• 제목/요약/키워드: Korean -i/ka

검색결과 168건 처리시간 0.027초

제주도의 지질과 화산활동에 관한 연구 (I): 동부지역 저지대 시추코어 화산암류의 암석화학 및 $^{40}Ar/^{39}Ar$ 절대연대 (The Study on Geology and Volcanism in Jeju Island (I): Petrochemistry and $^{40}Ar/^{39}Ar$ Absolute ages of the Subsurface Volcanic Rock Cores from Boreholes in the Eastern Lowland of Jeiu Island)

  • 고기원;박준범;박윤석
    • 자원환경지질
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    • 제41권1호
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    • pp.93-113
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    • 2008
  • 제주도 동부 저지대 (해발 200m 이내), 한동-종달-우도-수산-삼달-하천 지역의 20개 시추공에서 얻어진 화산암류의 암석학적 특징과 $^{40}Ar/^{39}Ar$절대연대를 보고하고, 이에 근거하여 이 지역의 지형형성과 화산활동에 대해 고찰한다. 이 지역의 지하에 분포하는 화산암류는 주로 현무암류(알칼리 현무암, 전이질 현무암, 솔리아이트질 현무암)와 솔리아이트질 안산암 및 현무암질 조면안산암으로 구성된다. 솔리아이트질, 전이질 및 알칼리암류가 서로 호층을 이루어 분포하는 것은 이 지역에서 이들 화산활동이 동시에 일어났었음을 지시한다. 특히, 조면현무암 혹은 현무암질 안산암이 이 지역의 기저부에 분포하는 점은 비교적 분화된 알칼리 화산활동이 먼저 시작되었음을 의미한다. 이 지역에 분포하는 화산암류의 $^{40}Ar/^{39}Ar$ 절대연대는 최고 $526{\pm}23Ka$에서 최저 $38{\pm}4Ka$이다. 동부 지역 저지대에서 용암류의 분출과 같은 하와이형 화산활동은 퇴적층의 관계, 화산암류의 전암 화학성분 및 $^{40}Ar/^{39}Ar$ 절대연대의 변화로 부터 다섯 단계로 구분된다. 즉, 서귀포층이 퇴적할 동안의, I-U기$(550{\sim}400Ka)$, II기$(400{\sim}300Ka)$, III기$(300{\sim}200Ka)$와 퇴적 이후 IV기$(200{\sim}100Ka)$, V기(100Ka이후)이다. 화산암류의 성분 변화 및 분포 지역의 차이 그리고 이들 시기 간에 분포하는 다양한 퇴적층(수성화산기원퇴적층 포함)의 존재는 화산활동이 오랜 기간 동안 간헐적으로 진행되었으며, 저지대의 육지지형이 화산활동 및 퇴적작용에 의해 내륙에서 해안으로 점진적으로 확대되면서 만들어졌음을 지시한다. 특히 시추코어 화산암의 $^{40}Ar/^{39}Ar$ 절대연대 자료는 제주도 동부 저지대 지역 대부분이 IV와 V 화산활동기 동안 분출된 200Ka 이내의 비교적 젊은 화산암류로 이루어져 있음을 지시한다. 이는 제주도 화산활동 시기 및 지형 형성에 대한 기존의 연구와는 상이한 결과이며, 화산암류의 K-Ar절대연대 자료를 바탕으로 한 기존의 제주도 화산활동 시기 구분이 재고되어야함을 확인하였다. 또한, 시추공에 근거한 화산 층서의 해석은 암석기재, 암석화학적 특징과 함께 절대연대 자료를 바탕으로 이루어져야 함을 강조한다.

