from the upcoming Square Kilometre Array (SKA) pathfinders' galaxy surveys. A standalone code, the so-called '2D Bayesian Automated Tilted-ring fitter' (2DBAT) that implements the Bayesian fits of 2D tilted-ring models is developed for deriving rotation curves of galaxies that are at least marginally resolved (> 3 beams across the semi-major axis) and moderately inclined (20 < i < 70 degree). The main layout of 2DBAT and its performance test are discussed using sample galaxies from Australia Telescope Compact Array (ATCA) observations as well as artificial data cubes built based on representative rotation curves of intermediate-mass and massive spiral galaxies.