• 한국인터넷방송통신학회논문지
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• 제8권3호
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• pp.101-113
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• 2008

사용자 요구의 다양화와 그에 따른 트래픽 증가 등 현재의 IMT-2000 기반에서 수용할 수 없는 보다 복잡한 이동 멀티미디어 환경이 도래하고 있다. 이러한 이동 멀티미디어 서비스를 원활히 제공하기 위해 ITU-R을 중심으로 한 전 세계 이동통신 업계는 이미 4세대용 시스템 규격 및 개발에 상당한 진전을 보이고 있다. 본 논문에서는 4세대 이동통신용 기술기준을 기존의 35세대인 WiBro의 기술기준을 근간으로 하였다. 향후 이동통신의 전송특성은 상/하향의 비대칭적인 통신 트래픽이 예상된다. 따라서 본 논문에서는 상/하향의 점유주파수 대역폭을 1:3과 1:6인 경우를 고려하여 물리계층 파라미터를 제안하였다. 그리고 모의실험을 통해 검증하였다. 따라서 본 논문의 결과를 4세대 이동통신을 위한 기술기준으로 제안한다.

• 대한물리의학회지
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• 제11권2호
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• pp.77-82
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• 2016

PURPOSE: The purpose of this study was to investigate the validity of dynamic balance measurements using a smartphone. METHODS: Thirty subjects were selected out of Y-university students without fractures, operation history, and inflammatory arthritis who had not started regular exercise during the past three months. Their dynamic balance ability was measured by the Biodex Balance System (Biodex Medical Systems, Inc., USA) using smartphones. The smartphone utilized in this study was the Galaxy Note4 LTE (SM-N910K, Samsung, Korea), and the application was the Sensor Kinetics pro (Ver.2.1.2, INNOVENTIONS Inc, US). The dynamic balance ability was measured in triplicate. RESULTS: With eyes closed, a low level of correlation (r>0.30, p<0.05) and low reliability (ICC>0.60) were determined between the roll value of the smartphone gyroscope versus the medial/lateral score of the Biodex Balance System. With eyes closed, a low level of correlation (r>0.30, p<0.05) and low reliability (ICC>0.60) were determined between the total value of the smartphone gyroscope versus the total score of the Biodex Balance System. CONCLUSION: This study indicated that using a smartphone can generate highly limited data regarding balance ability. They are unlikely to replace the existing more expensive devices entirely. However, smartphones may be highly useful in environments in which an expensive device is not available or when dynamic balance ability should be measured immediately or within a few hours.

• 천문학회지
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• 제24권1호
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• pp.71-94
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• 1991

With the 14 m radio telescope at DRAO and the 4 m at Nagoya University, we have made detailed maps of $^{12}CO$ and $^{13}CO$ emissions from two Barnard objects B133 and B134 in the $J=1{\rightarrow}O$ rotational transition lines. Usual LTE analyses of the CO observations led us to determine the distribution of column densities over an entire area encompassing both globules. Total gas masses estimated from the column density map are $90\;M_{\odot}$ and $20\;M_{\odot}$ for B133 and B134, respectively. The radial velocity of B133 is red shifted with respect to B134 by $0.8\;km\;s^{-1}$, which is too lagre to bind the two clouds as a binary system. We have shown that the usual stability analysis based on the simplified version of virial theorem with the second time-derivative of the moment of inertia term $\ddot{I}$ being ignored could mislead us in determining whether a given cloud eventually collapses or not. The lull version of the scalar virial theorem with the $\ddot{I}$ term is shown to be useful in following up the time-dependent variations of the cloud size R and its streaming velocity $\dot{R}$ as functions of time. Results of our stability analysis suggest that B133 will eventually collapse in $(2{\sim}4){\times}10^6$ years.

• 전기학회논문지
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• 제66권3호
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• pp.533-539
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• 2017

ERTMS/ETCS Level 2 is currently planning, making contract, constructing and operating at several lines in European well-developed railway countries different from past ten years ago, and applying extensively for purpose of its intercompatibility and operational efficiency, and economic feasibility. On the other hand, ATP system correspond to ETCS Level 1, which was domestically introduced in early 2000, has introduced, operated, and planned or constructed in national railwaynetwork, but the lines, which its improvement period is come, are being occurred starting Gyeongbu Line. Therefore, we study the consideration and construction plan by stages if LTE-R Korean Radio-based Train Control System for conventional & high-speed railway under domestic development is extensively applied as the third National Railway Network Construction Plan was announced.