골다공증성 흉요추부 압박 골절에서의 보존적 치료 (Conservative treatment of Osteoporotic Compression Fractures in Thoracolumbar spine)

  • 강규복;고영도
    • Journal of Trauma and Injury
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    • 제18권2호
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    • pp.107-111
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    • 2005
  • Backgrounds: To evaluate the effectiveness of conservative treatment in osteoporotic thoraco-lumbar compression fractures and to identify the factors influencing the progression of compression. Materials and Methods: From January 2003 to October 2004, Patients who were admitted to our hospital for osteoporotic thoraco-lumbar compression fractures were reviewed retrospectively with follow-up more than 12 months (ave. 14.6 months). With simple x-ray lateral view, we evaluate wedge compression ratio (WCR) and kyphotic angle (KA) at initial and final follow-up. We separate the patients into two groups baesed on the amount of progression of vertebral compression and evaluate a relation with BMD, vertebral fracture level, initial WCR, initial KA. All datas were statistically analyzed. Results: An average of T-score was -3.5 and the changes of KA between initial and final follow-up were average $3.5^{\circ}$. Compression of anterior column were progressed to 8.5%. The changes between initial and final WCR in Group I (N=24) was 17.8%, and Group II (N=18) was 3.3%. T-score in group I was -3.4 and group II was -3.8 (p=0.228). vertebral fracture level were 10 T12, 12 L1, 2 L2 in group I; 6 T12, 6 L1, 6 L2 in group II (p=0.156). Initail WCR was 0.74 in group I, 0.63 in group II, and there was statistical difference between two groups(p=0002). Initial kyphotic angle was $13.9^{\circ}$in group I, $16.2^{\circ}$in group II repectively (p=0.392). Conclusion: The conservative treatment with short-term bed rest and early embulation is effective and valuable method to patients who have osteoporotic thoraco-lumbar compression fractures. There was no statistical difference between two groups according to BMD, vertebral fracture level, KA. But in comparison with initail WCR between two groups, there was statistical difference. That means, in the case of small initial compression of anterior column, the progression of compression was bigger than else. In these patients, more strict use of appropriate brace and careful follow-up should be needed.

Ka-Band 위성중계기용 수신하향변환기 모듈 개발 (Development of a Receiver Downconverter Module for Ka-band Satellite Payload)

  • 장동필;염인복;이성팔
    • 한국전자파학회논문지
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    • 제14권1호
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    • pp.68-74
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    • 2003
  • 본 논문에서는 Ka-band 위성중계기에 사용되어지는 수신하향변환기(Receiver-Downconverter) 모듈의 설계 및 제작 그리고 시험 결과에 대하여 기술하였다. 개발된 수신하향변환기는 30.6 GHz∼31 GHz대역의 신호를 입력으로 받아들여 20.8 GHz∼21.2 GHz 대역의 신호를 출력하는 일종의 Downconverter 이지만, 모듈의 입력단에 저잡음 증폭부가 포함된 수신기의 역할도 하고 있다 개발된 모듈은 제작과정 및 시험과정에 있어 위성중계기 부품 제작 규정을 준수하였으며, 그 개발된 성능은 현재까지 알려진 국내외 유사 부품중의 최고의 성능을 보여주고 있다. 측정된 모듈의 성능은 상온에서 1.9 dB의 잡음지수, 55 dB 이득, 58 dBc의 C/I3 값을 보여주고 있다. 제작된 모듈의 크기는 93 mm${\times}$84 mm${\times}$26 mm이며 무게는 240 g으로서 국내외 유사 제품에 비해 소형이다.

Curcumin Attenuates Gliall Cell Activation But Cannot Suppress Hippocampal CA3 Neuronal Cell Death in i.c.v. Kanic Acid Injection Model

  • Cho, Jae-Young;Kong, Pil-Jae;Chun, Wan-Joo;Moon, Yeo-Ok;Park, Yee-Tae;Lim, So-Young;Kim, Sung-Soo
    • The Korean Journal of Physiology and Pharmacology
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    • 제7권6호
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    • pp.307-310
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    • 2003
  • Kainic acid (KA) is a structural analogue of glutamate that interacts with specific presynaptic and postsynaptic receptors to potentiate the release and excitatory actions of glutamate. Systemic or intracerebroventricular (i.c.v.) administration of KA to experimental animals elicits multifocal seizures with a predominantly limbic localization, and results in neuronal death of cornu ammonia 1 (CA1), reactive gliosis and biochemical changes in the hippocampus and other limbic structures. Several lines of evidence suggest that reactive oxygen species (ROS) play a pivotal role in the pathogenesis of excitotoxic death by KA. Curcumin has been known to possess anti-oxidative and anti-inflammatory activities. In this study, the effects of curcumin on KA induced hippocampal cell death, reactive gliosis and biochemical changes in reactive glia were investigated by immunohistochemical methods. Our data demonstrated that curcumin attenuated KA-induced astroglial and microglial activation although it did not protect KA-induced hippocampal cell death.

