• 대한전기학회:학술대회논문집
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• 대한전기학회 1993년도 하계학술대회 논문집 B
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• pp.954-956
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• 1993

This paper describes the process of levitation melting of metals in an axisymmetric induction heating system. This process has advantages of low heat losses, heating with short times and clean operating conditions. The shape of molten metal is determined using sensitivity analysis and optimization technique. Electromagnetic, gravitational and surface tension energies are considered, and these energies are used as an objective function in optimization process. Electromagnetic field are calculated using the finite element method. The fact that volume is constant in the process is also considered as an equality constraint.

• 대한수학회지
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• 제46권5호
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• pp.979-995
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• 2009

As warped product manifolds provide an excellent setting to model space time near black holes or bodies with large gravitational field, the study of these manifolds assumes significance in general. B. Y. Chen [4] initiated the study of CR-warped product submanifolds in a Kaehler manifold. He obtained a characterization for a CR-submanifold to be locally a CR-warped product and an estimate for the squared norm of the second fundamental form of CR-warped products in a complex space form (cf [6]). In the present paper, we have obtained a necessary and sufficient conditions in terms of the canonical structures P and F on a CR-submanifold of a nearly Kaehler manifold under which the submanifold reduces to a locally CR-warped product submanifold. Moreover, an estimate for the second fundamental form of the submanifold in a generalized complex space is obtained and thus extend the results of Chen to a more general setting.

• 천문학회지
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• 제2권1호
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• pp.1-9
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• 1969

On the instantaneous tidal relaxation approximation, formulae are derived for the ellipticities and virial theorem of a slightly flattened homogeneous rotating cluster (the largest axis of the cluster is directed towards the Galactic center), in terms of the Galactic tidal force and the characteristic intrinsic plus orbital angular velocity. The expression for a purely tidally-determined ellipticity is identical to that for an incompressible fluid body of uniform density. Orbital motion generally contributes significantly to the shape of the cluster. The virial theorem is identical to that for an isolated cluster except that the gravitational potential energy is multiplied by (1-${\chi}$), where ${\chi}$ is a positive tidal correction term. To obtain the actual mass of a cluster, the virial theorem mass based on an isolated cluster should be multiplied by the factor 1/(1-${\chi}$). The formulae are applied to open star clusters, the globular cluster ${\omega}$ Centauri, and dwarf elliptical galaxies in the Local Group.

• Nuclear Engineering and Technology
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• 제53권11호
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• pp.3772-3783
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• 2021

This work proposes a new efficient meta-heuristic optimization algorithm called Gamma Ray Interactions Based Optimization (GRIBO). The algorithm mimics different energy loss processes of a gamma-ray photon during its passage through a matter. The proposed novel algorithm has been applied to search for the global minima of 30 standard benchmark functions. The paper also considers solving real optimization problem in the field of nuclear engineering, radioisotope identification. The results are compared with those obtained by the Particle Swarm Optimization, Genetic Algorithm, Gravitational Search Algorithm and Grey Wolf Optimizer algorithms. The comparisons indicate that the GRIBO algorithm is able to provide very competitive results compared to other well-known meta-heuristics.

• 천문학논총
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• 제33권3호
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• pp.45-57
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• 2018

Low-mass star-formation studies deal with the birth of individual solar-type stars as it occurs in nearby molecular clouds. While this isolated mode of star formation may not represent the most common form of stellar birth, its study often provides first evidence for the general ingredients of star formation, such as gravitational infall, disk formation, or outflow acceleration. Here I briefly review the current status and the main challenges in our understanding of low-mass star formation, with emphasis in the still mysterious pre-stellar phase. In addition to presenting by-now classical work, I also show how ALMA is starting to play a decisive role driving progress in this field.

• 천문학회보
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• 제43권2호
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• pp.29.3-29.3
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• 2018

Neutrino astronomy is now possible as the technology to detect neutrinos has been advancing. Current and planned neutrino-detecting facilities can be operated as a conventional telescope because they can measure the direction toward the celestial sources as well as their physical properties like energy. Together with gravitational wave, neutrino astronomy opens a new field of astronomy, often called, multi-messenger astronomy, which also involves "traditional" electro-magnetic-wave-detection-based astronomy. Expecting that Korean Neutrino Observatory (KNO) will be one of the best neutrino observatories when it is constructed, a group of Korean astronomers and astrophysicists formed a working group and began to investigate possible astronomical neutrino sources that could be detected by KNO and other neutrino observatories. This talk presents the recent activities of the working group and introduces the list of possible neutrino sources.