• Journal of the Korean Wood Science and Technology
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• 제39권2호
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• pp.163-171
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• 2011

Because Japanese cedar shows lower mechanical performance, glued-laminated timber (glulam) can be a better way to utilize Japanese cedar for structural purpose. However, low yield of higher grade lamination from log makes it difficult to design structural glulam. This study was aimed to increase the yield of higher grade lamination and provide higher efficiency of manufacturing structural lamination by ultrasonic log sorting technology. Logs were sorted by an existing log grading rule regulated by Korea Forest Research Institute (KFRI). It was found that the KFRI log grading rule contributed to finding better logs in viewpoint of the volumetric yield and it can reduce the number of rejected lumber by visual grading. However, it could not identify better logs to produce higher-grade products. To find an appropriate log-sorting-method for structural products, log diameter and ultrasonic time of flight (TOF) for the log were considered as factors to affect mechanical performance of resulting products. However, it was found that influence of log diameter on mechanical performance of resulting products was very small. The TOF showed a possibility to sort logs by mechanical performance of resulting products even though a coefficient of correlation was not strong (R = 0.6). In a case study, the log selection based on the ultrasonic TOF of the log increased the yield of the outermost tension lamination (E8 or better grade, KS F 3021) from 2.6% to 12.5% and reduced LTE5 (lower than E5 grade) lamination from 43.6% to 10.3%, compared with the existing KFRI log grading rule.

• 천문학회보
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• 제36권2호
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• pp.152.1-152.1
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• 2011

We report preliminary results of long-slit near-infrared (NIR) spectroscopy of Luminous Blue Variables (LBVs) with moderate resolution of R ~ 2400. We obtained Jshort (1.04-1.26 micron) and Ks (2.02-2.31 micron) band spectra of 4 LBVs and 3 LBV candidates in Southern hemisphere using IRIS2, infrared imager and spectrograph, mounted on the 4-m Anglo-Australian Telescope. All targets are fairly bright in NIR so that we can obtain high signal-to-noise ratio for clear line detection and modeling. They are also widely distributed in the HR diagram so that we can compare the spectral properties of LBVs in different temperature and luminosity ranges. Among them, we present the results of two well-known LBVs AG Car and HR Car. Their spectra show similar properties with hydrogen, He I, and metallic lines such as Fe II and Mg II, most of them in emission. We discuss, in particular, the He I 1.083 micron lines formed in stellar wind because these two LBVs show large variation in their He I line intensities, compared to previous studies. Since the He I 1.083 line is known to be anticorrelated with the photometric variation of LBVs, strong line intensities with P-Cygni profiles in both stars indicate that they are now near the visual minimum phase. We model the obtained spectra using non-LTE atmosphere code CMFGEN of Hillier (1998) to derive stellar parameters such as wind velocity and mass loss rate, and discuss the long-term variability of stellar parameters of these LBVs. deduced from our otometric solution.

• 한국철도학회논문집
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• 제16권6호
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• pp.510-518
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• 2013

현재 국내외적으로 차세대 철도 무선망에 대한 관심이 높아지고 있으며, 지금까지 열차제어신호 중심의 철도무선망에서 영상 및 대용량 데이터를 전송하기 위한 철도통합 무선망에 대한 연구가 진행 중이다. 본 논문에서는 철도통합 무선망 구축을 위한 무선통신방식과 우리나라에서 사용하고 있는 주파수대역에서 철도 전용주파수 대역으로 할당이 가능한 후보 주파수대역을 제안한다. 본 연구내용은 국내 철도의 열차 운행효율 향상은 물론 철도의 안전성과 편의성 최적화에 기여할 것이며, 세계 기술시장 변화에 대응하는 무선통신기반의 한국형 철도 통합무선망 구축을 실현 할 수 있을 것으로 예상된다.