Inhibition of HBV replication and gene expression in vitro and in vivo with a single AAV vector delivering two shRNA molecules

  • Li, Zhi;He, Ming-Liang;Yao, Hong;Dong, Qing-Ming;Chen, Yang-Chao;Chan, Chu-Yan;Zheng, Bo-Jian;Yuen, Kwok-Yung;Peng, Ying;Sun, Qiang;Yang, Xiao;Lin, Marie C.;Sung, Joseph J.Y.;Kung, Hsiang-Fu
    • BMB Reports
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    • 제42권1호
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    • pp.59-64
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    • 2009
  • Hepatitis B virus (HBV) infection is highly prevalent worldwide. The major challenge for current antiviral treatment is the elevated drug resistance that occurs via rapid viral mutagenesis. In this study, we developed AAV vectors to simultaneously deliver two or three shRNAs targeting different HBV-related genes. These vectors showed markedly better antiviral effects than ones that delivered a single shRNA in vitro. A dual shRNA expression vector (AAV-157i/1694i), which simultaneously expressed two shRNAs targeted the S and X genes of HBV, reduced HBsAg, HBeAg and HBV DNA levels by $87{\pm}4$, $80.3{\pm}2.6$ and $86.2{\pm}7%$ respectively, eight days post-transduction. In a mouse model of prophylactic treatment, HBsAg and HBeAg were reduced to undetectable levels and the serum HBV DNA level was reduced by at least 100 fold. These results indicate that AAV-157i/1694i generates potent anti-HBV effects and that the strategy of constructing multi-shRNA expression vectors may lead to enhanced anti-HBV efficacy and overcome the evading mechanism of the virus and thus the development of drug resistance.

Observational Studies on Evolved Stars Using KVN and KaVA/EAVN

  • Cho, Se-Hyung;Yun, Youngjoo;Imai, Hiroshi
    • 천문학회보
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    • 제44권2호
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    • pp.51.1-51.1
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    • 2019
  • At the commissioning phase of KVN from 2009 to 2013, single-dish survey and monitoring observations were performed toward about 1000 evolved stars and about 60 relatively strong SiO and H2O maser sources respectively. Based on these single-dish results and VLBI feasibility test observations at K/Q/W/D bands in 2014, KVN Key Science Project (KSP) has started from 2015 and will be completed in 2019 as KSP phase I. Here we present the overview of observational studies on evolved stars using KVN. In KSP phase I, we have focused on nine KSP sources which show a successful astrometrically registered maps of SiO and H2O masers using the source frequency phase referencing method. We aim at investigating the spatial structure and dynamical effect from 43/42/86/129 GHz SiO to 22 GHz H2O maser regions associated with a stellar pulsation and development of asymmetry in circumstellar envelopes. Using the combined network KaVA (KVN+Japanese VLBI network VERA), KaVA Large Program titled on "Expanded Study on Stellar Masers: ESTEMA Phase I" was performed from 2015 to 2016. Based on ESTEMA Phase I, EAVN Large Program titled on "EAVN Synthesis of Stellar Maser Animations: ESTEMA Phase II" was also performed from 2018. The ESTEMA II project aims to publish composite animations of circumstellar H2O and SiO masers, which taken from up to 6 long-period variable stars with a variety of the pulsation periods (333-1000 days). The animations will exhibit the three-dimensional kinematics of the maser gas clumps with complexity caused by stellar pulsation-driven shock waves and anisotropy of clump ejections from the stellar surface. Adding three EAVN telescopes (Tianma 65m, Nanshan 26m and NRO 45m telescopes) with KaVA always secures the high quality of the maser image frames through the monitoring program.

