• 대한기계학회논문집B
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• 제23권8호
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• pp.945-956
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• 1999

This work reports a set of approximate analytical solutions describing the initial transient process of close-contact melting between a rectangular parallelepiped solid and a flat plate on which either constant temperature or constant heat flux is imposed. Not only relative motion of the solid block tangential to the heating plate, but also the density difference between the solid and liquid phase is incorporated in the model. The thin film approximation reduces the force balance between the solid weight and liquid pressure, and the energy balance at the melting front into a simultaneous ordinary differential equation system. The normalized model equations admit compactly expressed analytical solutions which include the already approved two-dimensional solutions as a subset. In particular, the normalized liquid film thickness is independent of all pertinent parameters, thereby facilitating to define the transition period of close-contact melting. A unique behavior of the solid descending velocity due to the density difference is also resolved by the present solution. A new geometric function which alone represents the three-dimensional effect is introduced, and its properties are clarified. One of the representative results is that heat transfer is at least enhanced at the expense of the increase in friction as the cross-sectional shape deviates from the square under the same contact area.

• 한국분말재료학회지
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• 제21권6호
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• pp.447-453
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• 2014

Effect of oxygen content in the ultrafine tungsten powder fabricated by electrical explosion of wire method on the behvior of spark plasma sintering was investigated. The initial oxygen content of 6.5 wt% of as-fabricated tungsten powder was reduced to 2.3 and 0.7 wt% for the powders which were reduction-treated at $400^{\circ}C$ for 2 hour and at $500^{\circ}C$ for 1h in hydrogen atmosphere, respectively. The reduction-treated tungsten powders were spark-plasma sintered at $1200-1600^{\circ}C$ for 100-3600 sec. with applied pressure of 50 MPa under vacuum of 0.133 Pa. Maximun sindered density of 97% relative density was obtained under the condition of $1600^{\circ}C$ for 1h from the tungsten powder with 0.7 wt% oxygen. Sintering activation energy of $95.85kJ/mol^{-1}$ was obtained, which is remarkably smaller than the reported ones of $380{\sim}460kJ/mol^{-1}$ for pressureless sintering of micron-scale tungsten powders.

• 한국식품조리과학회지
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• 제19권4호
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• pp.439-446
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• 2003

This study was performed to investigate the change in the chemical components of red pepper powder using different packaging materials and various storage conditions. Red pepper powders with 11 and 15% initial moisture content were packed with five different materials and stored at different temperatures (0, 20, and 30 C) for a one year period. Over the storage period, each combination was periodically sampled, and examined for composition changes. The five packaging materials were: linear low density polyethylene(LLDPE), nylon/LLDPE(Ny/LLDPE), saran coated ethylene vinyl acetate copolymer/linear low density polyethylene(B650), nylon/Tie/nylon/ethylene-vinyl alcohol copolymer/nylon/Tie/LLDPE(RDX-2787) and oriented polypropylene/alumimum/LLDPE(OPP/Al/LLDPE), and the three storage conditions were (28.3${\pm}$1.0)$^{\circ}C$ with (15.5${\pm}$2.8)% relative humidity, (18.6${\pm}$0.5)$^{\circ}C$ with (46.6${\pm}$4.9)% RH, and (0${\pm}$2)$^{\circ}C$ with (80${\pm}$10)% RH, respectively. The moisture contents of all samples changed according to the relative storage humidity, except those of the samples packed with OPP/Al/LLDPE, which remained constant throughout the storage period. The capsaicinoids content of the red pepper powder did not change significantly for 6 months, but gradually decreased after that until about 85% of the original amount remained at the final stage of storage. The ASTA color values of all samples decreased gradually throughout the storage period. The higher the storage temperature, the more severe the deterioration. The color deterioration seemed greatly related to the existence of oxygen, as the deterioration was especially severe in the samples packed with LLDPE and B650, where the oxygen transmission rate were highest among the five packaging materials.

• 한국지반공학회논문집
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• 제18권3호
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• pp.73-85
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• 2002

본 논문에서는 비등방 압밀된 낙동강 포화모래의 비배수 반복 전단강도 거동이 연구되었으며, 등방압밀된 시료의 반복삼축시험은 비등방 압밀시료와의 비교를 위하여 수행되었다. 초기 정적 전단음력과 상대밀도의 다양한 조합하에 반복 전단강도는 고찰되었다. 음력반전과 비응력반전 모두에 대하여 반복하중을 받는 시료의 파괴는 5%의 양진폭변형율과 5%의 잔류축변형율로서 정의하였다. 비등방 압밀된 시료의 반복 전단강도는 초기 정적 전단강도에 영향을 받는 것으로 나타났다. 비등방 압밀 낙동강 모래의 반복 전단강도는 Toyoura 실리카 모래의 전단강도 보다는 크지만, Dogs Bay 카보나이트 모래의 전단강도 보다는 작게 나타났다. 실험결과와 예측결과의 비교에 의하면, 낙동강 모래의 잔류 간극수압에 대한 Hyodo 모델의 적용성이 입증되었다.

