본 연구는 한국 갯기름나물의 지형적 분포와 해식애 군집구조의 기초자료로 제공하기 위하여 해안과 지형별 종조성 및 생육양상을 조사한 바 이의 결과를 요약하면 다음과 같다. 갯기름나물과 동반 출현하는 식물은 57과 130속에 속한 170 분류군이었으며, 과별로는 국화과가 30 분류군으로 가장 많았다. 출현빈도가 가장 높은 식물은 해국(54.1%)이었고, 해안별로는 동해안과 서해안에서 해국, 남해안에서 억새의 출현빈도가 가장 높았다. 해안별 공통종은 서해안과 남해안간이 35.6%(47 분류군)로서 가장 높았고 다음으로 동해안과 서해안(30.4%), 동해안과 남해안(26.4%)순이었다. 갯기름나물이 출현하는 해안지형은 경사도 17.4˚의 해식애 암석해안, 평탄면, 암괴원, 수평절리, 수직절리, 요철지형이었고 지형 별 분포지역은 암석해안이 61 지역으로 가장 많았다. 군도에 따른 갯기름나물의 생육양상은 군도계급 3이 83지역(54.6%)으로서 가장 많았다.

Biological control of Liriomyza trifolii (Burgess) using Diglyphus isaea (Walker) has been evaluated in tomato greenhouse, for three seasonal culture types: spring type (March-July), summer type (June-October) and autumn type (July-December). For spring type, totally 5.8 individuals/㎡ of D. isaea has been released at six times from late April, when the density of L. trifolii was about 1.0 individuals/plant. Corrected mortality of Liriomyza trifolii caused by parasitoids was 97.6% at early July, and the proportion of D. isaea was 88.9% of all parasitoids collected in the greenhouse. In the case of summer type, totally 1.8 individuals/㎡ of D. isaea has been released at five times from early July, when the density of L. trifolii was about 0.4 individuals/plant. Corrected mortality of L. trifolii caused by parasitoids was 84.4% during the whole season, but the proportion of D. isaea was very low (only 13.8%). Immigrating parasitoids such as Chrysocharis penthus were synchronized to control the leafminer in the greenhouse. For autumn type, totally 2.7 individuals/㎡ of D. isaea has been released at four times from mid September, when the density of L. trifolii was about 0.7 individuals/plant. Corrected mortality of L. trifolii caused by parasitoids was 85.7% at mid December, and the proportion of the D. isaea was 83.4%.

본 연구는 우리나라 RCC/RSC의 효율성을 2개의 투입자료와 4개의 산출자료를 이용하여 DEA법을 이용하여 측정하였고, 정성적 자료는 전문가의 설문 및 면접결과로 평가하였다. 또한, 이러한 자료를 통합하기 위한 방법은 의사결정지원시스템인 퍼지로직을 적용하였고, 이 평가방법을 이용하여 RCC/RSC의 운영효율성의 우선순위를 평가하였다. 그 결과 목포, 제주, 부산, 통영, 인천, 여수, 동해, 울산, 포항, 속초, 태안, 완도, 군산RSC 순으로 효율성이 높은 것으로 나타났다.

We report a high resolution spectrum of AG Pegasi observed at Bohyunsan Optical Astronomy Observatory (BOAO) on October 2, 2004. Some of permitted emission lines, for example H I, He I, He II, Fe II and Ti II were observed in the spectrum of AG Pegasi in 2004. Lines presented in the longer wavelength region than 6500＼AA are identified. And radial velocities for each element are measured. Then we carefully discuss the geometrical feature of AG Pegasi in October 2004.

Electromagnetic fields of all frequencies represent one of the most common and fastest growing environmental influences, about which anxiety and speculation are spreading. All populations are now exposed to varying degrees of electromagnetic field, and the levels will continue to increase as technology advances. The objectives of this study were to measure and analyze emitting characteristics of extremely low frequency electromagnetic field at micro-environments. We measured magnetic field at microenvironments such as home, school, educational institute, internet pc game room for children attending the primary school. The range of time weighted average (TWA) of 60 Hz EMF in micro-environment were 0.26∼ 7.62 mG and the highest TWA 7.62 mG was measured in PC room possessed more than 50 computers. We will measure personal exposure levels of primary students and analyze correlation between major micro-environments and personal exposure level.

We have reviewed the magnetic activity in close binaries. Solar like magnetic activity indicators such as photometric spots, chromo spheric emission, coronal X-ray and radio emission, and flare activity are commonplace in many cool stars with convective envelopes. Using the UV spectra we confirmed the strength of stellar activity increases with more rapid rotation and later spectral types which corresponds to the increasing depth of the star's convective envelope. Apart from very young stellar objects such as T Tauri stars, the stars with the highest levels of activity are close binary systems composed of cool stars, i.e., the chromospherically active binaries such as RS CVn, BY Dra, W UMa and related systems. The IUE low and high dispersion spectra of V711 Tau, VW Cep and SW Lac are used for ultraviolet photometry and for a variation study of chromospheric activity. Evidence of chromospherically activity is indicated by the intensity variation of the Mg II emission line with orbital phase.

본 연구의 목적은 냉연공장 폐수재이용을 위해 3단 역삼투시스템 사용시 각단에서의 투과특성을 조사하는 것이다 판틀형 모듈 7개를 사용하여 회수율이 75% 가 되도록 3단 (배열 : 4+2+1) 으로 구성하여 장기간에 걸친 pilot test를 통해 막오염 진행에 따른 각 단에서의 유량 및 수질변화를 조사하였다 실험결과 각 단 모듈 1개당 평균 투과수량은 운전초기에는 1단, 2단, 3단의 순서로 많았으나 운전시간이 경과하며 막오염이 진행됨에 따라 1단은 감소하는 반면 2단은 거의 변화가 없고 3단의 투과수량은 증가하였다 즉 막오염은 주로 1단에서 발생하며 점차 2단. 3단으로 진행되는 것을 확인할수 있었다. 한편 투과수 수질은 예상한 것과 같이 1단이 가장 우수하였고 다음으로는 2단, 3단의 순서였으며 막오염에 영향을 받지않았다.