• Korean Chemical Engineering Research
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• v.61 no.4
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• pp.627-634
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• 2023

Graphitic carbon nitride (g-C₃N₄) has attracted considerable attention since its discovery for its catalysis of water splitting to hydrogen and oxygen under visible light irradiation. However, pristine g-C₃N₄ confers only low photocatalytic efficiency and requires surface cocatalysts to reach moderate activity due to a lack of accessible surface active sites. Inspired by the high specific surface area and superior electron transfer of graphene, we developed a strongly coupled binary structure of graphene and g-C₃N₄ aerogel with 3D porous skeleton. The as-prepared 3D structure photocatalysts achieve a high surface area that favors efficient photogenerated charge separation and transfer, enhances the light-harvesting efficiency, and significantly improves the photocatalytic hydrogen evolution rate as well. The photocatalyst performance is observed to be optimized at the ratio 3:7 (g-C₃N₄:GO), leading to photocatalytic H₂ evolution of 16125.1 mmol. g^-1. h^-1 under visible light irradiation, more than 161 times higher than the rate achieved by bulk g-C₃N₄.

• Journal of applied mathematics & informatics
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• v.28 no.1_2
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• pp.383-395
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• 2010

In the present paper, we construct the traveling wave solutions involving parameters of nonlinear evolution equations in the mathematical physics via the (3+1)- dimensional potential- YTSF equation, the (3+1)- dimensional generalized shallow water equation, the (3+1)- dimensional Kadomtsev- Petviashvili equation, the (3+1)- dimensional modified KdV-Zakharov- Kuznetsev equation and the (3+1)- dimensional Jimbo-Miwa equation by using a simple method which is called the ($\frac{G'}{G}$)- expansion method, where $G\;=\;G(\xi)$ satisfies a second order linear ordinary differential equation. When the parameters are taken special values, the solitary waves are derived from the travelling waves. The travelling wave solutions are expressed by hyperbolic, trigonometric and rational functions.

• Proceedings of the Korean Information Science Society Conference
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• 2005.11a
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• pp.265-267
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• 2005

본 논문에서는 무선 랜과의 인터워킹 등 새로운 특징을 갖는 주요 기능들을 추가하기 위한 기반 시스템인 3G Evolution 시스템 개발에 필요한 액세스 시스템 내의 서브 시스템인 RRCS(Radio Resource Control Subsystem)를 구현 및 검증하기 위하여 단말-기지국간 무선 액세스 프로토콜을 형식 기술 언어인 SDL(Specification and Description Language)을 이용해 구현하였다. 여기서 효율적 시스템 설계를 위해 복잡한 각 메시지 처리 함수는 C 언어를 이용해 라이브러리화하고 이를 SDL 시스템 내에서 호출하도록 지원하는 방법을 사용했다.

• Publications of The Korean Astronomical Society
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• v.30 no.2
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• pp.267-268
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• 2015

One of the long-standing problems in modern astronomy is the curious division of globular clusters (GCs) into two groups, according to the mean period (<$P_{ab}$>) of type ab RR Lyrae variables. In light of the recent discovery of multiple populations in GCs, we suggest a new model explaining the origin of the Sandage period-shift and the difference in mean period of type ab RR Lyrae variables between the two Oosterhoff groups. In our models, the instability strip in the metal-poor group II clusters, such as M15, is populated by second generation stars (G2) with enhanced helium and CNO abundances, while the RR Lyraes in the relatively metal-rich group I clusters like M3 are mostly produced by first generation stars (G1) without these enhancements. This population shift within the instability strip with metallicity can create the observed period-shift between the two groups, since both helium and CNO abundances play a role in increasing the period of RR Lyrae variables. The presence of more metal-rich clusters having Oosterhoff-intermediate characteristics, such as NGC 1851, as well as of most metal-rich clusters having RR Lyraes with the longest periods (group III) can also be reproduced, as more helium-rich third and later generations of stars (G3) penetrate into the instability strip with further increase in metallicity. Therefore, although there are systems where the suggested population shift cannot be a viable explanation, for the most general cases, our models predict that RR Lyraes are produced mostly by G1, G2, and G3, respectively, for the Oosterhoff groups I, II, and III.

