Stable Isotope Analysis (SIA) of carbon and nitrogen is useful tool for the understanding functional roles of target organisms in biological interactions in the food web. Recently, mixing model based on SIA is frequently used to determine which of the potential food sources predominantly assimilated by consumers, however, application of model is often limited and difficult for non-expert users of software. In the present study, we suggest easy manual of R software and package SIAR with example data regarding selective feeding of crustaceans dominated freshwater zooplankton community. We collected SIA data from the experimental mesocosms set up at the littoral area of eutrophic Chodae Reservoir, and analyzed the dominant crustacean species main food sources among small sized particulate organic matters (POM, <50 μm), large sized POM (>50 μm), and attached POM using mixing model. From the results obtained by SIAR model, Daphnia galeata and Ostracoda mainly consumed small sized POM while Simocephalus vetulus consumed both small and large sized POM simultaneously. Copepods collected from the reservoir showed no preferences on various food items, but in the mesocosm tanks, main food sources for the copepods was attached POM rather than planktonic preys including rotifers. The results have suggested that their roles as grazers in food web of eutrophicated reservoirs are different, and S. vetulus is more efficient grazer on wide range of food items such as large colony of phytoplankton and cyanobacteria during water bloom period.

We have developed a cylindrical mixing layer model of a stellar jet including cooling effect in order to understand an optical emission mechanism along collimated high velocity stellar jets associated with young stellar objects. The cylindrical results have been calculated to be the same as the 2D ones presented by Canto & Raga(1991) because the entrainment efficiency in our cylindrical model has been obtained to be the same value as the 2D model has given. We have discussed the morphological and physical characteristics of the mixing layers by the cooling effect. As the jet Mach number increases, the initial temperature of the mixing layer goes high because the kinetic energy of the jet partly converts to the thermal energy of the mixing layer. The initial cooling of the mixing layer is very severe, changing its outer boundary radius. A subsequent change becomes adiabatic. The number of the Mach disks in the stellar jet and the total radiative luminosity of the mixing layer, based on our cylindrical calculation, have quite agreed with the observations.

준설 시 발생하는 부유물의 이송 확산 과정을 해석하기 위하여 퍼프모형을 개발하였다. 본 연구에서 개발된 퍼프 모형은 추적방법에 따라 전방추적모형과 후방추적모형으로 나눌 수 있으며, 이 두 가지 추적방법은 계산효율과 수치 오차에 있어서 상이한 특성을 나타내었다. 경계처리에 있어서 입자추적모형과 상이한 방법을 사용하는 퍼프모형은 폐경계에서는 입자추적모형과 동일한 결과를 나타내지만 개경계에서는 다른 결과를 나타내었다. 또한 오염원이 임의의 공간적 분포를 갖는

자연하천에 유입된 오염물질의 확산거동을 해석하기 위하여 통계학적인 개념을 이용하여 오염물질 입자의 운동을 묘사하는 2차원 Random-Walk 모형을 개발하였다. 개발된 모형을 검정한 결과, 고정격자의 개수를 증가시키거나 각각의 고정격자 내에 포함된 입자개수의 평균값을 증가시키면 해의 정밀도가 증가하는 것으로 나타났다. 본 모형의 현장 적용성을 검토하기 위하여 캐나다에 위치한 Grand River에서 수행된 정상상태의 색소실험 결과와 본 모형에 의한 계