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RCP 시나리오에 근거한 고해상도 미래 풍력 기상자원 분석
임윤정(Yun-Jung Lim),김선애(Seonae Kim),장동호(Dong-Ho Jang),박종철(Jongchul Park),김연희(Yeon-Hee Kim),김백조(Baek-Jo Kim),김맹기(Maeng-Ki Kim) 건국대학교 기후연구소 2016 기후연구 Vol.11 No.1
We developed the Parameter-elevation Regressions on Independent Slopes Model(PRISM)-based Dynamical downscaling Error correction(PRIDE)-Wind speed(WS) model version 3.0 to produce highresolution(1km) grid data at a monthly time scale by using observation and Regional Climate Model(RCM) wind speed data. We consequently produced monthly wind speed grid data during the observation period(2000~2014) and the future period(2021~2100) for Representative Concentration Pathway(RCP) 2 type scenarios by using the PRIDE-WS model. The PRIDE-WS model is constructed by combining the MK(Modified Korean)-PRISM-Wind, the RCM anomaly and Cumulative Density Function(CDF) fitting, basically based on Kim et al.(2016)’s algorithm applied for daily precipitation. The upper level wind(80m altitude) was estimated by Deacon equation using surface wind speed that was produced by the PRIDE-WS model. The results show that the wind speed at the upper level generally increased during the summer season while it decreased during the spring, autumn and winter seasons.
배종철(JongChul Bae),박성승(Sung Seung Park),안윤애(Yun Ae Ahn),류근해(Keun Ho Ryu),주재우(Jae Woo Joo) 한국정보과학회 2000 한국정보과학회 학술발표논문집 Vol.27 No.2Ⅰ
시공간 추론에 관한 연구는 그 역사가 오래되었으며 지난 수 십년 동안 매우 많은 이론적인 연구 결과를 얻었다. 그러나, 이와 관련된 응용분야의 연구는 거의 진척되지 않았기 때문에 시공간 추론의 이론과 응용 사이의 간격을 줄이고 실제 활용 가능한 시스템 개발을 위해서는 관련 이론을 토대로 한 응용 시스템의 개발이 필요하게 되었다. 따라서, 이 논문에서는 그 동안 연구된 시공간 추론의 이론을 특정 응용 분야인 전장분석에 적용하여 전장분석 및 평가에 중요한 영향을 미치는 미상의 부대, 미확인 부대, 주타격 방향을 추론하고, 부대의 이동 위치 및 이동시간을 추정하는 시공간 추론 시스템을 설계 및 구현하였다.
NONTHERMAL BROADENING OF UV LINES OBSERVED AT THE LIMB OF THE QUIET SUN
LEE HVUNSOOK,YUN HONG SIK,CHAE JONGCHUL The Korean Astronomical Society 2000 Journal of The Korean Astronomical Society Vol.33 No.1
We have done a spectroscopic study of the solar transition region using high resolution UV & EUV data obtained by SUMER(Solar Ultraviolet Measurements of Emitted Radiation) on board SOHO(Solar and Heliospheric Observatory). Optically thin and conspicuous emission lines observed at the solar limb are carefully selected to acquire average values of physical parameters for the quiet region as a function of radial distance. Our main results found from the present study can be summarized as follows. 1) Nonthermal velocities estimated from various UV lines do not decrease with height at least within one total line intensity scale height above the limb. 2) Nonthermal velocity distribution with temperature is very similar to that of the disk center, in the sense that its peak is located around $2{\times}10^5 K$, but the value is systematically larger than that of the disk. 3) It is found that nonthermal velocity is inversely proportional. to quadratic root of electron density up to about 10 arc seconds above the limb, i.e. ${\xi}\~N_e^{-1/4}$, implying that the observed nonthermal broadening can be attributed to Alfven waves passing through the medium. 41 Electron density estimated from the O V 629/760 line ratio is found to range from about $1{\times}10^{10}cm^{-3}$ to $2{\times} 10^{12}cm^{-3}$ in the transition region.