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대한해협 대륙붕 해역의 홀로세 해수면 상승과 고환경변화 (Holocene sea-level rise and paleoenvironmental changes in Korea Strait shelf)

  • 남승일;장정해;공기수;김성필;유동근
    • 한국제4기학회지
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    • 제17권1호
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    • pp.7-16
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    • 2003
  • 대한해협 북서연안의 내대륙붕(약 40m수심)에서 약 31m의 심부 코아 SSDP-102를 시추하여, 고해상의 층서를 확립하고 홀로세 해침에 의한 고환경 변화를 복원하기 위하여 퇴적상과 유기지화학 분석을 수행하였다. 시추 코아의 층서는 6점의 AMS $^{14}C$ 연대측정 자료를 이용하였으며, 약 12.1 ka BP 이후의 퇴적환경 변화가 기록되어 있다. 탄성파 탐사자료와 퇴적물 암상 그리고 유기지화학 자료에 의하면 코아 SSDP-102는 음향 기반암 위에 쌓인 3개의 퇴적 단위 (Unit III, II, I)로 나뉘어 지며, 각 Uni에는 해침이 시작된 이후 3회에 걸쳐 뚜렷한 퇴적환경변화가 기록되어 있다. (1) Unit III은 12.1에서 6.2 ka BP까지 해침이 시작된 염하구 환경: (2) Unit II는 6.2에서 5.1 ka BP까지 해수면 상승이 둔화된 연안환경: (3) Unit 1은 5.1 ka BP 이후 현재까지 연안 및 외해 환경에서 퇴적되었다. 특히 대마난류의 영향을 받는 현재의 퇴적환경은 약 5.1 ka BP 이후 점진적으로 형성된 것으로 보인다.

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토양수분함량 예측 및 계획관개 모의 모형 개발에 관한 연구(I) (A Study on the Development of a Simulation Model for Predicting Soil Moisture Content and Scheduling Irrigation)

