• 한국HCI학회:학술대회논문집
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• 2007.02a
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• pp.675-680
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• 2007

컴퓨터를 활용하는 응용 수많은 가시화 방법론들 중 하나인 3차원 모델링은 경우에 따라 더 구체적인 이해를 위해 모형 형태로 조형작업을 하기도 한다. 그러나, 이러한 입체 모델의 조형은 수작업으로 할 경우에 많은 시간과 노력을 필요로 한다. 이를 해결하기 위하여 Rapid Prototyping기술이 개발 및 보급되어왔다. 이러한 장비와 OS를 포함한 관련 소프트웨어는 고가이기도 하고 동시에 1인 밖에 사용할 수 없는 자원인 경우가 많다. 또한, 사용하기 위하여 장비가 위치한 곳 까지 이동하여야 하는 경우가 많다. 그러나, 원격데스크탑 형태의 인터페이스와 장비 구동과 동작 과정을 모니터링 할 수 있는 인터페이스, 임차를 위한 사용자관리 시스템 등을 포함한 클러스터 컴퓨터 환경으로 구성하고 인터넷을 통하여 제공하면 비록 제한된 수준이기는 하지만, 현업에서 사용하는 고가의 Rapid Prototyping장비를 실제 이용하는데 무리가 없는 임차 및 공유 가능 자원으로 변화 시킬 수 있다. 이 임차 방법론은 고가의 산업 장비와 소프트웨어를 공유할 수 있는 실제적인 예를 제공한다.

• The Bulletin of The Korean Astronomical Society
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• v.35 no.1
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• pp.41.2-41.2
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• 2010

The infrared astronomy satellite AKARI/FIS (Far-Infrared Surveyor) performed all-sky survey in 4 Far-IR bands (50 - 200${\mu}m$ range). It observed around 94% of the whole sky twice or more with a higher spatial resolution and a wider wavelength coverage than that of previous all-sky mission, IRAS. The AKARI/FIS bright source catalogue ${\beta}-2$ is the second released version which included around 290,000 point sources. It provides us with more reliable position and flux information, and around 4 times larger number of sources compared with the first version of catalogue. The sensitivity limit at $90{\mu}m$ band is 0.6 Jy and the estimated flux uncertainty is 20-35% for bright sources. The catalogue will be open to public in this year after the improvement of accuracy, reliability and completeness.

• Communications of the Korean Mathematical Society
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• v.10 no.2
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• pp.293-300
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• 1995

Let $R = k[y_1,\cdots,y_n] \otimes E[x_1, \cdots, x_n]$ with characteristic $k = p > 2$ (odd prime), where $$\mid$y_i$\mid$ = 2, $\mid$x_i$\mid$ = 1$ and $y_i = \betax_i, \beta$ is the Bockstein homomorphism. Topologically, $R = H^*(B(Z/p)^n,k)$. For a symmetric group $\sum_n, R^{\sum_n} = k[\sigma_1,\cdots,\sigma_n] \otimes E[d\sigma_1, \cdots, d\sigma_n]$ where d is the derivation satisfying $d(y_i) = x_i$ and $d(x_iy_i) = x_iy_i + x_jy_i, 1 \leq i, j \leq n$. We give a direct proof of this theorem by using induction.

• Journal of Astronomy and Space Sciences
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• v.33 no.3
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• pp.147-166
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• 2016

A radio-quiet γ-ray pulsar is a neutron star that has significant γ-ray pulsation but without observed radio emission or only limited emission detected by high sensitivity radio surveys. The launch of the Fermi spacecraft in 2008 opened a new epoch to study the population of these pulsars. In the 2^nd Fermi Large Area Telescope catalog of γ-ray pulsars, there are 35 (30 % of the 117 pulsars in the catalog) known samples classified as radio-quiet γ-ray pulsars with radio flux density (S₁₄₀₀) of less than 30 μJy. Accompanying the observations obtained in various wavelengths, astronomers not only have the opportunity to study the emitting nature of radio-quiet γ-ray pulsars but also have proposed different models to explain their radiation mechanism. This article will review the history of the discovery, the emission properties, and the previous efforts to study pulsars in this population. Some particular cases known as Geminga-like pulsars (e.g., PSR J0633+1746, PSR J0007+7303, PSR J2021+4026, and so on) are also specified to discuss their common and specific features.