• 천문학회보
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• 제44권1호
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• pp.64.1-64.1
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• 2019

Thermal fracture and cracking near the perihelion are found to be a possible mechanism to produce the dust trail of the near-Earth asteroid, (3200) Phaethon (Jewitt and Li, 2013, ApJ 771, L36). It is, however, not well understood how the debris particles were escalated from the regolith against the asteroid's gravity. Thus, the scenario that these debris particles are responsible for the detected activities (Li and Jewitt, 2013, ApJ, 145, 154), is not complete yet. Here, we hypothesize that the thermal radiation pressure around the perihelion passage would exert substantial force outwards from the regolith on dust grains, and they can be lifted up and contributes the dust tail formation with further help of solar radiation pressure. Our modeling indicates that particles with sizes of roughly ~1-10 micron can be ejected from Phaethon by the mechanism, while a detailed model of gravitational field is required for accurate estimation of the particle size range. Our idea is not necessarily limited to Phaethon case, but is applicable to any atmosphereless bodies.

• 천문학회지
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• 제29권spc1호
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• pp.19-21
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• 1996

We apply topological measures of clustering such as percolation and genus curves (PC & GC) and shape statistics to a set of scale free N-body simulations of large scale structure. Both genus and percolation curves evolve with time reflecting growth of non-Gaussianity in the N-body density field. The amplitude of the genus curve decreases with epoch due to non-linear mode coupling, the decrease being more noticeable for spectra with small scale power. Plotted against the filling factor GC shows very little evolution - a surprising result, since the percolation curve shows significant evolution for the same data. Our results indicate that both PC and GC could be used to discriminate between rival models of structure formation and the analysis of CMB maps. Using shape sensitive statistics we find that there is a strong tendency for objects in our simulations to be filament-like, the degree of filamentarity increasing with epoch.

• 지질공학
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• 제31권3호
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• pp.283-293
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• 2021

고해상 드론 기반의 지형 정보와 중력장 데이터를 이용하여 다짐지반의 모양과 균질성을 분석하였다. 지형과 수문 모형에서 계산된 지형요소 중 곡률은 다짐과정에서 발생한 지형의 변화를 효과적으로 보여 주었으며 이를 통해 불균질 다짐 영역을 확인할 수 있다. 지형 정보의 적정 해상도는 10 cm 정도였다. 성토지반의 공간적인 밀도변화를 분석하기 위해 중력장 해석을 수행하였으며 완전 부게이상의 변화로부터 불균질 다짐 영역과 지하 밀도구조 모델링을 통해 다짐도 차이에 의한 불균질 영역을 파악하였다. 연구결과로부터 지형요소와 중력장 해석법은 다짐된 지반의 균질성을 평가법이 될 수 있을 것으로 판단된다.

• 한국식품저장유통학회지
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• 제18권3호
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• pp.294-301
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• 2011

중첩에너지(FGFE)가 방사선조사식품의 판별 특성에 미치는 영향을 연구하고자, 밀과 대두를 시료로 0-5 kGy의 감마선을 조사한 다음 FGFE 처리된 시료의 발광특성(광자극발광, 열발광)과 발아율의 변화를 처리직후와 6개월 저장 후 비교하였다. 조사식품의 스크리닝 방법으로서 두 시료에 대한 광자극발광(PSL) 분석 결과, 비 조사 시료(0 kGy)는 모두 700 photon counts/min 이하의 음성(negative)을 나타내었고, 1 kGy 이상 조사시료는 5,000 photon counts/min 이상의 양성(positive)을 나타내엇다. 그러나 FGFE 처리된 조사시료는 모두 700-5,000 사이의 중간값(intermediate)을 나타내어 FGFE 처리는 조사시료의 광자극 발광을 유의적으로 감소시켰으며, 6개월 저장 후에도 유사한 결과가 유지되었다. 조사식품의 판별확증방법으로서 두 시료에 대한 열발광(TL) 분석 결과, 조사시료와 조사 후 FGFE 처리시료 모두 $150-250^{\circ}C$ 사이에서 발광곡선이 나타났고, TL ratio ($TL_1/TL_2$) 또한 0.1 이상을 보여 조사여부 판별에는 큰 차이가 없었다. 그러나 발광곡선의 온도범위는 FGFE 처리에 따라 $150-200^{\circ}C$에서 $180-230^{\circ}C$로 shift 현상이 나타났으며, 조사시료의 TL 강도 또한 FGFE 처리로써 37-60%의 감소를 보였다. 저장 6개월 후에는 모든 시료구에서 TL 강도가 다소 감소하였으나 조사여부의 판별은 가능하였다. 밀과 대두의 발아율에서 조사시료(5 kGy)는 비 조사 시료 대비 72%를 나타내었으나 FGFE 처리로써 85%로 증가되었다. 저장 6개월 후 조사시료(5 kGy)의 발아율은 63%로 감소하였으나, 조사 후 FGFE 처리시료는 91%의 발아율 증가를 나타내어 이에 대한 보다 구체적인 연구가 필요한 것으로 사료된다.