• 산업기술연구
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• 제12권
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• pp.15-23
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• 1992

This research is to investigate the effect of base roughness of footing on characteristics of load-settlement curve. Parametric experiments of small scaled model test were performed with changing the properties of base roughness of model footing; Gluing the vinyl, aluminum, sand paper, sand beneath the model footing surface. The width of model footing and relative density of soil foundation were also changed to investigate their effects on settlement characteristics of footing. The ultimate bearing capacity as well as the initial slope of load-settlement curve obtained from test results were compared with those from limit equilibrium methods proposed by Terzaghi, Hansen and Meyerhof. From test results, it was confirmed that the base roughness affected the failure mechanisms of showing different shapes of slip lines formed beneath the footing.

• 한국지진공학회:학술대회논문집
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• 한국지진공학회 2003년도 추계 학술발표회논문집
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• pp.90-97
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• 2003

The purpose of this study is to understand the dissipation pattern of excess pore pressure after liquefaction which governs the post-liquefaction behavior of liquefied sand deposits. 1-g shaking table tests were carried out on 5 different kinds of sands, all of which had high liquefaction potentials. During the tests excess pore pressure at various depths, and surface settlements were measured. The measured curve of the excess pore pressure dissipation was simulated using the solidification theory, and from the analysis of the velocity of dissipation, the dissipation pattern of excess pore pressure after liquefaction was examined. The dissipation velocity of excess pore pressure after liquefaction had a linear correlation with the effective grain size ( $D_{10}$) divided by the coefficient of uniformity ( $C_{u}$), and the increase in the initial relative density of the ground played a role in shifting this correlation curve toward an increased dissipation velocity. From the correlation, an approximate method was recommended for prediction of the dissipation curve of excess pore pressure after liquefaction in saturated sand deposits.s.s.

• 한국지반공학회논문집
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• 제22권1호
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• pp.35-44
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• 2006

일반적으로 현장지반은 대부분 일정량의 세립분을 포함하고 있으므로 세립분 함유량을 고려한 지반 거동에 관한 연구가 요구된다. 이와 더불어, 기초 지반은 하중초기단계부터 상당한 비선형 거동특성을 나타내고 있어, 응력단계에 따른 지반의 비선형성 또한 매우 중요한 고려사항이다. 본 연구에서는 일련의 실내시험을 수행하여 지반의 전단강도 및 비선형 감쇠 특성을 도출하고자 하였으며, 수정 Hyerbolic 모델을 적용하여 분석된 실트질 모래 지반의 비선형 거동특성은 실트함유량과 상대밀도에 의해 정량화되었다. 실트질 모래 시료의 응력-변형률 곡선을 도출하기 위해 세립분 함유량을 변화시켜가며 일련의 삼축압축시험이 수행되었다. 또한 비선형 특성의 정규화에 요구되는 미소변형률 구간의 초기전단탄성계수의 도출을 위해서 삼축압축시험의 시료조건과 유사한 시료에 대해 공진주시험이 수행되었다. 또한 실트함유량별로 도출된 비선형 특성치는 상대밀도의 영향이 가장 큰 것으로 나타났으며, 상대밀도 증가에 따라 파괴시의 탄성계수의 비인 f값은 감소하고, 지반강성도 감쇠율을 나타내는 9의 경우 증가하는 경향을 나타내었다. 이와 더불어 비선형 특성치를 상대밀도 $D_R$을 간극비로 환산한 절대적 간극비 $e_{sk}$에 따른 정량화 결과의 경우, $e_{sk}$의 증가에 따라 f값은 증가하고 g값은 감소하는 경향을 나타내었다.