• Proceedings of the Korean Society of Broadcast Engineers Conference
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• 2008.02a
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• pp.99-102
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• 2008

차세대 이동 통신 서비스 4G는 이동 중 100Mbps, 정지 중 1Gbps급 전송 속도를 제공하는 미래 무선 통신 기술이다. 이것은 현재 상용서비스가 이뤄지고 있는 3G HSDPA(High Speed Packet Access)의 전송속도 14Mbps에 비해 10~100배까지 빠른 속도로 무선 인터넷이 가능함으로 유선으로 인터넷을 사용할 필요가 없어진다. 현재 4G 기술로 진화하기 위한 중간 단계로써 ITU-R, 3GPP, 3GPP2, IEEE 등 세계 각국의 표준 및 기술 단체에서 새로운 무선 이동 통신 기술을 제안하고 있다. 이 중에서 2G의 GSM과 3G의 비동기식 기술 WCDMA의 진화 기술인 3GPP LTE(Long Term Evolution) 및 SAE(System Architecture Evolution)가 유력한 4G 이동 통신 기술 후보로 평가 받고 있다. 본 논문에서는 4G 기술로 주목 받고 있는 3GPP LTE 및 SAE 네트워크에서 3G 시스템 보다 진화된 서비스를 제공하기 위한 목적으로 논의되고 있는 일반적인 요구사항과 이를 만족시키기 위한 기술에 대하여 알아본다. 또한 LTE 표준화와 병행하여 네트워크의 구조를 결정하는 SAE의 구성요소와 프로토콜 구조를 소개하고 LTE 및 SAE 네트워크의 보안위협과 안전한 통신을 위한 키 관리 방법에 대하여 논의한다.

• Journal of the Korean Ceramic Society
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• v.37 no.1
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• pp.70-76
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• 2000

In order to investigate the properties of the blended cement using coarsely ground blasturnace slag blended coements which were substituted from 10 to 70 wt% low Blaine slag powder (2,000 and 3,000 cm2/g) for porland cement clinker were prepared and Cal(OH)2 contents in hydrates hydration heat the fluidity and the compressive strength were measured. As the content of slag was increased the hydration heat and the early strength was decreased and the fluidity of the cement paste was improved. The heat evolution of the cement with 2,000cm2/g slag was lower than that of 3,000 cm2/g slag blended cement. Especially the heat evolution of 60wt% or above slag blended cement was similar to that of belite rich cement.

• Information and Communications Magazine
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• v.24 no.12
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• pp.31-38
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• 2007

본고에서는 현재 3GPP(3rd Generation Partner Project)에서 표준화 작업이 진행중인 LTE(Long Term Evolution) 시스템에서, Layer 2와 Layer 3에 해당되는 무선프로토콜 기술에 대해서 알아본다.

• The Bulletin of The Korean Astronomical Society
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• v.39 no.2
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• pp.67.2-67.2
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• 2014

The presence of multiple populations is now well-established in most globular clusters in the Milky Way. In light of this progress, here we suggest a new model explaining the origin of the Sandage period-shift and the difference in mean period of type ab RR Lyrae variables between the two Oosterhoff groups. In our models, the instability strip in the metal-poor group II clusters, such as M15, is populated by second generation stars (G2) with enhanced helium and CNO abundances, while the RR Lyraes in the relatively metal-rich group I clusters like M3 are mostly produced by first generation stars (G1) without these enhancements. This population shift within the instability strip with metallicity can create the observed period-shift between the two groups, since both helium and CNO abundances play a role in increasing the period of RR Lyrae variables. The presence of more metal-rich clusters having Oosterhoff-intermediate characteristics, such as NGC 1851, as well as of most metal-rich clusters having RR Lyraes with longest periods (group III) can also be reproduced, as more helium-rich third and later generations of stars (G3) penetrate into the instability strip with further increase in metallicity. Therefore, although there are systems where the suggested population shift cannot be a viable explanation, for the most general cases, our models predict that the RR Lyraes are produced mostly by G1, G2, and G3, respectively, for the Oosterhoff groups I, II, and III.

• TTA Journal
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• s.100
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• pp.51-57
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• 2005

차세대 이동통신 표준화는 크게 네가지 분야에서 진행되고 있다. 3GPP, 3GPP2에서의 3G Evolution, IEEE 802.16에서의 Broadband Wireless Access, OMA에서의 응용서비스의 표준화, 그리고 ITU-R에서의 Spectrum 및 Beyond 3G 비전 연구 등이다. 본 고에서는 현 시점에서 각 기구에서 진행되고 있는 표준활동의 개요를 간단히 소개한다.

• Korean Journal of Soil Science and Fertilizer
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• v.27 no.4
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• pp.290-295
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• 1994

Soil $CO_2$ evolution was measured using the soda-lime method for 20-year-old L. tulipifera, P. albaglandulosa, and Q. rubra plantations planted on a similar soil type in the Kwangneung Experimental Forest during the growing season of 1994. Soil $CO_2$ evolution ranged from $0.21g/m^2/hr$ for Q. rubra to $0.33g/m^2/hr$ for L. tulipifera. and was significantly different among species. We found positive correlations between soil $CO_2$ evolution and air(p<0.001, r=0.39) and soil temperatures(p<0.001, r=0.49). Peaks in seasonal soil $CO_2$ evolution occurred in July and August. Seasonal soil $CO_2$evolution did not necessarily follow changes in air and soil temperatures. This study implies that more work is needed to clarify the influence of other factors on soil $CO_2$evolution.