• 한국작물학회지
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• 제42권6호
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• pp.766-777
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• 1997

수도 저하발아성에 대한 유전 양상을 구명하여 저온발아성 품종 육성의 기초 자료를 얻고자 숙기가 다른 세 그룹에서 10품종을 선정 '94년에 15일 간격 4시기로 파종 및 이앙을 실시하여 수량한 종자를 '95년 4~5월에 13$^{\circ}C$ 항온 실내 시험과, 건답 직파의 포장 시험으로 저온발아성을 조사하고, 저온발아성 고 1품종, 저 1품종, 중 4품종을 선정 '94 하계에 절영법에 의한 정역이면교잡을 실시하여 얻어진 F$_1$ 교배입을 '95년 5월에 13$^{\circ}C$ 항온에서 저온발아 시험을 실시하여 얻은 결과를 요약하면 다음과 같다. 1. 재배 시기를 달리하여 수량된 종자의 실내 및 포장에서의 저온발아성 분산분석 결과 품종에 따라 재배시기간에 고도의 유의차가 인정되었다. 2. 실내 13$^{\circ}C$ 항온 저온발아계수와 포장의 자연상태 건답직파에서의 출아계수와의 상관분석 결과 고도의 유의한 상관(r=0.5111)이 인정되었다. 3. 조합능력 분석 결과 일반조합능력 및 특정조합능력 모두 고도의 유의성이 인정되었으며, 일반조합능력이 특정조합능력보다 커서 상가적작용이 상위성 작용보다 더 크게 나타났다. 4. 정역차이 분산분석 결과 정역간에 고도의 유의차가 인정되었다. 5. 부친열 공분산/모친열 공분산 Graph에서 6개의 교배열 모두가 모본 효과를 보였으며, Alpha와 Beta 유전 분석 결과, 저온발아성의 정역간 차이는 Alpha 유전의 효과로 나타났다. 6. 평균우성도 분석 결과, 30개 조합 중 17개 조합에서 초월분리를 보였으며, 그 중 9개 조합이 저온발아성이 낮은 쪽으로 초월분리를 보였다.

• 천문학회지
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• 제24권2호
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• pp.217-271
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• 1991

We have observed dense core around young stellar objects, DR21, S140, Orion-KL, and L1551 using four millimeter-wave transitions of $HC_3N\;J$=4-3, J=5-4, J=10-9, and J=12-11. The spatial distribution of $HC_3N$ emission closely resembles the morphology of the previous CS observations that trace high density gas. These observations reveal the existence of $HC_3N$ dense cores around central IR source, elliptical in shape and almost perpendicular to the CO bipolar outflow axis. Small differences can be explained by that $HC_3N$ molecular line is more optically thin and is seen to be more detailed structure in the neighborhood of central IR sources. In S140 and Orion-KL, massive(${\sim}10\;M_{\odot}$), slowly rotating dense cores lie near at the central IR sources of bipolar outflows. The velocity channel maps of DR21 show that the bipolar outflow gas may have a correlation with the dense core of DR21. We analyzed intensities of the four lines to derive physical conditions in dense core from two methods, LTE and LVG. The column density of $HC_3N$, $N(HC_3N)$, between LTE and LVG calculations agree well with each other. The abundances of $HC_3N$ in each observing source have been estimated using the average values of $n(H_2)$ and $N(HC_3N)$ and assuming the size of dense core. The fractional $HC_3N$ abundances in massive dense cores of DR21, S140, and Orion-KL have a range of $(2-7){\times}10^{-10}$, while that of low mass dense core, L1551, has one order of magnitude greater value of $2{\times}10^{-9}$. This should be considered good agreement with the result by Morris et al.(1976). It may be considered that dense cores of DR21, S140, and Orion-KL may have almost same stage of chemical evolution, and their abundances have a small values relative to that of L1551. The column density $N(HC_3N)$ decreases with increasing distance from the densest part of the cloud, the central infrared source, and have the relation of $N(HC_3N){\varpropto}R^{\alpha}$, where a has a range of 0.65 to 0.89. The values of $n(H_2)$ are not varied with increasing distance from the dense core, and have almost same values. Therefore, it is considered that the dense cores in these regions probably consist of dense clumps in diffuse molecular gas medium, and $n(H_2)$ of each clump is ${\sim}10^5\;cm^{-3}$. Levels in the $T_{ex}$ increases with $n(H_2)$. It is considered that the $HC_3N$ dense cores are not completely thermalized. We examine the relationships between the luminosity of central infrared sources versus mass of the dense cores, and the luminosity of central infrared sources versus molecular hydrogen column density. Luminosities of the central IR sources show good correlation with mass and hydrogen column density of the dense core. Same has been found from CS observations. However, mass and size derived from $HC_3N$ observations are one order of magnitude smaller than those from CS. It can be interpreted that we see more central part of the cloud cores in $NC_3N$ lines than CS lines.