• 한국수산과학회지
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• 제32권4호
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• pp.444-451
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• 1999

실험실에서 배양한 어린 포자체 (최대길이 0.63 cm)를 밀도 4단계로 조절하여 경남 일광연안에 양성하고, 1996년 1월부터 7월까지 생장과 생존을 조사하였다. 서로 다른 밀도로 양성한 포자체는 저밀도에서 높은 생존율을 보였다. 실험된 4개의 밀도집단 중 3개의 저밀도 집단에서 최종적으로 생존한 개체의 수는 34$\~$38 개체${\cdot}100 cm^{-2}$의 범위로 유사하였다. 그러나 가장 고밀도 집단에서는 사망률이 다른 집단에 비해 상대적으로 높아 7월 말에는 단지 21 개체${\cdot}100 cm^{-2}$ 개체만이 생존하였다. 양성 후 2개월 이전에는 각 밀도집단의 엽체의 크기는 초기 밀도가 높을 수록 작았으나, 집단간 밀도차이가 없어지는 3개월 이후로는 크기 차이가 없어졌다. 집단의 밀도가 높아질수록 엽장의 빈도분포가 오른쪽으로 심한 비대칭을 이루었다. 각 집단에서 가장 큰 10개의 크기는 언제나 저밀도 집단에서 높았다. 엽체의 크기가 클수록 상대성장률과 생존율이 높았다. 3월부터 7월까지 yield-den-sity 관계식의 기울기는 -0.060에서 -0.137의 범위였다. 이 결과들로부터 밀도가 다시마의 성장과 생존에 심각하게 영향을 미침을 알 수 있었으나, 밀도 종속적 성장과 사망유형은 육상식물의 경우와는 일치하지 않았다.

• 천문학회보
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• 제42권2호
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• pp.48.3-49
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• 2017

Interplanetary space of the solar system contains a large number of dust particles, referred to as Interplanetary Dust Particles (IDPs) cloud complex. They are observable through meteors and zodiacal lights. The relative contribution of possible sources to the IDPs cloud complex was an controversial topic, however, recent research (Yang & Ishiguro, 2015 and references therein) suggested a dominance of cometary origin. In this study, we numerically investigated the orbital evolution of cometary dust particles, with special concerns on different evolutionary tracks and its consequences according to initial orbits, size and particle shape. The effect of dust particle density and initial size-frequency distribution (SFD) were not decisive in total cloud complex mass and mass supply rate, when these physical quantities are confined by observed zodiacal light brightness and dust particle SFD at 1 au. We noticed that, if we assume the existence of fluffy aggregates discovered in the Earth's stratosphere and the coma of 67P/Churyumov-Gerasimenko, the required mass supply rate decreases significantly. We also found out that close encounters with planets (mostly Jupiter) are the dominating factor of the orbital evolution of dust particles, as the result, the lifetime of cometary dust particles are shorter than Poynting-Robertson lifetime (around 250 thousand years). As another consequence of severe close encounters, only a small fraction of cometary dust particles can be transferred into the orbit < 1 au. This effect is significant for large size particles of ${\beta}$ < 0.01. The exceptional cases are dust particles ejected from 2P/Encke and active asteroids. Because they rarely encounter with Jupiter, most dust particles ejected from those objects are governed by Poynting-Robertson effect and well transferred into the orbits of small semimajor axis. In consideration of the above effects, we directly estimated probability of mutual collisions between dust particles and concluded that mutual collisions in the IDPs cloud complex is mostly ignorable, except for the case of large sized particles from active asteroids.

• 한국수산과학회지
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• 제43권3호
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• pp.223-230
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• 2010

To compare seed collection and the growth of Anadara subcrenata in Suncheon and Boseong Bays, environmental factors and the growth of larvae and spats were investigated from August 2008 to July 2009 in commercial farming sites in both bays. The variation in water temperature in both bays was similar, but the salinity was lower in Suncheon Bay than in Boseong Bay. The chlorophyll-a content was higher in Suncheon Bay due to the large inflow of freshwater. The density and shell length of A. subcrenata larvae did not differ significantly between the two bays. However, the relative growth of shell height to shell length was significantly higher in Suncheon Bay (P<0.05). The growth of A. subcrenata spats attached to a collector was significantly faster in Suncheon Bay (P<0.05). The spats in Suncheon and Boseong Bays grew to 24.3 and 21.0 mm in shell length, respectively, within 1 year after spawning, and the shell length reached 35.6 and 34.8 mm, respectively, within 2 years of spawning. The initial spats density was higher in Boseong Bay, but the growth of spats was better in Suncheon Bay. The faster growth of A. subcrenata in Suncheon Bay can be explained by the high chlorophyll-a content in this bay. Based on the low survival (%) and slower growth rate of spats in Boseong Bay, the commercial culture density of A. subcrenata in Boseong Bay should be reduced to the optimum level of the carrying capacity.