• Proceedings of the Korean Society of Precision Engineering Conference
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• 2002.10a
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• pp.954-957
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• 2002

The objective of design process modeling is a systematic support of rapid redesign process fur a modified input data. The design process modeling is realized by storing key parameters or geometric entities used in the intermediate design steps and reusing them for change of the designed parts or assemblies according to the modified input. In this paper, we adopted and implemented the design process modeling approach to our injection mold design system developed based on the Unigraphics system. It was proved that the productivity of mold redesign process is raised highly by introducing the design process modeling technique mold design system.

• 한국금형공학회:학술대회논문집
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• 2008.06a
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• pp.175-181
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• 2008

The technologies of mold design, manufacturing, injection molding process and computer aided engineering(CAE) are developed rapidly with the growth of plastic product market. Injection molding process optimum design can not be easily determined. This study was determined factors and levels which carried out to analyze an influence of narrow pitch BGA socket warpage and performed investigating the main effect and interaction effect between factors using design of experiment. The result of this paper is injection time and packing pressure are affect on narrow pitch BGA socket warpage at injection molding.

• The Journal of Korean Medicine
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• v.19 no.2
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• pp.100-111
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• 1998

This study is designed to investigate the effects of Saengmaegsan extract on cultured myocardial cell sheets affected by oxygen tension change. The results were as follows : 1. Saengmaegsan meaningfully restored the cellular activity decrease in the cultured myocardial cells affected by high oxygen tension. 2. Saengmaegsan meaningfully lessened the degree of total protein decrease in the myocardial cells caused by high oxygen tension. 3. Saengmaegsan meaningfulJy refrained from syntetic decrease of 4-hydroxyproline in both low oxygen tension group and high oxygen tension group.

• Journal of Information Technology Applications and Management
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• v.21 no.3
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• pp.53-64
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• 2014

It is important to keep learners' feeling positive during learning to enhance learning performance. According to flow theory,challenge-skill balance is a precondition for flow experience: Learners feel anxiety when the challenge of learning is higher than their ability, feel boredom when the challenge of learning is lower than learners' ability, and engage in flow status when the challenge of learning matches the learners' ability. However, the current empirical study reveals that emotions related to enjoyment may appear when the learners' skill is equal to or higher than the learning challenge. Nevertheless, boredom emotion may appear when learners perceive the courses are difficult but unimportant. These empirical survey results revealed the necessary of rethinking the appearance of boredom and enjoyment emotions in computer education.

• Journal of The Korean Astronomical Society
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• v.39 no.1
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• pp.1-7
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• 2006

We present the results of a highly sensitive (${\sim}10$ mK rms) survey toward the central parts of 22 barred spiral galaxies in $^{12}CO(1-0)$ line using the NRAO 12m telescope at Kitt Peak. Seven of the target galaxies were detected in CO; NGC 3686 has been detected with CO for the first time. We estimated central CO fluxes of $50{\sim}1000\;Jy\;km\;s^{-1}$ and molecular gas masses of $10^7{\sim}10^8\;M_{\odot}$ for those galaxies.

• Proceedings of the KIEE Conference
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• 2006.10a
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• pp.89-90
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• 2006

We synthesized emissive materiaJs, nameJy $Zn(HPB)_2$. The fundamentaJ structures of the OLEDs were ITO / NPB (40 nm) $Zn(HPB)_2$ (40 nm) / $Alq_3$:DCJTB (20, 30, or 40 nm) / LiF / AI. We varied the thickness of $Alq_3$:DCJTB from 20 nm to 40nm. We measured current density-voJtage and luminance-voJtage characteristics at room temperature. When the thickness of the Alq3:DCJTB layer was 40 nm, white emission is achieved. The CIE coordinates are (0.32, 0.33) at an applied voltage of 14V.