  • 김철회;고재군
    • 한국농공학회지
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    • 제19권1호
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    • pp.4279-4295
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    • 1977
  • Two types of model were established in order to product the soil moisture content by which information on irrigation could be obtained. Model-I was to represent the soil moisture depletion and was established based on the concept of water balance in a given soil profile. Model-II was a mathematical model derived from the analysis of soil moisture variation curves which were drawn from the observed data. In establishing the Model-I, the method and procedure to estimate parameters for the determination of the variables such as evapotranspirations, effective rainfalls, and drainage amounts were discussed. Empirical equations representing soil moisture variation curves were derived from the observed data as the Model-II. The procedure for forecasting timing and amounts of irrigation under the given soil moisture content was discussed. The established models were checked by comparing the observed data with those predicted by the model. Obtained results are summarized as follows: 1. As a water balance model of a given soil profile, the soil moisture depletion D, could be represented as the equation(2). 2. Among the various empirical formulae for potential evapotranspiration (Etp), Penman's formula was best fit to the data observed with the evaporation pans and tanks in Suweon area. High degree of positive correlation between Penman's predicted data and observed data with a large evaporation pan was confirmed. and the regression enquation was Y=0.7436X+17.2918, where Y represents evaporation rate from large evaporation pan, in mm/10days, and X represents potential evapotranspiration rate estimated by use of Penman's formula. 3. Evapotranspiration, Et, could be estimated from the potential evapotranspiration, Etp, by introducing the consumptive use coefficient, Kc, which was repre sensed by the following relationship: Kc=Kco$.$Ka+Ks‥‥‥(Eq. 6) where Kco : crop coefficient Ka : coefficient depending on the soil moisture content Ks : correction coefficient a. Crop coefficient. Kco. Crop coefficients of barley, bean, and wheat for each growth stage were found to be dependent on the crop. b. Coefficient depending on the soil moisture content, Ka. The values of Ka for clay loam, sandy loam, and loamy sand revealed a similar tendency to those of Pierce type. c. Correction coefficent, Ks. Following relationships were established to estimate Ks values: Ks=Kc-Kco$.$Ka, where Ks=0 if Kc,=Kco$.$K0$\geq$1.0, otherwise Ks=1-Kco$.$Ka 4. Effective rainfall, Re, was estimated by using following relationships : Re=D, if R-D$\geq$0, otherwise, Re=R 5. The difference between rainfall, R, and the soil moisture depletion D, was taken as drainage amount, Wd. {{{{D= SUM from { {i }=1} to n (Et-Re-I+Wd)}}}} if Wd=0, otherwise, {{{{D= SUM from { {i }=tf} to n (Et-Re-I+Wd)}}}} where tf=2∼3 days. 6. The curves and their corresponding empirical equations for the variation of soil moisture depending on the soil types, soil depths are shown on Fig. 8 (a,b.c,d). The general mathematical model on soil moisture variation depending on seasons, weather, and soil types were as follow: {{{{SMC= SUM ( { C}_{i }Exp( { - lambda }_{i } { t}_{i } )+ { Re}_{i } - { Excess}_{i } )}}}} where SMC : soil moisture content C : constant depending on an initial soil moisture content $\lambda$ : constant depending on season t : time Re : effective rainfall Excess : drainage and excess soil moisture other than drainage. The values of $\lambda$ are shown on Table 1. 7. The timing and amount of irrigation could be predicted by the equation (9-a) and (9-b,c), respectively. 8. Under the given conditions, the model for scheduling irrigation was completed. Fig. 9 show computer flow charts of the model. a. To estimate a potential evapotranspiration, Penman's equation was used if a complete observed meteorological data were available, and Jensen-Haise's equation was used if a forecasted meteorological data were available, However none of the observed or forecasted data were available, the equation (15) was used. b. As an input time data, a crop carlender was used, which was made based on the time when the growth stage of the crop shows it's maximum effective leaf coverage. 9. For the purpose of validation of the models, observed data of soil moiture content under various conditions from May, 1975 to July, 1975 were compared to the data predicted by Model-I and Model-II. Model-I shows the relative error of 4.6 to 14.3 percent which is an acceptable range of error in view of engineering purpose. Model-II shows 3 to 16.7 percent of relative error which is a little larger than the one from the Model-I. 10. Comparing two models, the followings are concluded: Model-I established on the theoretical background can predict with a satisfiable reliability far practical use provided that forecasted meteorological data are available. On the other hand, Model-II was superior to Model-I in it's simplicity, but it needs long period and wide scope of observed data to predict acceptable soil moisture content. Further studies are needed on the Model-II to make it acceptable in practical use.

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KEY SCIENCE OBSERVATIONS OF AGNs WITH THE KaVA ARRAY

  • KINO, MOTOKI;NIINUMA, KOTARO;ZHAO, GUANG-YAO;SOHN, BONG WON
    • 천문학논총
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    • 제30권2호
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    • pp.633-636
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    • 2015
  • KaVA (KVN and VERA Array) is a new combined VLBI array composed of KVN (Korean VLBI Network) and VERA (VLBI Exploration of Radio Astrometry). Here, we report the following two issues. (1) We review the initial results of imaging observations of M87 at 23 GHz following Niinuma et al. (2014). The KaVA images reveal extended outflows including complex substructures such as knots and limb-brightening, in agreement with previous VLBI observations. KaVA achieves a high dynamic range of ~1000, more than three times better than that achieved by VERA alone. (2) Based on subsequent observations and discussions led by the KaVA AGN SubWorking Group, we set monitoring observations of Sgr $A^{\ast}$ and M87 as our Key Science Project (hereafter KSP) because of the closeness and largeness of their central super-massive black holes. The main science goals of the KSP are (i) testing the magnetically-driven-jet paradigm by mapping velocity fields of the M87 jet, and (ii) obtaining tight constraints on physical properties of the radio emitting region in Sgr $A^{\ast}$. Towards KSP, we show the first preliminary images of M87 at 23 GHz and Sgr $A^{\ast}$ at 43 GHz with the bandwidth of 256 MHz.